Note that proprietary data rights apply to the point or extended source(s) that have been approved by the Time Allocation Committee (TAC), and about which the PIs have been informed by ISOC. The data rights policy as outlined in the AO- 12 documentation is applicable.
| SOURCE NAME | RA | DEC | PI | PROP ID | Open Time Proposals | TAC Data Rights Strategy |
|---|---|---|---|---|---|---|
| Galaxy | 0.000 | 0.000 | Krivonos | 1230022 | 1220022 | Data rights are allocated to the analysis of diffuse continuum and line emissions. Data rights on point sources are not a priori reserved to the PIs of this proposal. |
| Galaxy | 0.000 | 0.000 | Sunyaev | 1230021 | 1220021 | Data rights are allocated to the analysis of diffuse continuum and line emissions. Data rights on point sources are not a priori reserved to the PIs of this proposal. |
| NGC 1275 | 49.951 | 41.512 | Eckert | 1230037 | 1220037 | |
| XPer | 58.846 | 31.046 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| Orion_Eri | 74.045 | -1.196 | Diehl | 1230006 | 1220006 | Data right are awarded for the study of diffuse emission towards the Orion region (26Al, 511 keV emission and de-excitation lines) |
| Orion_BL | 80.989 | 2.781 | Diehl | 1230006 | 1220006 | Data right are awarded for the study of diffuse emission towards the Orion region (26Al, 511 keV emission and de-excitation lines) |
| Orion_OB | 81.524 | -2.324 | Diehl | 1230006 | 1220006 | Data right are awarded for the study of diffuse emission towards the Orion region (26Al, 511 keV emission and de-excitation lines) |
| 4U 0614+09 | 94.280 | 9.137 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Cen X-4 | 224.591 | -31.669 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Scorpius-Centaurus | 226.468 | -29.398 | Krause | 1230035 | 1220035 | Data right are awarded for the study of diffuse emission towards the Orion region (26Al, 511 keV emission and de-excitation lines) |
| Scorpius-Centaurus | 234.476 | -23.916 | Krause | 1230035 | 1220035 | Data right are awarded for the study of diffuse emission towards the Orion region (26Al, 511 keV emission and de-excitation lines) |
| UW CrB | 241.441 | 25.863 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Sco X-1 | 244.979 | -15.640 | Revnivtsev | 1230027 | 1220027 | |
| ScoX-1 | 244.979 | -15.640 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| GX340+0 | 251.449 | -45.611 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| MAXI J1647-227 | 251.960 | -22.750 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| MAXI J1647-227 | 251.960 | -22.750 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | |
| Her X-1 | 254.458 | 35.342 | Staubert | 1230032 | 1220032 | |
| MAXI J1659-152 | 254.792 | -15.268 | Wilms | 1230018 | 1220035 1220009 | |
| XTE J1701-462 | 255.244 | -46.186 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1701-407 | 255.435 | -40.856 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1701-407 | 255.435 | -40.858 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| MXB 1658-298 | 255.527 | -29.946 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| H1658-298 | 255.527 | -29.946 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U1700-377 | 255.987 | -37.844 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| GX349+2 | 256.435 | -36.423 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U 1702-429 | 256.564 | -43.036 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| H1702-429 | 256.564 | -43.036 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U 1708-23 | 257.096 | -22.803 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1705-32 | 257.227 | -32.316 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1705-32 | 257.227 | -32.316 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1705-44 | 257.227 | -44.102 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| H1705-440 | 257.227 | -44.102 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| IGR J17091-3624 | 257.279 | -36.407 | Wilms | 1230018 | 1220035 1220009 | |
| XTE J1709-267 | 257.376 | -26.657 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1709-267 | 257.376 | -26.658 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1710-281 | 257.551 | -28.132 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1710-281 | 257.551 | -28.132 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1711.6-3808 | 257.892 | -38.122 | Wilms | 1230018 | 1220035 1220009 | |
| 4U 1708-40 | 258.096 | -40.843 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1708-40 | 258.099 | -40.843 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1712.6-3739 | 258.142 | -37.643 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1712.6-3739 | 258.142 | -37.643 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 2S 1711-339 | 258.582 | -34.046 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1711-34 | 258.582 | -34.046 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| RX J1718.4-4029 | 259.600 | -40.492 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| RX J1718.4-4029 | 259.601 | -40.492 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1H 1715-321 | 259.697 | -32.178 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1H 1715-321 | 259.698 | -32.178 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| MXB 1716-31 | 259.750 | -31.877 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17191-2821 | 259.808 | -28.326 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17191-2821 | 259.813 | -28.299 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GRS 1716-249 | 259.904 | -25.018 | Wilms | 1230018 | 1220035 1220009 | |
| XTE J1720-318 | 259.975 | -31.749 | Wilms | 1230018 | 1220035 1220009 | |
| XTE J1723-376 | 260.908 | -37.662 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1723-376 | 260.911 | -37.662 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17254-3257 | 261.356 | -32.955 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17254-3257 | 261.356 | -32.955 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U1722-30 | 261.888 | -30.803 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U 1722-30 | 261.888 | -30.802 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1722-30 | 261.889 | -30.802 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17285-2922 | 262.171 | -29.382 | Wilms | 1230018 | 1220035 1220009 | |
| 3A1728-169 | 262.934 | -16.962 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| GX 354-0 | 262.989 | -33.835 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1728-34 | 262.991 | -33.834 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GX354-0 | 262.992 | -33.835 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U1730-335 | 263.350 | -33.388 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| MXB 1730-335 | 263.350 | -33.388 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| MXB 1730-335 | 263.353 | -33.389 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| KS 1730-312 | 263.383 | -31.217 | Wilms | 1230018 | 1220035 1220009 | |
| KS 1731-260 | 263.556 | -26.088 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| KS 1731-260 | 263.556 | -26.088 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Swift J1734.5-3027 | 263.602 | -30.398 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Swift J1734.5-3027 | 263.613 | -30.453 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17353-3539 | 263.846 | -35.670 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1RXH J173523.7-354013 | 263.846 | -35.670 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1732-304 | 263.945 | -30.483 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1732-304 | 263.948 | -30.482 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17364-2711 | 264.117 | -27.199 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17364-2711 | 264.117 | -27.199 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17380-3749 | 264.475 | -37.783 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1735-269 | 264.571 | -26.994 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1735-269 | 264.571 | -26.994 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U1735-444 | 264.742 | -44.450 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U 1735-444 | 264.743 | -44.450 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1739-285 | 264.975 | -28.496 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1739-285 | 264.975 | -28.496 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GRS 1737-31 | 265.025 | -31.033 | Wilms | 1230018 | 1220035 1220009 | |
| SLX 1737-282 | 265.162 | -28.297 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1737-282 | 265.178 | -28.302 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GRS 1739-278 | 265.665 | -27.748 | Wilms | 1230018 | 1220035 1220009 | |
| KS 1741-293 | 266.213 | -29.355 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| KS 1741-293 | 266.233 | -29.352 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XMM J174457-2850.3 | 266.239 | -28.839 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XMM J174457-2850.3 | 266.258 | -28.838 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GRANAT 1741.9-2853 | 266.260 | -28.914 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GRS 1741.9-2853 | 266.260 | -28.914 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Swift J174510.8-262411 | 266.295 | -26.403 | Wilms | 1230018 | 1220035 1220009 | |
| AX J1745.6-2901 | 266.399 | -29.026 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| AX J1745.6-2901 | 266.401 | -29.026 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1A 1742-289 | 266.404 | -29.019 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1A 1742-289 | 266.404 | -29.019 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SGR A* | 266.417 | -29.008 | Wilms | 1230009 | 1220009 | |
| 1A 1742-294 | 266.522 | -29.515 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1A 1742-294 | 266.523 | -29.515 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGRJ17464-3213 | 266.567 | -32.234 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| H 1743-322 | 266.567 | -32.234 | Wilms | 1230018 | 1220035 1220009 | |
| GX 0.2-0.2 | 266.761 | -28.883 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1747.0-2853 | 266.761 | -28.883 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17464-2811 | 266.817 | -28.180 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17464-2811 | 266.817 | -28.180 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17473-2721 | 266.825 | -27.344 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17473-2721 | 266.825 | -27.344 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1744-300 | 266.856 | -30.045 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1744-300 | 266.856 | -30.045 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1744-299 | 266.858 | -29.999 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX 1744-299 | 266.858 | -30.021 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GX 3+1 | 266.983 | -26.564 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17480-2446 | 266.999 | -24.767 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1748-288 | 267.000 | -28.483 | Wilms | 1230018 | 1220035 1220009 | |
| XTE J1748-288 | 267.000 | -28.483 | Wilms | 1230018 | 1220035 1220009 | |
| IGR J17480-2446 | 267.020 | -24.780 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| EXO 1745-248 | 267.022 | -24.780 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| EXO 1745-248 | 267.022 | -24.780 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SWIFT J174805.3-244637 | 267.022 | -24.777 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Sw J174805.3-244637 | 267.023 | -24.777 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1A1744-36 | 267.055 | -36.132 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 1A 1744-361 | 267.055 | -36.132 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1A 1744-361 | 267.080 | -36.121 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1748.9-2021 | 267.217 | -20.359 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1748.9-2021 | 267.217 | -20.359 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Swift J1749.4-2807 | 267.383 | -28.135 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Swift J1749.4-2807 | 267.383 | -28.135 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SLX1746-331 | 267.461 | -33.199 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| IGR J17498-2921 | 267.481 | -29.322 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17498-2921 | 267.481 | -29.322 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1746-37 | 267.553 | -37.052 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1746-37 | 267.553 | -37.052 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1H1746-370 | 267.554 | -37.051 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| SAX J1750.8-2900 | 267.600 | -29.038 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1750.8-2900 | 267.602 | -29.038 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| EXO 1747-214 | 267.602 | -21.422 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| EXO 1747-214 | 267.607 | -21.422 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GRS 1747-312 | 267.690 | -31.292 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GRS 1747-312 | 267.695 | -31.275 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17511-3057 | 267.786 | -30.962 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17511-3057 | 267.788 | -30.961 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1752-223 | 268.063 | -22.343 | Wilms | 1230018 | 1220035 1220009 | |
| SAX J1752.3-3138 | 268.100 | -31.628 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1752.3-3138 | 268.100 | -31.628 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1753.5-2349 | 268.383 | -23.821 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1753.5-2349 | 268.383 | -23.821 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| AX J1754.2-2754 | 268.561 | -27.910 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| AX J1754.2-2754 | 268.561 | -27.910 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1755-324 | 268.887 | -32.495 | Wilms | 1230018 | 1220035 1220009 | |
| H1755-338 | 269.667 | -33.808 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U 1755-338 | 269.667 | -33.808 | Wilms | 1230018 | 1220035 1220009 | |
| IGR J17597-2201 | 269.940 | -22.027 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J17597-2201 | 269.940 | -22.028 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GX5-1 | 270.284 | -25.079 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| GRS 1758-258 | 270.302 | -25.743 | Hirsch | 1230025 | 1220009 | |
| GX9+1 | 270.384 | -20.529 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 1RXS J180408.9-34205 | 271.034 | -34.347 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 1RXS J180408.9-342058 | 271.038 | -34.349 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1806.5-2215 | 271.642 | -22.252 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1806.5-2215 | 271.642 | -22.252 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 2S 1803-245 | 271.709 | -24.588 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 2S 1803-245 | 271.711 | -24.591 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTEJ1807-294 | 271.749 | -29.408 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| SAX J1808.4-3658 | 272.115 | -36.979 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1810-189 | 272.587 | -19.070 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1810-189 | 272.608 | -19.070 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1810.8-2609 | 272.685 | -26.150 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SAX J1810.8-2609 | 272.685 | -26.150 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1814-338 | 273.413 | -33.773 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XTE J1814-338 | 273.413 | -33.773 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GX 13+1 | 273.631 | -17.157 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GX 13+1 | 273.631 | -17.157 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | |
| GX 13+1 | 273.631 | -17.157 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 4U 1812-12 | 273.776 | -12.096 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GX 17+2 | 274.006 | -14.036 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| GX17+2 | 274.006 | -14.036 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| XTE J1818-245 | 274.603 | -24.538 | Wilms | 1230018 | 1220035 1220009 | |
| V4641 Sgr | 274.840 | -25.407 | Wilms | 1230018 | 1220035 1220009 | |
| 4U 1820-303 | 275.919 | -30.361 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| H1820-303 | 275.919 | -30.361 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U 1820-303 | 275.919 | -30.361 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| AX J1824.5-2451 | 276.123 | -24.850 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| AX J1824.5-2451 | 276.125 | -24.850 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| IGR J18245-2452 | 276.135 | -24.869 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 3A1822-371 | 276.445 | -37.105 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| SAX J1828.5-1037 | 277.142 | -10.617 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Ginga 1826-24 | 277.368 | -23.797 | Chenevez | 1230039 | 1220009 1220035 | Data rights are granted to any burst whose flux remains >10% above the pre-burst level for more than 5 minutes, on the accepted list of targets. Data rights on shorter bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, PropID: 1220010). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| Ginga1826-24 | 277.368 | -23.791 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| GS 1826-24 | 277.368 | -23.797 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| XB 1832-330 | 278.932 | -32.991 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| 3A1850-087 | 283.270 | -8.705 | Watanabe | 1230007 | 1220035 1220037 1220009 | Data rights are granted on unknown/unpredicted gamma-ray lines with SPI. The known lines are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1156 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun) |
| 4U 1850-086 | 283.270 | -8.705 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| HETE J1900.1-2455 | 285.036 | -24.920 | Sanchez-Fernandez | 1230010 | 1220006 1220035 1220009 1220032 | Data rights on any bursts whose flux remains >10% above the pre-burst level for more than 5 minutes, are granted to another accepted proposal (PI: Chenevez, PropID: 1220039). If both kind of bursts (shorter and longer than 5 minutes) will be detected from the same source, data rights on the persistent emission of the correspondent sources will be shared among the two proposals. |
| SOURCE NAME | RA | DEC | PI | PROP ID | Open Time Proposals | TAC Data Rights Strategy |
|---|---|---|---|---|---|---|
| SN Ia | 0.000 | 0.000 | Diehl | 1240007 | 1240007 | |
| NEW | 0.000 | 0.000 | Falanga | 1240014 | 1240014 | |
| GRB | 0.000 | 0.000 | Gotz | 1240028 | 1240028 | |
| supernova | 0.000 | 0.000 | Grebenev | 1240037 | 1240037 | |
| new AXP/SGR | 0.000 | 0.000 | Götz | 1240026 | 1240026 | |
| Classical Nova | 0.000 | 0.000 | Hernanz | 1240018 | 1240018 | |
| FermiTransient1 | 0.000 | 0.000 | Hill | 1240033 | 1240033 | |
| Gamma-ray burst | 0.000 | 0.000 | Hurley | 1240005 | 1240005 | |
| SNIa Early Obs | 0.000 | 0.000 | Jordi | 1240025 | 1240025 | |
| New Transient Pulsar | 0.000 | 0.000 | Kreykenbohm | 1240013 | 1240013 | |
| NEW AXP | 0.000 | 0.000 | Kuiper | 1240010 | 1240010 | |
| TDE | 0.000 | 0.000 | Panessa | 1240012 | 1240012 | |
| New BH Transient | 0.000 | 0.000 | Rodriguez | 1240027 | 1240027 | |
| GRB outside the FoV | 0.000 | 0.000 | Savchenko | 1240030 | 1240030 | |
| Black Hole Transient | 0.000 | 0.000 | Wilms | 1240009 | 1240009 | |
| Black Hole Transient | 0.000 | 0.000 | Wilms | 1240009 | 1240009 | |
| PMN J0017-0512 | 4.399 | -5.212 | Pian | 1240011 | 1240011 | |
| GRB041219 | 6.112 | 62.843 | Hanlon | 1240036 | 1240036 | |
| IGR J00291+5934 | 7.262 | 59.572 | Campana | 1240034 | 1240034 | |
| IGR J00291+5934 | 7.263 | 59.572 | Falanga | 1240014 | 1240014 | |
| RBS 0076 | 8.393 | -19.359 | Pian | 1240011 | 1240011 | |
| 1ES 0033+595 | 8.969 | 59.835 | Pian | 1240011 | 1240011 | |
| XMMi J003833.3+40213 | 9.639 | 40.359 | Kuiper | 1240010 | 1240010 | |
| AX J0049-729 | 12.275 | -72.847 | Kreykenbohm | 1240013 | 1240013 | |
| PKS 0048-097 | 12.672 | -9.485 | Pian | 1240011 | 1240011 | |
| AX J0051-722 | 12.732 | -72.232 | Kreykenbohm | 1240013 | 1240013 | |
| PKS 0048-071 | 12.784 | -6.834 | Pian | 1240011 | 1240011 | |
| 2E 0050.1-7247 | 12.972 | -72.530 | Kreykenbohm | 1240013 | 1240013 | |
| RX J0052.1-7319 | 13.058 | -73.320 | Kreykenbohm | 1240013 | 1240013 | |
| RX J0052.9-7158 | 13.230 | -71.968 | Kreykenbohm | 1240013 | 1240013 | |
| RX J0053.8-7226 | 13.479 | -72.446 | Kreykenbohm | 1240013 | 1240013 | |
| XTE J0055-724 | 13.734 | -72.441 | Kreykenbohm | 1240013 | 1240013 | |
| RX J0059.2-7138 | 14.797 | -71.646 | Kreykenbohm | 1240013 | 1240013 | |
| CXO J010043.1-721134 | 15.180 | -72.193 | Kuiper | 1240010 | 1240010 | |
| AX J0105-722 | 16.287 | -72.196 | Kreykenbohm | 1240013 | 1240013 | |
| CXOU 010043-7211 | 17.679 | -72.193 | Götz | 1240026 | 1240026 | |
| PSR J0111-7317 | 17.785 | -73.279 | Kreykenbohm | 1240013 | 1240013 | |
| S2 0109+22 | 18.024 | 22.744 | Pian | 1240011 | 1240011 | |
| 4C 31.03 | 18.210 | 32.138 | Pian | 1240011 | 1240011 | |
| RX J0117.6-7330 | 19.422 | -73.514 | Kreykenbohm | 1240013 | 1240013 | |
| PKS 0116-219 | 19.739 | -21.692 | Pian | 1240011 | 1240011 | |
| PKS 0118-272 | 20.132 | -27.024 | Pian | 1240011 | 1240011 | |
| 1ES 0120+340 | 20.785 | 34.347 | Pian | 1240011 | 1240011 | |
| B3 0133+388 | 24.135 | 39.100 | Pian | 1240011 | 1240011 | |
| DA 055 | 24.244 | 47.858 | Pian | 1240011 | 1240011 | |
| TXS 0141+268 | 26.140 | 27.084 | Pian | 1240011 | 1240011 | |
| PKS 0142-278 | 26.264 | -27.560 | Pian | 1240011 | 1240011 | |
| 4U 0142+614 | 26.592 | 61.751 | Götz | 1240026 | 1240026 | |
| 4U 0142+61 | 26.593 | 61.751 | Kuiper | 1240010 | 1240010 | |
| PKS 0202-17 | 31.240 | -17.022 | Pian | 1240011 | 1240011 | |
| PKS 0208-512 | 32.692 | -51.017 | Pian | 1240011 | 1240011 | |
| PKS 0208-512 | 32.692 | -51.017 | Zhang | 1240001 | 1240001 | |
| CGRaBS J0211+1051 | 32.805 | 10.860 | Pian | 1240011 | 1240011 | |
| TXS 0214+517 | 34.391 | 51.966 | Pian | 1240011 | 1240011 | |
| PKS 0215+015 | 34.454 | 1.747 | Pian | 1240011 | 1240011 | |
| TXS 0218+357 | 35.273 | 35.937 | Pian | 1240011 | 1240011 | |
| 3C 66A | 35.665 | 43.036 | Pian | 1240011 | 1240011 | |
| PKS 0227-369 | 37.368 | -36.732 | Pian | 1240011 | 1240011 | |
| 1ES 0229+200 | 38.203 | 20.288 | Pian | 1240011 | 1240011 | |
| PKS 0235-618 | 39.222 | -61.604 | Pian | 1240011 | 1240011 | |
| 4C +28.07 | 39.468 | 28.802 | Pian | 1240011 | 1240011 | |
| PKS 0235+164 | 39.662 | 16.616 | Pian | 1240011 | 1240011 | |
| PKS 0244-470 | 41.500 | -46.855 | Pian | 1240011 | 1240011 | |
| PKS 0301-243 | 45.860 | -24.120 | Pian | 1240011 | 1240011 | |
| 1H 0323+342 | 51.172 | 34.179 | Pian | 1240011 | 1240011 | |
| 1H 0323+022 | 51.558 | 2.421 | Pian | 1240011 | 1240011 | |
| PKS 0332-403 | 53.557 | -40.140 | Pian | 1240011 | 1240011 | |
| PKS 0347-211 | 57.491 | -21.047 | Pian | 1240011 | 1240011 | |
| PKS 0402-362 | 60.974 | -36.084 | Pian | 1240011 | 1240011 | |
| PKS 0405-385 | 61.747 | -38.441 | Pian | 1240011 | 1240011 | |
| PMN J0413-5332 | 63.322 | -53.534 | Pian | 1240011 | 1240011 | |
| 1H 0414+009 | 64.224 | 1.082 | Pian | 1240011 | 1240011 | |
| SGR 0418+5729 | 64.641 | 57.540 | Kuiper | 1240010 | 1240010 | |
| SGR 0418+5729 | 64.642 | 57.540 | Götz | 1240026 | 1240026 | |
| XTE J0421+560 | 64.925 | 56.000 | Motta | 1240015 | 1240015 | |
| GRO J0422+32 | 65.428 | 32.909 | Motta | 1240015 | 1240015 | |
| GRO J0422+32 | 65.429 | 32.908 | Wilms | 1240009 | 1240009 | |
| GRO J0422+32 | 65.429 | 32.908 | Wilms | 1240009 | 1240009 | |
| PKS 0420-01 | 65.816 | -1.342 | Pian | 1240011 | 1240011 | |
| PKS 0426-380 | 67.168 | -37.939 | Pian | 1240011 | 1240011 | |
| NRAO 0190 | 70.661 | -0.295 | Pian | 1240011 | 1240011 | |
| PKS 0447-439 | 72.353 | -43.836 | Pian | 1240011 | 1240011 | |
| PKS 0454-234 | 74.263 | -23.414 | Pian | 1240011 | 1240011 | |
| SGR 0501+4516 | 75.265 | 45.272 | Götz | 1240026 | 1240026 | |
| SGR 0501+4516 | 75.283 | 45.275 | Kuiper | 1240010 | 1240010 | |
| RX J0502.9-6626 | 75.715 | -66.440 | Kreykenbohm | 1240013 | 1240013 | |
| 1ES 0502+675 | 76.984 | 67.623 | Pian | 1240011 | 1240011 | |
| PKS 0516-621 | 79.187 | -62.118 | Pian | 1240011 | 1240011 | |
| PKS 0521-36 | 80.742 | -36.459 | Pian | 1240011 | 1240011 | |
| SGR 0526-66 | 81.503 | -66.076 | Kuiper | 1240010 | 1240010 | |
| SGR 0525-66 | 81.504 | -66.077 | Götz | 1240026 | 1240026 | |
| RX J0529.8-6556 | 82.452 | -65.948 | Kreykenbohm | 1240013 | 1240013 | |
| PKS B0528+134 | 82.735 | 13.532 | Pian | 1240011 | 1240011 | |
| EXO 053109-6609.2 | 82.805 | -66.118 | Kreykenbohm | 1240013 | 1240013 | |
| PMN J0531-4827 | 82.994 | -48.460 | Pian | 1240011 | 1240011 | |
| PMN J0532+0732 | 83.162 | 7.545 | Pian | 1240011 | 1240011 | |
| RX J0535.6-6651 | 83.919 | -66.865 | Kreykenbohm | 1240013 | 1240013 | |
| PKS 0537-441 | 84.710 | -44.086 | Pian | 1240011 | 1240011 | |
| AX J0544.1-7100 | 86.026 | -71.014 | Kreykenbohm | 1240013 | 1240013 | |
| PKS 0548-322 | 87.670 | -32.272 | Pian | 1240011 | 1240011 | |
| H 0557-385 | 89.508 | -38.335 | Pian | 1240011 | 1240011 | |
| A0620-003 | 95.683 | 0.346 | Wilms | 1240009 | 1240009 | |
| A0620-003 | 95.683 | 0.346 | Wilms | 1240009 | 1240009 | |
| 1A 0620-00 | 95.685 | -0.346 | Motta | 1240015 | 1240015 | |
| 1A 0620-00 | 95.685 | -0.346 | Rodriguez | 1240027 | 1240027 | |
| 1A0620-00 | 95.685 | -0.346 | Rodriguez | 1240027 | 1240027 | |
| B2 0619+33 | 95.718 | 33.436 | Pian | 1240011 | 1240011 | |
| 1ES 0647+250 | 102.694 | 25.050 | Pian | 1240011 | 1240011 | |
| GB6 J0654+5042 | 103.595 | 50.707 | Pian | 1240011 | 1240011 | |
| CJ2 0650+453 | 103.599 | 45.240 | Pian | 1240011 | 1240011 | |
| PKS 0700-661 | 105.130 | -66.179 | Pian | 1240011 | 1240011 | |
| GB6 J0712+5033 | 108.182 | 50.556 | Pian | 1240011 | 1240011 | |
| 1FGL J0714.0+1935 | 108.482 | 19.583 | Pian | 1240011 | 1240011 | |
| TXS 0716+332 | 109.831 | 33.119 | Pian | 1240011 | 1240011 | |
| S5 0716+71 | 110.473 | 71.343 | Pian | 1240011 | 1240011 | |
| 4C 14.23 | 111.320 | 14.420 | Pian | 1240011 | 1240011 | |
| 3A 0726-260 | 112.222 | -26.108 | Kreykenbohm | 1240013 | 1240013 | |
| PKS 0727-11 | 112.580 | -11.687 | Pian | 1240011 | 1240011 | |
| PKS B0735+178 | 114.531 | 17.705 | Pian | 1240011 | 1240011 | |
| 1FGL J0742.2+5443 | 115.666 | 54.740 | Pian | 1240011 | 1240011 | |
| PKS 0805-07 | 122.065 | -7.853 | Pian | 1240011 | 1240011 | |
| 1ES 0806+524 | 122.455 | 52.316 | Pian | 1240011 | 1240011 | |
| PMN J0811+0237 | 123.008 | 2.626 | Pian | 1240011 | 1240011 | |
| RX J0812.4-3114 | 123.118 | -31.248 | Kreykenbohm | 1240013 | 1240013 | |
| S4 0814+425 | 124.567 | 42.379 | Pian | 1240011 | 1240011 | |
| TXS 0820+560 | 126.197 | 55.879 | Pian | 1240011 | 1240011 | |
| PKS 0823-223 | 126.507 | -22.508 | Pian | 1240011 | 1240011 | |
| B2 0827+24 | 127.720 | 24.183 | Pian | 1240011 | 1240011 | |
| Ginga 0834-430 | 128.979 | -43.185 | Kreykenbohm | 1240013 | 1240013 | |
| S5 0836+71 | 130.352 | 70.895 | Pian | 1240011 | 1240011 | |
| OJ 287 | 133.704 | 20.109 | Pian | 1240011 | 1240011 | |
| 3EG J0903-3531 | 136.200 | -35.200 | Pian | 1240011 | 1240011 | |
| PKS B0906+015 | 137.295 | 1.360 | Pian | 1240011 | 1240011 | |
| PKS 0907+022 | 137.416 | 2.001 | Pian | 1240011 | 1240011 | |
| S4 0917+44 | 140.244 | 44.698 | Pian | 1240011 | 1240011 | |
| XTE J0929-314 | 142.334 | -31.384 | Falanga | 1240014 | 1240014 | |
| PMN J0948+0022 | 147.239 | 0.374 | Pian | 1240011 | 1240011 | |
| S4 0954+55 | 149.409 | 55.383 | Pian | 1240011 | 1240011 | |
| 1FGL J1012.7+2440 | 153.172 | 24.656 | Pian | 1240011 | 1240011 | |
| GRS 1009-45 | 153.400 | -45.076 | Wilms | 1240009 | 1240009 | |
| GRS 1009-45 | 153.400 | -45.076 | Wilms | 1240009 | 1240009 | |
| GRS 1009-45 | 153.401 | -45.076 | Motta | 1240015 | 1240015 | |
| 1ES 1011+496 | 153.768 | 49.434 | Pian | 1240011 | 1240011 | |
| PMN J1016+0512 | 154.013 | 5.217 | Pian | 1240011 | 1240011 | |
| 1ES 1028+511 | 157.827 | 50.894 | Pian | 1240011 | 1240011 | |
| S4 1030+61 | 158.464 | 60.852 | Pian | 1240011 | 1240011 | |
| 4U 1036-56 | 159.398 | -56.803 | Kreykenbohm | 1240013 | 1240013 | |
| 1E 1048.1-5937 | 162.529 | -59.889 | Götz | 1240026 | 1240026 | |
| 1E 1048.1-5937 | 162.537 | -59.889 | Kuiper | 1240010 | 1240010 | |
| 1FGL J1053.6+4927 | 163.434 | 49.499 | Pian | 1240011 | 1240011 | |
| 1FGL J1054.5+2212 | 163.628 | 22.182 | Pian | 1240011 | 1240011 | |
| PKS 1055+018 | 164.623 | 1.566 | Pian | 1240011 | 1240011 | |
| RX J1058.6+5628 | 164.657 | 56.470 | Pian | 1240011 | 1240011 | |
| PKS 1057-79 | 164.680 | -80.065 | Pian | 1240011 | 1240011 | |
| 1ES 1101-232 | 165.907 | -23.492 | Pian | 1240011 | 1240011 | |
| Mkn 421 | 166.114 | 38.209 | Pian | 1240011 | 1240011 | |
| Mrk 421 | 166.114 | 38.209 | Kreikenbohm | 1240032 | 1240032 | |
| RBS 0958 | 169.276 | 20.236 | Pian | 1240011 | 1240011 | |
| XTE J1118+480 | 169.545 | 48.037 | Motta | 1240015 | 1240015 | |
| XTE J1118+480 | 169.545 | 48.037 | Rodriguez | 1240027 | 1240027 | |
| XTE J1118+480 | 169.545 | 48.037 | Rodriguez | 1240027 | 1240027 | |
| XTE J1118+480 | 169.546 | 48.037 | Wilms | 1240009 | 1240009 | |
| XTE J1118+480 | 169.546 | 48.037 | Wilms | 1240009 | 1240009 | |
| PKS 1118-056 | 170.355 | -5.899 | Pian | 1240011 | 1240011 | |
| GS 1124-68 | 171.611 | -68.676 | Motta | 1240015 | 1240015 | |
| GS 1124-684 | 171.611 | -68.676 | Rodriguez | 1240027 | 1240027 | |
| GS 1124-684 | 171.611 | -68.676 | Rodriguez | 1240027 | 1240027 | |
| GRS 1124-684 | 171.612 | -68.676 | Wilms | 1240009 | 1240009 | |
| GRS 1124-684 | 171.612 | -68.676 | Wilms | 1240009 | 1240009 | |
| PKS 1124-186 | 171.768 | -18.955 | Pian | 1240011 | 1240011 | |
| PKS 1127-14 | 172.531 | -14.824 | Pian | 1240011 | 1240011 | |
| Mkn 180 | 174.110 | 70.158 | Pian | 1240011 | 1240011 | |
| BWE 1133+6753 | 174.126 | 67.618 | Pian | 1240011 | 1240011 | |
| PKS 1144-379 | 176.756 | -38.203 | Pian | 1240011 | 1240011 | |
| H 1145-619 | 177.000 | -62.207 | Kreykenbohm | 1240013 | 1240013 | |
| 4C 29.45 | 179.883 | 29.245 | Pian | 1240011 | 1240011 | |
| RBS 1093 | 184.470 | 30.117 | Pian | 1240011 | 1240011 | |
| PG 1218+304 | 185.341 | 30.177 | Pian | 1240011 | 1240011 | |
| ON 231 | 185.382 | 28.233 | Pian | 1240011 | 1240011 | |
| PKS 1222+21 | 186.227 | 21.380 | Pian | 1240011 | 1240011 | |
| 3C 273 | 187.278 | 2.052 | Pian | 1240011 | 1240011 | |
| GB6 J1239+0443 | 189.886 | 4.718 | Pian | 1240011 | 1240011 | |
| PKS 1244-255 | 191.695 | -25.797 | Pian | 1240011 | 1240011 | |
| PG 1246+586 | 192.078 | 58.341 | Pian | 1240011 | 1240011 | |
| TXS 1250+532 | 193.300 | 53.020 | Pian | 1240011 | 1240011 | |
| 3C 279 | 194.050 | -5.789 | Pian | 1240011 | 1240011 | |
| MAXI J1305-704 | 196.731 | -70.450 | Motta | 1240015 | 1240015 | |
| OP 313 | 197.619 | 32.346 | Pian | 1240011 | 1240011 | |
| TXS 1310+487 | 198.181 | 48.475 | Pian | 1240011 | 1240011 | |
| Cen A | 201.365 | -43.019 | Steinle | 1240003 | 1240003 | |
| PKS 1329-049 | 203.019 | -5.162 | Pian | 1240011 | 1240011 | |
| 1FGL J1333.2+5056 | 203.474 | 50.960 | Pian | 1240011 | 1240011 | |
| B3 1343+451 | 206.388 | 44.883 | Pian | 1240011 | 1240011 | |
| PKS 1352-104 | 208.694 | -10.684 | Pian | 1240011 | 1240011 | |
| Swift J1357.2-0933 | 209.320 | -9.320 | Motta | 1240015 | 1240015 | |
| GS 1354-645 | 209.540 | -64.735 | Motta | 1240015 | 1240015 | |
| GS 1354-64 | 209.542 | -64.735 | Wilms | 1240009 | 1240009 | |
| GS 1354-64 | 209.542 | -64.735 | Wilms | 1240009 | 1240009 | |
| PKS 1406-076 | 212.235 | -7.874 | Pian | 1240011 | 1240011 | |
| 1E 1415.6+2557 | 214.486 | 25.724 | Pian | 1240011 | 1240011 | |
| H 1417-624 | 215.304 | -62.698 | Kreykenbohm | 1240013 | 1240013 | |
| PKS 1424+240 | 216.752 | 23.800 | Pian | 1240011 | 1240011 | |
| PKS 1424-41 | 216.985 | -42.105 | Pian | 1240011 | 1240011 | |
| 1ES 1426+428 | 217.135 | 42.674 | Pian | 1240011 | 1240011 | |
| 1ES 1440+122 | 220.701 | 12.011 | Pian | 1240011 | 1240011 | |
| PKS 1454-354 | 224.361 | -35.653 | Pian | 1240011 | 1240011 | |
| Cen X-4 | 224.592 | -31.669 | Campana | 1240034 | 1240034 | |
| PKS 1502+106 | 226.104 | 10.494 | Pian | 1240011 | 1240011 | |
| PKS 1502+036 | 226.277 | 3.442 | Pian | 1240011 | 1240011 | |
| PKS 1508-05 | 227.723 | -5.719 | Pian | 1240011 | 1240011 | |
| PKS 1510-089 | 228.211 | -9.100 | Pian | 1240011 | 1240011 | |
| Ap Lib | 229.424 | -24.372 | Pian | 1240011 | 1240011 | |
| TXS 1520+319 | 230.542 | 31.737 | Pian | 1240011 | 1240011 | |
| 4U 1524-617 | 232.070 | -61.883 | Motta | 1240015 | 1240015 | |
| A 1524-617 | 232.071 | -61.883 | Wilms | 1240009 | 1240009 | |
| A 1524-617 | 232.071 | -61.883 | Wilms | 1240009 | 1240009 | |
| Swift J1539.2-6227 | 234.800 | -62.467 | Motta | 1240015 | 1240015 | |
| 1ES 1544+820 | 235.067 | 81.918 | Pian | 1240011 | 1240011 | |
| GB6 J1542+6129 | 235.737 | 61.499 | Pian | 1240011 | 1240011 | |
| MAXI J1543-564 | 235.823 | -56.414 | Motta | 1240015 | 1240015 | |
| XTE J1543-568 | 236.008 | -56.712 | Kreykenbohm | 1240013 | 1240013 | |
| 4U 1543-475 | 236.786 | -47.669 | Motta | 1240015 | 1240015 | |
| 4U 1543-475 | 236.788 | -47.669 | Wilms | 1240009 | 1240009 | |
| 4U 1543-475 | 236.788 | -47.669 | Wilms | 1240009 | 1240009 | |
| 1E 1547.0–5408 | 237.729 | -54.322 | Götz | 1240026 | 1240026 | |
| 1E 1547.0-5408 | 237.730 | -54.317 | Kuiper | 1240010 | 1240010 | |
| XTE J1550-564 | 237.745 | -56.477 | Motta | 1240015 | 1240015 | |
| XTE J1550-564 | 237.745 | -56.474 | Rodriguez | 1240027 | 1240027 | |
| XTE J1550-564 | 237.745 | -56.474 | Rodriguez | 1240027 | 1240027 | |
| XTE J1550-564 | 237.746 | -56.477 | Wilms | 1240009 | 1240009 | |
| XTE J1550-564 | 237.746 | -56.477 | Wilms | 1240009 | 1240009 | |
| PKS 1551+130 | 238.386 | 12.948 | Pian | 1240011 | 1240011 | |
| PG 1553+113 | 238.930 | 11.190 | Pian | 1240011 | 1240011 | |
| 4U 1608-52 | 243.179 | -52.423 | Campana | 1240034 | 1240034 | |
| PSR J1622-4950 | 245.687 | -49.848 | Götz | 1240026 | 1240026 | |
| PSR J1622-4950 | 245.687 | -49.848 | Kuiper | 1240010 | 1240010 | |
| PKS 1622-253 | 246.445 | -25.461 | Pian | 1240011 | 1240011 | |
| PKS 1622-29 | 246.526 | -29.857 | Pian | 1240011 | 1240011 | |
| 4U 1630-472 | 248.500 | -47.394 | Wilms | 1240009 | 1240009 | |
| 4U 1630-472 | 248.500 | -47.394 | Wilms | 1240009 | 1240009 | |
| 4C 38.41 | 248.815 | 38.134 | Pian | 1240011 | 1240011 | |
| SGR 1627-41 | 248.966 | -47.590 | Götz | 1240026 | 1240026 | |
| SGR 1627-41 | 248.967 | -47.587 | Kuiper | 1240010 | 1240010 | |
| IGR J16358-4726 | 248.974 | -47.428 | Kreykenbohm | 1240013 | 1240013 | |
| CXO J164710.2-455216 | 251.792 | -45.871 | Götz | 1240026 | 1240026 | |
| CXO J164710.2-455216 | 251.792 | -45.871 | Kuiper | 1240010 | 1240010 | |
| XTE J1650-500 | 252.504 | -49.962 | Motta | 1240015 | 1240015 | |
| XTE J1650-500 | 252.504 | -49.962 | Rodriguez | 1240027 | 1240027 | |
| XTE J1650-500 | 252.504 | -49.962 | Rodriguez | 1240027 | 1240027 | |
| XTE J1650-500 | 252.504 | -49.962 | Wilms | 1240009 | 1240009 | |
| XTE J1650-500 | 252.504 | -49.962 | Wilms | 1240009 | 1240009 | |
| XTE J1652-453 | 253.085 | -45.344 | Motta | 1240015 | 1240015 | |
| Mkn 501 | 253.468 | 39.760 | Pian | 1240011 | 1240011 | |
| Mrk 501 | 253.468 | 39.760 | Kreikenbohm | 1240032 | 1240032 | |
| GRO J1655-40 | 253.500 | -39.846 | Wilms | 1240009 | 1240009 | |
| GRO J1655-40 | 253.500 | -39.846 | Wilms | 1240009 | 1240009 | |
| GRO J1655-40 | 253.500 | -39.846 | Motta | 1240015 | 1240015 | |
| GRO J1655-40 | 253.501 | -39.846 | Rodriguez | 1240027 | 1240027 | |
| GRO J1655-40 | 253.501 | -39.846 | Rodriguez | 1240027 | 1240027 | |
| MAXI J1659-152 | 254.756 | -15.258 | Motta | 1240015 | 1240015 | |
| MAXI J1659-152 | 254.792 | -15.268 | Rodriguez | 1240027 | 1240027 | |
| GB6 J1700+6830 | 255.039 | 68.502 | Pian | 1240011 | 1240011 | |
| XTE J 1701-462 | 255.244 | -46.186 | Paizis | 1240016 | 1240016 | |
| H 1658-298 | 255.529 | -29.946 | Campana | 1240034 | 1240034 | |
| GX 339-4 | 255.706 | -48.790 | Motta | 1240015 | 1240015 | |
| GX 339-4 | 255.706 | -48.790 | Rodriguez | 1240027 | 1240027 | |
| GX 339-4 | 255.706 | -48.790 | Rodriguez | 1240027 | 1240027 | |
| GX 339-4 | 255.708 | -48.790 | Wilms | 1240009 | 1240009 | |
| GX 339-4 | 255.708 | -48.790 | Wilms | 1240009 | 1240009 | |
| H 1705-250 | 257.062 | -25.091 | Wilms | 1240009 | 1240009 | |
| H 1705-250 | 257.062 | -25.091 | Wilms | 1240009 | 1240009 | |
| H 1705-250 | 257.069 | -25.091 | Motta | 1240015 | 1240015 | |
| 1RXS J170849-400910 | 257.192 | -40.148 | Götz | 1240026 | 1240026 | |
| 1RXS J170849-400910 | 257.195 | -40.195 | Kuiper | 1240010 | 1240010 | |
| IGR J17091-3624 | 257.282 | -36.407 | Motta | 1240015 | 1240015 | |
| XTE J1709-267 | 257.375 | -26.658 | Campana | 1240034 | 1240034 | |
| B3 1708+433 | 257.424 | 43.312 | Pian | 1240011 | 1240011 | |
| SAX J1711.6-3808 | 257.900 | -38.142 | Wilms | 1240009 | 1240009 | |
| SAX J1711.6-3808 | 257.900 | -38.142 | Wilms | 1240009 | 1240009 | |
| SAX J1711.6-3808 | 257.905 | -38.118 | Motta | 1240015 | 1240015 | |
| CXO J171405.7-381031 | 258.524 | -38.175 | Kuiper | 1240010 | 1240010 | |
| CXOUJ171405.7-381031 | 258.524 | -38.175 | Götz | 1240026 | 1240026 | |
| PKS 1717+177 | 259.806 | 17.752 | Pian | 1240011 | 1240011 | |
| GRS 1716-249 | 259.904 | -25.018 | Motta | 1240015 | 1240015 | |
| GRS 1716-249 | 259.904 | -25.018 | Wilms | 1240009 | 1240009 | |
| GRS 1716-249 | 259.904 | -25.018 | Wilms | 1240009 | 1240009 | |
| XTE J1720-318 | 259.992 | -31.780 | Motta | 1240015 | 1240015 | |
| XTE J1720-318 | 259.996 | -31.750 | Wilms | 1240009 | 1240009 | |
| XTE J1720-318 | 259.996 | -31.750 | Wilms | 1240009 | 1240009 | |
| XTE J1720-318 | 259.998 | -31.750 | Rodriguez | 1240027 | 1240027 | |
| XTE J1720-318 | 259.998 | -31.750 | Rodriguez | 1240027 | 1240027 | |
| PSR J1723-2837 | 260.847 | -28.633 | Papitto | 1240031 | 1240031 | |
| H 1722+119 | 261.268 | 11.871 | Pian | 1240011 | 1240011 | |
| ZW I 187 | 262.078 | 50.219 | Pian | 1240011 | 1240011 | |
| NRAO 0530 | 263.261 | -13.081 | Pian | 1240011 | 1240011 | |
| KS 1730-312 | 263.383 | -31.217 | Wilms | 1240009 | 1240009 | |
| KS 1730-312 | 263.383 | -31.217 | Wilms | 1240009 | 1240009 | |
| KS 1730-312 | 263.407 | -31.220 | Motta | 1240015 | 1240015 | |
| KS 1731-260 | 263.554 | -26.089 | Campana | 1240034 | 1240034 | |
| XTE J1739-285 | 264.975 | -28.496 | Campana | 1240034 | 1240034 | |
| GRS 1737-31 | 265.038 | -31.040 | Motta | 1240015 | 1240015 | |
| GRS 1737-31 | 265.038 | -31.040 | Rodriguez | 1240027 | 1240027 | |
| GRS 1737-31 | 265.038 | -31.040 | Rodriguez | 1240027 | 1240027 | |
| GRS 1737-31 | 265.038 | -31.033 | Wilms | 1240009 | 1240009 | |
| GRS 1737-31 | 265.038 | -31.033 | Wilms | 1240009 | 1240009 | |
| GRS 1739-278 | 265.667 | -27.748 | Motta | 1240015 | 1240015 | |
| GRS 1739-278 | 265.667 | -27.748 | Wilms | 1240009 | 1240009 | |
| GRS 1739-278 | 265.667 | -27.748 | Wilms | 1240009 | 1240009 | |
| GRS 1739-278 | 265.668 | -27.748 | Rodriguez | 1240027 | 1240027 | |
| GRS 1739-278 | 265.668 | -27.748 | Rodriguez | 1240027 | 1240027 | |
| 1E 1740.7-2942 | 265.979 | -29.745 | Wilms | 1240009 | 1240009 | |
| 1E 1740.7-2942 | 265.979 | -29.745 | Wilms | 1240009 | 1240009 | |
| 1ES 1741+196 | 265.991 | 19.586 | Pian | 1240011 | 1240011 | |
| GRO J1744-28 | 266.138 | -28.741 | Kreykenbohm | 1240013 | 1240013 | |
| SWIFT J174510.8-2624 | 266.295 | -26.403 | Rodriguez | 1240027 | 1240027 | |
| 1A 1742-289 | 266.405 | -29.018 | Motta | 1240015 | 1240015 | |
| Sgr A* | 266.417 | -29.008 | Sunyaev | 1240023 | 1240023 | |
| SGR J1745-2900 | 266.417 | -29.008 | Götz | 1240026 | 1240026 | |
| SGR J1745-2900 | 266.417 | -29.008 | Kuiper | 1240010 | 1240010 | |
| H1743-322 | 266.565 | -32.234 | Motta | 1240015 | 1240015 | |
| H 1743-322 | 266.565 | -32.234 | Rodriguez | 1240027 | 1240027 | |
| H 1743-322 | 266.565 | -32.234 | Rodriguez | 1240027 | 1240027 | |
| H 1743-322 | 266.567 | -32.234 | Wilms | 1240009 | 1240009 | |
| H 1743-322 | 266.567 | -32.234 | Wilms | 1240009 | 1240009 | |
| SAX J1747.0-2853 | 266.762 | -28.883 | Campana | 1240034 | 1240034 | |
| XTE J1748-288 | 267.021 | -28.474 | Wilms | 1240009 | 1240009 | |
| XTE J1748-288 | 267.021 | -28.474 | Wilms | 1240009 | 1240009 | |
| XTE J1748-288 | 267.023 | -28.474 | Rodriguez | 1240027 | 1240027 | |
| XTE J1748-288 | 267.023 | -28.474 | Rodriguez | 1240027 | 1240027 | |
| XTE J1748-288 | 267.023 | -28.474 | Motta | 1240015 | 1240015 | |
| 1A 1744-361 | 267.080 | -36.121 | Kreykenbohm | 1240013 | 1240013 | |
| S4 1749+70 | 267.137 | 70.097 | Pian | 1240011 | 1240011 | |
| AX J1749.2-2725 | 267.292 | -27.421 | Kreykenbohm | 1240013 | 1240013 | |
| SWIFT J1749.4-2807 | 267.383 | -28.135 | Falanga | 1240014 | 1240014 | |
| IGR J17497-2821 | 267.409 | -28.355 | Motta | 1240015 | 1240015 | |
| IGR J17498-2921 | 267.450 | -29.350 | Falanga | 1240014 | 1240014 | |
| SLX 1746-331 | 267.454 | -33.205 | Wilms | 1240009 | 1240009 | |
| SLX 1746-331 | 267.454 | -33.205 | Wilms | 1240009 | 1240009 | |
| SLX 1746-331 | 267.461 | -33.199 | Motta | 1240015 | 1240015 | |
| SLX 1746-331 | 267.461 | -33.199 | Rodriguez | 1240027 | 1240027 | |
| SLX 1746-331 | 267.461 | -33.199 | Rodriguez | 1240027 | 1240027 | |
| SAX J1750.8-2900 | 267.600 | -29.038 | Campana | 1240034 | 1240034 | |
| EXO 1747-214 | 267.604 | -21.422 | Campana | 1240034 | 1240034 | |
| IGR J17511-3057 | 267.786 | -30.961 | Falanga | 1240014 | 1240014 | |
| XTE J1751-305 | 267.804 | -30.623 | Campana | 1240034 | 1240034 | |
| XTE J1751-305 | 267.806 | -30.623 | Falanga | 1240014 | 1240014 | |
| PKS 1749+096 | 267.887 | 9.650 | Pian | 1240011 | 1240011 | |
| XTE J1752-223 | 268.000 | -22.300 | Motta | 1240015 | 1240015 | |
| Swift J1753.5-0127 | 268.368 | -1.452 | Motta | 1240015 | 1240015 | |
| SWIFT J1753.5-0127 | 268.368 | -1.452 | Rodriguez | 1240027 | 1240027 | |
| SWIFT J1753.5-0127 | 268.368 | -1.452 | Rodriguez | 1240027 | 1240027 | |
| XTE J1755-324 | 268.869 | -32.478 | Motta | 1240015 | 1240015 | |
| XTE J1755-324 | 268.871 | -32.478 | Wilms | 1240009 | 1240009 | |
| XTE J1755-324 | 268.871 | -32.478 | Wilms | 1240009 | 1240009 | |
| A 1742-289 | 269.000 | -29.600 | Wilms | 1240009 | 1240009 | |
| A 1742-289 | 269.000 | -29.600 | Wilms | 1240009 | 1240009 | |
| swift J1756.9-2508 | 269.238 | -25.107 | Falanga | 1240014 | 1240014 | |
| SGR 1801-23 | 269.488 | -22.947 | Götz | 1240026 | 1240026 | |
| 4U 1755-338 | 269.667 | -33.808 | Motta | 1240015 | 1240015 | |
| 4U 1755-338 | 269.667 | -33.808 | Wilms | 1240009 | 1240009 | |
| 4U 1755-338 | 269.667 | -33.808 | Wilms | 1240009 | 1240009 | |
| S5 1803+784 | 270.192 | 78.468 | Pian | 1240011 | 1240011 | |
| SGR 1801-23 | 270.245 | -22.947 | Kuiper | 1240010 | 1240010 | |
| GRS 1758-258 | 270.300 | -25.743 | Wilms | 1240009 | 1240009 | |
| GRS 1758-258 | 270.300 | -25.743 | Wilms | 1240009 | 1240009 | |
| GRS 1758-258 | 270.303 | -25.741 | Hirsch | 1240020 | 1240020 | |
| PMN J1802-3940 | 270.678 | -39.669 | Pian | 1240011 | 1240011 | |
| XTE J1807-294 | 271.749 | -29.408 | Falanga | 1240014 | 1240014 | |
| SAX J1808.4-3658 | 272.115 | -36.979 | Falanga | 1240014 | 1240014 | |
| SAX J1808.4-3658 | 272.117 | -36.979 | Campana | 1240034 | 1240034 | |
| SGR 1806-20 | 272.164 | -20.411 | Götz | 1240026 | 1240026 | |
| SGR 1806-20 | 272.164 | -20.411 | Kuiper | 1240010 | 1240010 | |
| XTE J1810-197 | 272.462 | -19.731 | Götz | 1240026 | 1240026 | |
| XTE J1810-197 | 272.463 | -19.731 | Kuiper | 1240010 | 1240010 | |
| XTE J1814-338 | 273.413 | -33.773 | Falanga | 1240014 | 1240014 | |
| XTE J1817-330 | 274.431 | -33.019 | Motta | 1240015 | 1240015 | |
| XTE J1817-330 | 274.431 | -33.019 | Rodriguez | 1240027 | 1240027 | |
| XTE J1817-330 | 274.431 | -33.019 | Rodriguez | 1240027 | 1240027 | |
| XTE J1818-245 | 274.605 | -24.542 | Rodriguez | 1240027 | 1240027 | |
| XTE J1818-245 | 274.605 | -24.542 | Rodriguez | 1240027 | 1240027 | |
| XTE J1818-245 | 274.605 | -24.542 | Motta | 1240015 | 1240015 | |
| AX J1818.8-1559 | 274.717 | -15.989 | Götz | 1240026 | 1240026 | |
| XTE J1819-254 | 274.840 | -25.407 | Motta | 1240015 | 1240015 | |
| V4641 Sgr | 274.842 | -25.407 | Wilms | 1240009 | 1240009 | |
| V4641 Sgr | 274.842 | -25.407 | Wilms | 1240009 | 1240009 | |
| Swift J1822.3-1606 | 275.576 | -16.074 | Götz | 1240026 | 1240026 | |
| Swift J1822.3-1606 | 275.576 | -16.074 | Kuiper | 1240010 | 1240010 | |
| IGR J18245-2452 | 276.111 | -24.857 | Falanga | 1240014 | 1240014 | |
| PKS 1830-21 | 278.416 | -21.061 | Pian | 1240011 | 1240011 | |
| SGR 1833-0832 | 278.435 | -8.519 | Götz | 1240026 | 1240026 | |
| SGR 1833-0832 | 278.442 | -8.537 | Kuiper | 1240010 | 1240010 | |
| Swift J1834.9-0846 | 278.725 | -8.767 | Götz | 1240026 | 1240026 | |
| Swift J1834.9-0846 | 278.725 | -8.767 | Kuiper | 1240010 | 1240010 | |
| Sct X-1 | 278.858 | -7.614 | Kreykenbohm | 1240013 | 1240013 | |
| MAXI J1836-194 | 278.931 | -19.320 | Motta | 1240015 | 1240015 | |
| 1E 1841-045 | 280.331 | -4.936 | Kuiper | 1240010 | 1240010 | |
| 1E 1841-045 | 280.333 | -4.936 | Götz | 1240026 | 1240026 | |
| Ginga 1839-04 | 280.450 | -4.450 | Kreykenbohm | 1240013 | 1240013 | |
| Swift J1842.5-1124 | 280.500 | -11.400 | Motta | 1240015 | 1240015 | |
| AX J1845.0-0258 | 281.222 | -2.945 | Kuiper | 1240010 | 1240010 | |
| AX J1844.8-0258 | 281.229 | -2.948 | Götz | 1240026 | 1240026 | |
| PSR J1846-0258 | 281.602 | -2.974 | Götz | 1240026 | 1240026 | |
| PSR J1846-0258 | 281.602 | -2.974 | Kuiper | 1240010 | 1240010 | |
| 3A 1845-024 | 282.074 | -2.420 | Kreykenbohm | 1240013 | 1240013 | |
| TXS 1846+322 | 282.095 | 32.317 | Pian | 1240011 | 1240011 | |
| EXO 1846-031 | 282.317 | -3.068 | Motta | 1240015 | 1240015 | |
| S4 1849+67 | 282.320 | 67.095 | Pian | 1240011 | 1240011 | |
| EXO 1846-031 | 282.321 | -3.062 | Wilms | 1240009 | 1240009 | |
| EXO 1846-031 | 282.321 | -3.062 | Wilms | 1240009 | 1240009 | |
| 3XMM J1852+0033 | 283.194 | -0.556 | Götz | 1240026 | 1240026 | |
| 3XMM J185246.6+00331 | 283.194 | 0.556 | Kuiper | 1240010 | 1240010 | |
| XTE J1855-026 | 283.880 | -2.607 | Kreykenbohm | 1240013 | 1240013 | |
| Ginga 1855-02 | 284.500 | -2.733 | Kreykenbohm | 1240013 | 1240013 | |
| XTE J1859+226 | 284.673 | 22.658 | Motta | 1240015 | 1240015 | |
| XTE J1859+226 | 284.673 | 22.658 | Rodriguez | 1240027 | 1240027 | |
| XTE J1859+226 | 284.673 | 22.658 | Rodriguez | 1240027 | 1240027 | |
| XTE J1859+226 | 284.675 | 22.658 | Wilms | 1240009 | 1240009 | |
| XTE J1859+226 | 284.675 | 22.658 | Wilms | 1240009 | 1240009 | |
| XTE J1858+034 | 284.679 | 3.439 | Kreykenbohm | 1240013 | 1240013 | |
| HETE J1900.1-2455 | 285.036 | -24.920 | Falanga | 1240014 | 1240014 | |
| 4U 1901+03 | 285.905 | 3.192 | Kreykenbohm | 1240013 | 1240013 | |
| SGR 1900+14 | 286.810 | 9.323 | Götz | 1240026 | 1240026 | |
| SGR 1900+14 | 286.810 | 9.322 | Kuiper | 1240010 | 1240010 | |
| XTE J1908+094 | 287.221 | 9.385 | Wilms | 1240009 | 1240009 | |
| XTE J1908+094 | 287.221 | 9.385 | Wilms | 1240009 | 1240009 | |
| XTE J1908+094 | 287.224 | 9.385 | Motta | 1240015 | 1240015 | |
| PKS 1908-201 | 287.790 | -20.115 | Pian | 1240011 | 1240011 | |
| Aql X-1 | 287.817 | 0.585 | Campana | 1240034 | 1240034 | |
| PMN J1913-3630 | 288.337 | -36.505 | Pian | 1240011 | 1240011 | |
| PKS 1915-458 | 289.819 | -45.727 | Pian | 1240011 | 1240011 | |
| OHIO V -235 | 290.884 | -21.076 | Pian | 1240011 | 1240011 | |
| 4U 1957+11 | 299.850 | 11.708 | Motta | 1240015 | 1240015 | |
| 4U 1957+115 | 299.850 | 11.709 | Wilms | 1240009 | 1240009 | |
| 4U 1957+115 | 299.850 | 11.709 | Wilms | 1240009 | 1240009 | |
| 1ES 1959+650 | 299.999 | 65.149 | Pian | 1240011 | 1240011 | |
| GS 2000+251 | 300.707 | 25.236 | Motta | 1240015 | 1240015 | |
| GS 2000+251 | 300.708 | 25.236 | Wilms | 1240009 | 1240009 | |
| GS 2000+251 | 300.708 | 25.236 | Wilms | 1240009 | 1240009 | |
| PKS 2004-447 | 301.980 | -44.579 | Pian | 1240011 | 1240011 | |
| PKS 2005-489 | 302.356 | -48.832 | Pian | 1240011 | 1240011 | |
| XTE J2012+381 | 303.158 | 38.184 | Motta | 1240015 | 1240015 | |
| XTE J2012+381 | 303.158 | 38.184 | Wilms | 1240009 | 1240009 | |
| XTE J2012+381 | 303.158 | 38.184 | Wilms | 1240009 | 1240009 | |
| SGR J2013+34 | 303.476 | 34.332 | Kuiper | 1240010 | 1240010 | |
| SGR 2013+34 | 303.487 | 34.330 | Götz | 1240026 | 1240026 | |
| V404 Cyg | 306.016 | 33.868 | Rodriguez | 1240027 | 1240027 | |
| V404 Cyg | 306.016 | 33.868 | Rodriguez | 1240027 | 1240027 | |
| GS 2023+338 | 306.016 | 33.868 | Motta | 1240015 | 1240015 | |
| V404 Cyg | 306.017 | 33.868 | Wilms | 1240009 | 1240009 | |
| V404 Cyg | 306.017 | 33.868 | Wilms | 1240009 | 1240009 | |
| PKS B2022-077 | 306.418 | -7.595 | Pian | 1240011 | 1240011 | |
| PKS 2052-474 | 314.068 | -47.247 | Pian | 1240011 | 1240011 | |
| GRO J2058+42 | 314.750 | 41.717 | Kreykenbohm | 1240013 | 1240013 | |
| SAX J2103.5+4545 | 315.899 | 45.752 | Kreykenbohm | 1240013 | 1240013 | |
| XTE J2123-058 | 320.812 | -5.798 | Campana | 1240034 | 1240034 | |
| PMN J2139-4235 | 324.851 | -42.589 | Pian | 1240011 | 1240011 | |
| 1FGL J2143.4+1742 | 325.898 | 17.730 | Pian | 1240011 | 1240011 | |
| PKS 2144+092 | 326.792 | 9.496 | Pian | 1240011 | 1240011 | |
| PKS 2142-75 | 326.803 | -75.604 | Pian | 1240011 | 1240011 | |
| TXS 2155+312 | 329.370 | 31.450 | Pian | 1240011 | 1240011 | |
| PKS 2155-304 | 329.717 | -30.226 | Pian | 1240011 | 1240011 | |
| PKS 2155-83 | 330.583 | -83.637 | Pian | 1240011 | 1240011 | |
| BL Lac | 330.680 | 42.278 | Pian | 1240011 | 1240011 | |
| PKS 2201+171 | 330.862 | 17.430 | Pian | 1240011 | 1240011 | |
| PKS 2204-54 | 331.932 | -53.776 | Pian | 1240011 | 1240011 | |
| PHL 5225 | 337.420 | -8.548 | Pian | 1240011 | 1240011 | |
| CTA 102 | 338.152 | 11.731 | Pian | 1240011 | 1240011 | |
| PMN J2250-2806 | 342.685 | -28.111 | Pian | 1240011 | 1240011 | |
| 3C 454.3 | 343.490 | 16.148 | Pian | 1240011 | 1240011 | |
| 1E 2259+586 | 345.283 | 58.879 | Götz | 1240026 | 1240026 | |
| 1E 2259+586 | 345.435 | 58.879 | Kuiper | 1240010 | 1240010 | |
| B2 2308+34 | 347.772 | 34.420 | Pian | 1240011 | 1240011 | |
| B3 2322+396 | 351.324 | 39.960 | Pian | 1240011 | 1240011 | |
| PKS 2325+093 | 351.890 | 9.669 | Pian | 1240011 | 1240011 | |
| PKS 2326-502 | 352.337 | -49.928 | Pian | 1240011 | 1240011 | |
| PMN J2345-1555 | 356.302 | -15.919 | Pian | 1240011 | 1240011 | |
| 1ES 2344+514 | 356.770 | 51.705 | Pian | 1240011 | 1240011 | |
| H 2356-309 | 359.782 | -30.627 | Pian | 1240011 | 1240011 |
Accepted proposals where the PI is from the Russian Federation follow a similar kind of policy except that the rest of the field will be open only to all Russian Federation scientists currently working at Russian Federation scientific institutes. Access to these data for such scientists will be provided by the Russian Science Data Centre for INTEGRAL located at the Space Research Institute in Moscow. The data under these proposals from the Russian Federation will only be open to the public at large after the 1-year proprietary period has ended