INTEGRAL AO-13 Data Rights Proposals

AO-13 Target Allocations

Posted by ESA/ISOC on 2015/11/23

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- 13 documentation is applicable.

Data Rights on Sources of Non-TOO Proposals (TOO Proposals)

SOURCE NAMERADECPIPROP IDOpen Time ProposalsTAC Data Rights Strategy
Galactic hard X-ray and Gamma-ray Background 0.000 0.000 Krivonos 1330026 1320026 Data rights for the study of the Al26 and 511 keV lines and the diffuse continuum
Galactic hard X-ray and Gamma-ray Background 0.000 0.000 Sunyaev 1330025 1320025 Data rights for the study of the Al26 and 511 keV lines and the diffuse continuum
Earth + CXB 0.000 0.000 Türler 1330022 1320022 Data rights to study the CXB and any auroral emission.
Earth + CXB 0.000 0.000 Türler 1330022 1320022
Tycho SNR 6.308 64.144 Diehl 1330004 1320004 Lines at 68, 79 and 1157 keV of Ti44, the 511 keV line from positrons and the 4.4 MeV nuclear de-excitation of C12.
Tycho SNR 6.308 64.144 Diehl 1330004 1320004
Tycho SNR 6.308 64.144 Diehl 1330004 1320004
Tycho SNR 6.308 64.144 Diehl 1330004 1320004
3A0114+650 19.511 65.292 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
H0115+634 19.633 63.740 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
EXO 0748-676 117.139 -67.750 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
VelaX-1 135.529 -40.555 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023
2S 0918-549 140.110 -55.207 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
mkn110 141.304 52.286 Panessa 1330015 1320015 All data
Carina region 157.500 -57.900 Diehl 1330019 1320019 Diffuse emission in the lines of Al26 and Fe60.
Carina region 157.500 -57.900 Diehl 1330020 1320019 1320027 511 keV line and broad band positronium emission (100 to 550 keV band).
4U1036-56 159.398 -56.803 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
Cen X-3 170.316 -60.623 Klochkov 1330027 1320027
1E1145.1-6141 176.869 -61.954 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
GX301-2 186.657 -62.770 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
4U 1246-588 192.351 -59.092 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
4U 1254-69 194.405 -69.289 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
SAX J1324.5-6313 201.113 -63.224 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
4U 1323-62 201.651 -62.136 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
Cen X-4 224.591 -31.669 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
Scorpius-Centaurus 226.468 -29.398 Diehl 1330002 1320002 TARGET: Sco-Cen region Data rights for the study of diffuse emission in the Al26 line.
Cir X-1 230.170 -57.167 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
Scorpius-Centaurus 234.476 -23.916 Diehl 1330002 1320002 TARGET: Sco-Cen region Data rights for the study of diffuse emission in the Al26 line.
1H 1538-522 235.597 -52.386 Klochkov 1330027 1320027
XTEJ1543-568 236.008 -56.712 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
XTEJ1550-564 237.745 -56.477 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
UW CrB 241.441 25.863 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
4U 1608-522 243.179 -52.423 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
ScoX-1 244.982 -15.640 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
4U1626-67 248.070 -67.462 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023
4U 1636-536 250.231 -53.751 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
GX340+0 251.449 -45.611 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
MAXI J1647-227 251.960 -22.750 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027
XTEJ1650-500 252.504 -49.962 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
Her X-1 254.458 35.342 Klochkov 1330027 1320027
Her X-1 254.458 35.342 Klochkov 1330027 1320027
MAXI J1659-152 254.792 -15.268 Wilms 1330010 1320002 1320027 1320023
OAO1657-415 255.200 -41.673 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 keV (Ti44), 847, 1238 keV (Co56), 122, 136 keV (Co57) and 2213, 4438, 6129 keV (H2, from the Sun)
XTE J1701-462 255.244 -46.186 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
XTE J1701-407 255.435 -40.856 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
4U1700-377 255.987 -37.844 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
IGR J17062-6143 256.568 -61.711 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
4U 1708-23 257.096 -22.803 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
4U 1705-32 257.227 -32.316 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
IGR J17091-3624 257.279 -36.407 Wilms 1330010 1320002 1320027 1320023
XTE J1709-267 257.376 -26.658 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 -26.657 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330010 1320002 1320027 1320023
4U 1708-40 258.096 -40.843 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
IGR J17191-2821 259.808 -28.326 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330010 1320002 1320027 1320023
XTE J1720-318 259.975 -31.749 Wilms 1330010 1320002 1320027 1320023
XTE J1723-376 260.908 -37.662 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1722-30 261.888 -30.802 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330010 1320002 1320027 1320023
3A1728-169 262.934 -16.962 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1728-34 262.990 -33.834 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1730-335 263.350 -33.388 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330010 1320002 1320027 1320023
KS 1731-260 263.556 -26.088 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 J17354-3255 263.854 -32.938 Sidoli 1330012 1320023
SLX 1732-304 263.945 -30.483 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
SLX 1735-269 264.571 -26.994 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1735-444 264.743 -44.450 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
XTE J1739-285 264.975 -28.496 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330010 1320002 1320027 1320023
SLX 1737-282 265.162 -28.297 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330010 1320002 1320027 1320023
KS 1741-293 266.213 -29.355 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330010 1320002 1320027 1320023
AX J1745.6-2901 266.398 -29.026 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330023 1320023
1A 1742-294 266.522 -29.515 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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.
H 1743-322 266.567 -32.234 Wilms 1330010 1320002 1320027 1320023
GX 0.2-0.2 266.761 -28.883 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330010 1320002 1320027 1320023
IGR J17480-2446 267.020 -24.780 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 267.023 -24.777 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1744-361 267.055 -36.132 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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.
SLX1746-331 267.452 -33.205 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 267.600 -29.038 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330010 1320002 1320027 1320023
SAX J1752.3-3138 268.100 -31.628 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 J17541-2252 268.525 -22.867 Sidoli 1330012 1320023
AX J1754.2-2754 268.561 -27.910 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330010 1320002 1320027 1320023
4U 1755-338 269.667 -33.808 Wilms 1330010 1320002 1320027 1320023
IGR J17597-2201 269.940 -22.028 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 -22.027 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330013 1320023
GX9+1 270.385 -20.529 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027
GX 13+1 273.631 -17.157 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
IGR J18159-3353 273.988 -33.890 Sidoli 1330012 1320023
GX 17+2 274.006 -14.036 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
XTE J1817-330 274.431 -33.019 Wilms 1330010 1320002 1320027 1320023
IGR J18175-2419 274.470 -24.329 Sidoli 1330012 1320023
XTE J1818-245 274.603 -24.538 Wilms 1330010 1320002 1320027 1320023
SAX J1818.6–1703 274.658 -17.047 Sidoli 1330012 1320023
V4641 Sgr 274.840 -25.407 Wilms 1330010 1320002 1320027 1320023
4U 1820-303 275.919 -30.361 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1820-303 275.919 -30.361 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
3A1822-371 276.445 -37.105 Watanabe 1330003 1320004 1320002 1320027 1320019 1320023 Data rights on unknown/unpredicted gamma-ray lines with SPI. The known lines, excluded for this proposal, are at 511 keV (e+-e-), 1809 keV (Al26), 59, 1173, 1333 keV (Fe60), 68, 78, 1157 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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
Ginga 1826-24 277.368 -23.797 Chenevez 1330029 1320023 1320002 1320027 Long (>5min) Type-I X-ray bursts in the light curves of Gal. X-ray bursters
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 Type-I X-ray bursts are granted to another accepted proposal (PI: Sanchez-Fernandez, Prop ID: 1320016).
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.
GS 1826-24 277.368 -23.797 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
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, Prop ID: 1320029).
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 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
4U 1850-086 283.270 -8.705 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
HETE J1900.1-2455 285.036 -24.920 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
SAX J2224.9+5421 336.217 54.365 Sanchez-Fernandez 1330016 1320023 1320002 1320004 1320019 1320027 Type-I X-ray bursts.
Cas A 350.866 58.812 Diehl 1330004 1320004 Lines at 68, 79 and 1157 keV of Ti44, the 511 keV line from positrons and the 4.4 MeV nuclear de-excitation of C12.
Cas A 350.866 58.812 Diehl 1330004 1320004
Cas A 350.866 58.812 Diehl 1330004 1320004
Cas A 350.866 58.812 Diehl 1330004 1320004

Data Rights on Sources of TOO Proposals (Non TOO Proposals)

SOURCE NAMERADECPIPROP IDOpen Time ProposalsTAC Data Rights Strategy
New BH Transient 0.000 0.000 Belloni 1340010 1340010
Gamma-ray transient 0.000 0.000 Bottacini 1340025 1340025
SN Ia 0.000 0.000 Diehl 1340017 1340017
NEW 0.000 0.000 Ferrigno 1340011 1340011
NEW 0.000 0.000 Ferrigno 1340020 1340020
GRB 0.000 0.000 Gotz 1340002 1340002
supernova 0.000 0.000 Grebenev 1340032 1340032
new AXP/SGR 0.000 0.000 Götz 1340012 1340012
Classical Nova 0.000 0.000 Hernanz 1340026 1340026
FermiTransient1 0.000 0.000 Hill 1340029 1340029
Gamma-ray burst 0.000 0.000 Hurley 1340001 1340001
SNIa Early Obs 0.000 0.000 Isern 1340005 1340005
Transient black hole 0.000 0.000 Kalemci 1340009 1340009
New Transient Pulsar 0.000 0.000 Kreykenbohm 1340013 1340013
TDE 0.000 0.000 Panessa 1340003 1340003
GRB1 0.000 0.000 Pozanenko 1340007 1340007
GRB outside the FoV 0.000 0.000 Savchenko 1340021 1340021
PMN J0017-0512 4.399 -5.212 Pian 1340015 1340015
GRB041219 6.112 62.843 Martin-Carrillo 1340030 1340030
IGR J00291+5934 7.263 59.572 Ferrigno 1340020 1340020
RBS 0076 8.393 -19.359 Pian 1340015 1340015
1ES 0033+595 8.969 59.835 Pian 1340015 1340015
AX J0049-729 12.275 -72.847 Kreykenbohm 1340013 1340013
PKS 0048-097 12.672 -9.485 Pian 1340015 1340015
AX J0051-722 12.732 -72.232 Kreykenbohm 1340013 1340013
PKS 0048-071 12.784 -6.834 Pian 1340015 1340015
2E 0050.1-7247 12.972 -72.530 Kreykenbohm 1340013 1340013
RX J0052.1-7319 13.058 -73.320 Kreykenbohm 1340013 1340013
RX J0052.9-7158 13.230 -71.968 Kreykenbohm 1340013 1340013
RX J0053.8-7226 13.479 -72.446 Kreykenbohm 1340013 1340013
XTE J0055-724 13.734 -72.441 Kreykenbohm 1340013 1340013
RX J0059.2-7138 14.797 -71.646 Kreykenbohm 1340013 1340013
AX J0105-722 16.287 -72.196 Kreykenbohm 1340013 1340013
CXOU 010043-7211 17.679 -72.193 Götz 1340012 1340012
PSR J0111-7317 17.785 -73.279 Kreykenbohm 1340013 1340013
S2 0109+22 18.024 22.744 Pian 1340015 1340015
4C 31.03 18.210 32.138 Pian 1340015 1340015
RX J0117.6-7330 19.422 -73.514 Kreykenbohm 1340013 1340013
PKS 0116-219 19.739 -21.692 Pian 1340015 1340015
PKS 0118-272 20.132 -27.024 Pian 1340015 1340015
1ES 0120+340 20.785 34.347 Pian 1340015 1340015
B3 0133+388 24.135 39.100 Pian 1340015 1340015
DA 055 24.244 47.858 Pian 1340015 1340015
TXS 0141+268 26.140 27.084 Pian 1340015 1340015
PKS 0142-278 26.264 -27.560 Pian 1340015 1340015
4U 0142+614 26.592 61.751 Götz 1340012 1340012
PKS 0202-17 31.240 -17.022 Pian 1340015 1340015
PKS 0208-512 32.692 -51.017 Pian 1340015 1340015
CGRaBS J0211+1051 32.805 10.860 Pian 1340015 1340015
TXS 0214+517 34.391 51.966 Pian 1340015 1340015
PKS 0215+015 34.454 1.747 Pian 1340015 1340015
TXS 0218+357 35.273 35.937 Pian 1340015 1340015
3C 66A 35.665 43.036 Pian 1340015 1340015
PKS 0227-369 37.368 -36.732 Pian 1340015 1340015
1ES 0229+200 38.203 20.288 Pian 1340015 1340015
PKS 0235-618 39.222 -61.604 Pian 1340015 1340015
4C +28.07 39.468 28.802 Pian 1340015 1340015
PKS 0235+164 39.662 16.616 Pian 1340015 1340015
PKS 0244-470 41.500 -46.855 Pian 1340015 1340015
PKS 0301-243 45.860 -24.120 Pian 1340015 1340015
1H 0323+342 51.172 34.179 Pian 1340015 1340015
1H 0323+022 51.558 2.421 Pian 1340015 1340015
PKS 0332-403 53.557 -40.140 Pian 1340015 1340015
V0332+53 53.750 53.173 Lutovinov 1340023 1340023
PKS 0347-211 57.491 -21.047 Pian 1340015 1340015
PKS 0402-362 60.974 -36.084 Pian 1340015 1340015
PKS 0405-385 61.747 -38.441 Pian 1340015 1340015
PMN J0413-5332 63.322 -53.534 Pian 1340015 1340015
1H 0414+009 64.224 1.082 Pian 1340015 1340015
SGR 0418+5729 64.642 57.540 Götz 1340012 1340012
XTE J0421+560 64.925 56.000 Belloni 1340010 1340010
GRO J0422+32 65.428 32.909 Belloni 1340010 1340010
GRO J0422+32 65.428 32.909 Kalemci 1340009 1340009
PKS 0420-01 65.816 -1.342 Pian 1340015 1340015
PKS 0426-380 67.168 -37.939 Pian 1340015 1340015
NRAO 0190 70.661 -0.295 Pian 1340015 1340015
PKS 0447-439 72.353 -43.836 Pian 1340015 1340015
PKS 0454-234 74.263 -23.414 Pian 1340015 1340015
SGR 0501+4516 75.265 45.272 Götz 1340012 1340012
RX J0502.9-6626 75.715 -66.440 Kreykenbohm 1340013 1340013
1ES 0502+675 76.984 67.623 Pian 1340015 1340015
PKS 0516-621 79.187 -62.118 Pian 1340015 1340015
PKS 0521-36 80.742 -36.459 Pian 1340015 1340015
SGR 0525-66 81.504 -66.077 Götz 1340012 1340012
RX J0529.8-6556 82.452 -65.948 Kreykenbohm 1340013 1340013
PKS B0528+134 82.735 13.532 Pian 1340015 1340015
EXO 053109-6609.2 82.805 -66.118 Kreykenbohm 1340013 1340013
PMN J0531-4827 82.994 -48.460 Pian 1340015 1340015
PMN J0532+0732 83.162 7.545 Pian 1340015 1340015
RX J0535.6-6651 83.919 -66.865 Kreykenbohm 1340013 1340013
PKS 0537-441 84.710 -44.086 Pian 1340015 1340015
AX J0544.1-7100 86.026 -71.014 Kreykenbohm 1340013 1340013
PKS 0548-322 87.670 -32.272 Pian 1340015 1340015
H 0557-385 89.508 -38.335 Pian 1340015 1340015
1A 0620-00 95.685 -0.346 Belloni 1340010 1340010
A0620-00 95.685 -0.346 Kalemci 1340009 1340009
B2 0619+33 95.718 33.436 Pian 1340015 1340015
1ES 0647+250 102.694 25.050 Pian 1340015 1340015
GB6 J0654+5042 103.595 50.707 Pian 1340015 1340015
CJ2 0650+453 103.599 45.240 Pian 1340015 1340015
PKS 0700-661 105.130 -66.179 Pian 1340015 1340015
GB6 J0712+5033 108.182 50.556 Pian 1340015 1340015
1FGL J0714.0+1935 108.482 19.583 Pian 1340015 1340015
TXS 0716+332 109.831 33.119 Pian 1340015 1340015
S5 0716+71 110.473 71.343 Pian 1340015 1340015
4C 14.23 111.320 14.420 Pian 1340015 1340015
3A 0726-260 112.222 -26.108 Kreykenbohm 1340013 1340013
PKS 0727-11 112.580 -11.687 Pian 1340015 1340015
PKS B0735+178 114.531 17.705 Pian 1340015 1340015
1FGL J0742.2+5443 115.666 54.740 Pian 1340015 1340015
PKS 0805-07 122.065 -7.853 Pian 1340015 1340015
1ES 0806+524 122.455 52.316 Pian 1340015 1340015
PMN J0811+0237 123.008 2.626 Pian 1340015 1340015
RX J0812.4-3114 123.118 -31.248 Kreykenbohm 1340013 1340013
S4 0814+425 124.567 42.379 Pian 1340015 1340015
TXS 0820+560 126.197 55.879 Pian 1340015 1340015
PKS 0823-223 126.507 -22.508 Pian 1340015 1340015
B2 0827+24 127.720 24.183 Pian 1340015 1340015
Ginga 0834-430 128.979 -43.185 Kreykenbohm 1340013 1340013
S5 0836+71 130.352 70.895 Pian 1340015 1340015
OJ 287 133.704 20.109 Pian 1340015 1340015
3EG J0903-3531 136.200 -35.200 Pian 1340015 1340015
PKS B0906+015 137.295 1.360 Pian 1340015 1340015
PKS 0907+022 137.416 2.001 Pian 1340015 1340015
S4 0917+44 140.244 44.698 Pian 1340015 1340015
XTE J0929-314 142.334 -31.384 Ferrigno 1340020 1340020
PMN J0948+0022 147.239 0.374 Pian 1340015 1340015
S4 0954+55 149.409 55.383 Pian 1340015 1340015
1FGL J1012.7+2440 153.172 24.656 Pian 1340015 1340015
GRS 1009-45 153.401 -45.076 Belloni 1340010 1340010
GRS 1009-45 153.401 -45.076 Kalemci 1340009 1340009
1ES 1011+496 153.768 49.434 Pian 1340015 1340015
PMN J1016+0512 154.013 5.217 Pian 1340015 1340015
1ES 1028+511 157.827 50.894 Pian 1340015 1340015
S4 1030+61 158.464 60.852 Pian 1340015 1340015
4U 1036-56 159.398 -56.803 Kreykenbohm 1340013 1340013
1E 1048.1-5937 162.529 -59.889 Götz 1340012 1340012
1FGL J1053.6+4927 163.434 49.499 Pian 1340015 1340015
1FGL J1054.5+2212 163.628 22.182 Pian 1340015 1340015
PKS 1055+018 164.623 1.566 Pian 1340015 1340015
RX J1058.6+5628 164.657 56.470 Pian 1340015 1340015
PKS 1057-79 164.680 -80.065 Pian 1340015 1340015
1ES 1101-232 165.907 -23.492 Pian 1340015 1340015
Mkn 421 166.114 38.209 Pian 1340015 1340015
Mrk 421 166.114 38.209 Kreikenbohm 1340027 1340027
RBS 0958 169.276 20.236 Pian 1340015 1340015
XTE J1118+480 169.545 48.037 Belloni 1340010 1340010
XTE J1118+480 169.545 48.037 Kalemci 1340009 1340009
PKS 1118-056 170.355 -5.899 Pian 1340015 1340015
GS 1124-68 171.611 -68.676 Belloni 1340010 1340010
GS 1124-68 171.611 -68.676 Kalemci 1340009 1340009
PKS 1124-186 171.768 -18.955 Pian 1340015 1340015
PKS 1127-14 172.531 -14.824 Pian 1340015 1340015
Mkn 180 174.110 70.158 Pian 1340015 1340015
BWE 1133+6753 174.126 67.618 Pian 1340015 1340015
PKS 1144-379 176.756 -38.203 Pian 1340015 1340015
H 1145-619 177.000 -62.207 Alfonso-Garzon 1340028 1340028
H 1145-619 177.000 -62.207 Kreykenbohm 1340013 1340013
4C 29.45 179.883 29.245 Pian 1340015 1340015
RBS 1093 184.470 30.117 Pian 1340015 1340015
PG 1218+304 185.341 30.177 Pian 1340015 1340015
ON 231 185.382 28.233 Pian 1340015 1340015
PKS 1222+21 186.227 21.380 Pian 1340015 1340015
3C 273 187.278 2.052 Pian 1340015 1340015
GB6 J1239+0443 189.886 4.718 Pian 1340015 1340015
PKS 1244-255 191.695 -25.797 Pian 1340015 1340015
PG 1246+586 192.078 58.341 Pian 1340015 1340015
TXS 1250+532 193.300 53.020 Pian 1340015 1340015
3C 279 194.050 -5.789 Pian 1340015 1340015
MAXI J1305-704 196.731 -70.450 Belloni 1340010 1340010
OP 313 197.619 32.346 Pian 1340015 1340015
TXS 1310+487 198.181 48.475 Pian 1340015 1340015
PKS 1329-049 203.019 -5.162 Pian 1340015 1340015
1FGL J1333.2+5056 203.474 50.960 Pian 1340015 1340015
B3 1343+451 206.388 44.883 Pian 1340015 1340015
PKS 1352-104 208.694 -10.684 Pian 1340015 1340015
Swift J1357.2-0933 209.320 -9.544 Belloni 1340010 1340010
SWIFT J1357.2-0933 209.325 -9.552 Kalemci 1340009 1340009
GS 1354-645 209.540 -64.735 Belloni 1340010 1340010
GS 1354-645 209.540 -64.735 Kalemci 1340009 1340009
PKS 1406-076 212.235 -7.874 Pian 1340015 1340015
1E 1415.6+2557 214.486 25.724 Pian 1340015 1340015
H 1417-624 215.304 -62.698 Kreykenbohm 1340013 1340013
MAXI J1421-613 215.413 -61.345 Belloni 1340010 1340010
PKS 1424+240 216.752 23.800 Pian 1340015 1340015
PKS 1424-41 216.985 -42.105 Pian 1340015 1340015
1ES 1426+428 217.135 42.674 Pian 1340015 1340015
1ES 1440+122 220.701 12.011 Pian 1340015 1340015
PKS 1454-354 224.361 -35.653 Pian 1340015 1340015
PKS 1502+106 226.104 10.494 Pian 1340015 1340015
PKS 1502+036 226.277 3.442 Pian 1340015 1340015
PKS 1508-05 227.723 -5.719 Pian 1340015 1340015
PKS 1510-089 228.211 -9.100 Pian 1340015 1340015
Ap Lib 229.424 -24.372 Pian 1340015 1340015
TXS 1520+319 230.542 31.737 Pian 1340015 1340015
4U 1524-617 232.070 -61.883 Belloni 1340010 1340010
X 1524-617 232.070 -61.883 Kalemci 1340009 1340009
Swift J1539.2-6227 234.800 -62.467 Belloni 1340010 1340010
Swift J1539.2-6227 234.800 -62.467 Kalemci 1340009 1340009
1ES 1544+820 235.067 81.918 Pian 1340015 1340015
GB6 J1542+6129 235.737 61.499 Pian 1340015 1340015
MAXI J1543-564 235.823 -56.414 Belloni 1340010 1340010
MAXI J1543-564 235.823 -56.414 Kalemci 1340009 1340009
XTE J1543-568 236.008 -56.712 Kreykenbohm 1340013 1340013
4U 1543-475 236.786 -47.669 Belloni 1340010 1340010
4U 1543-475 236.786 -47.669 Kalemci 1340009 1340009
1E 1547.0–5408 237.729 -54.322 Götz 1340012 1340012
XTE J1550-564 237.745 -56.477 Belloni 1340010 1340010
XTE J1550-564 237.745 -56.477 Kalemci 1340009 1340009
PKS 1551+130 238.386 12.948 Pian 1340015 1340015
PG 1553+113 238.930 11.190 Pian 1340015 1340015
PSR J1622-4950 245.687 -49.848 Götz 1340012 1340012
PKS 1622-253 246.445 -25.461 Pian 1340015 1340015
PKS 1622-29 246.526 -29.857 Pian 1340015 1340015
4C 38.41 248.815 38.134 Pian 1340015 1340015
SGR 1627-41 248.966 -47.590 Götz 1340012 1340012
IGR J16358-4726 248.974 -47.428 Kreykenbohm 1340013 1340013
CXO J164710.2-455216 251.792 -45.871 Götz 1340012 1340012
XTE J1650-500 252.504 -49.962 Belloni 1340010 1340010
XTE J1650-500 252.504 -49.962 Kalemci 1340009 1340009
XTE J1652-453 253.085 -45.344 Belloni 1340010 1340010
XTE J1652-453 253.085 -45.344 Kalemci 1340009 1340009
Mkn 501 253.468 39.760 Pian 1340015 1340015
Mrk 501 253.468 39.760 Kreikenbohm 1340027 1340027
GRO J1655-40 253.500 -39.846 Belloni 1340010 1340010
GRO J1655-40 253.500 -39.846 Kalemci 1340009 1340009
MAXI J1659-152 254.756 -15.258 Belloni 1340010 1340010
MAXI J1659-152 254.792 -15.268 Kalemci 1340009 1340009
GB6 J1700+6830 255.039 68.502 Pian 1340015 1340015
XTE J 1701-462 255.244 -46.186 Paizis 1340014 1340014
GX 339-4 255.706 -48.790 Belloni 1340010 1340010
H 1705-250 257.069 -25.091 Belloni 1340010 1340010
H 1705-250 257.069 -25.091 Kalemci 1340009 1340009
1RXS J170849-400910 257.192 -40.148 Götz 1340012 1340012
Swift J17091-3624 257.282 -36.407 Belloni 1340010 1340010
IGR J17091-3624 257.283 -36.407 Kalemci 1340009 1340009
B3 1708+433 257.424 43.312 Pian 1340015 1340015
SAX J1711.6-3808 257.905 -38.118 Belloni 1340010 1340010
SAX J1711.6-3808 257.905 -38.118 Kalemci 1340009 1340009
CXOUJ171405.7-381031 258.524 -38.175 Götz 1340012 1340012
IGR J17177-3656 259.427 -36.935 Kalemci 1340009 1340009
PKS 1717+177 259.806 17.752 Pian 1340015 1340015
GRS 1716-249 259.904 -25.018 Belloni 1340010 1340010
GRS 1716-249 259.904 -25.018 Kalemci 1340009 1340009
XTE J1720-318 259.992 -31.780 Belloni 1340010 1340010
XTE J1720-318 259.992 -31.780 Kalemci 1340009 1340009
PSR J1723-2837 260.847 -28.633 Papitto 1340024 1340024
H 1722+119 261.268 11.871 Pian 1340015 1340015
ZW I 187 262.078 50.219 Pian 1340015 1340015
NRAO 0530 263.261 -13.081 Pian 1340015 1340015
KS 1730-312 263.386 -31.217 Kalemci 1340009 1340009
KS 1730-312 263.407 -31.220 Belloni 1340010 1340010
GRS 1737-31 265.038 -31.040 Belloni 1340010 1340010
GRS 1737-31 265.038 -31.040 Kalemci 1340009 1340009
GRS 1739-278 265.667 -27.748 Belloni 1340010 1340010
GRS 1739-278 265.667 -27.748 Kalemci 1340009 1340009
1ES 1741+196 265.991 19.586 Pian 1340015 1340015
GRO J1744-28 266.138 -28.741 Kreykenbohm 1340013 1340013
SWIFT J174510.8-2624 266.295 -26.400 Kalemci 1340009 1340009
Swift J174510.8-2624 266.295 -26.405 Belloni 1340010 1340010
1A 1742-289 266.405 -29.018 Belloni 1340010 1340010
A 1742-289 266.405 -29.018 Kalemci 1340009 1340009
SGR J1745-2900 266.417 -29.008 Götz 1340012 1340012
H1743-322 266.565 -32.234 Belloni 1340010 1340010
H1743-322 266.565 -32.234 Kalemci 1340009 1340009
XTE J1748-288 267.023 -28.474 Belloni 1340010 1340010
XTE J1748-288 267.023 -28.474 Kalemci 1340009 1340009
1A 1744-361 267.080 -36.121 Kreykenbohm 1340013 1340013
S4 1749+70 267.137 70.097 Pian 1340015 1340015
AX J1749.2-2725 267.292 -27.421 Kreykenbohm 1340013 1340013
SWIFT J1749.4-2807 267.383 -28.135 Ferrigno 1340020 1340020
IGR J17497-2821 267.409 -28.355 Belloni 1340010 1340010
IGR J17497-2821 267.409 -28.355 Kalemci 1340009 1340009
IGR J17498-2921 267.450 -29.350 Ferrigno 1340020 1340020
SLX 1746-331 267.461 -33.199 Belloni 1340010 1340010
SLX 1746-331 267.461 -33.199 Kalemci 1340009 1340009
IGR J17511-3057 267.786 -30.961 Ferrigno 1340020 1340020
XTE J1751-305 267.806 -30.623 Ferrigno 1340020 1340020
PKS 1749+096 267.887 9.650 Pian 1340015 1340015
XTE J1752-223 268.000 -22.300 Belloni 1340010 1340010
XTE J1752-322 268.000 -22.300 Kalemci 1340009 1340009
XTE J1752-223 268.000 -22.300 Kalemci 1340009 1340009
Swift J1753.5-0127 268.368 -1.452 Belloni 1340010 1340010
SWIFT J1753.5-0127 268.368 -1.452 Kalemci 1340009 1340009
XTE J1755-324 268.869 -32.478 Belloni 1340010 1340010
XTE J1755-324 268.869 -32.478 Kalemci 1340009 1340009
swift J1756.9-2508 269.238 -25.107 Ferrigno 1340020 1340020
SGR 1801-23 269.488 -22.947 Götz 1340012 1340012
4U 1755-338 269.667 -33.808 Belloni 1340010 1340010
4U 1755-338 269.667 -33.808 Kalemci 1340009 1340009
S5 1803+784 270.192 78.468 Pian 1340015 1340015
GRS 1758-258 270.303 -25.741 Hirsch 1340018 1340018
PMN J1802-3940 270.678 -39.669 Pian 1340015 1340015
XTE J1807-294 271.749 -29.408 Ferrigno 1340020 1340020
SAX J1808.4-3658 272.115 -36.979 Ferrigno 1340020 1340020
SGR 1806-20 272.164 -20.411 Götz 1340012 1340012
XTE J1810-197 272.462 -19.731 Götz 1340012 1340012
XTE J1814-338 273.413 -33.773 Ferrigno 1340020 1340020
XTE J1817-330 274.431 -33.019 Belloni 1340010 1340010
XTE J1817-330 274.431 -33.019 Kalemci 1340009 1340009
XTE J1818-245 274.605 -24.542 Belloni 1340010 1340010
XTE J1818-245 274.605 -24.542 Kalemci 1340009 1340009
AX J1818.8-1559 274.717 -15.989 Götz 1340012 1340012
XTE J1819-254 274.840 -25.407 Belloni 1340010 1340010
X 1819-25 274.840 -25.407 Kalemci 1340009 1340009
Swift J1822.3-1606 275.576 -16.074 Götz 1340012 1340012
IGR J18245-2452 276.111 -24.857 Ferrigno 1340020 1340020
MAXI J1828-249 277.118 -24.906 Belloni 1340010 1340010
PKS 1830-21 278.416 -21.061 Pian 1340015 1340015
SGR 1833-0832 278.435 -8.519 Götz 1340012 1340012
Swift J1834.9-0846 278.725 -8.767 Götz 1340012 1340012
Sct X-1 278.858 -7.614 Kreykenbohm 1340013 1340013
MAXI J1836-194 278.931 -19.320 Belloni 1340010 1340010
MAXI J1836-194 278.931 -19.320 Kalemci 1340009 1340009
1E 1841-045 280.333 -4.936 Götz 1340012 1340012
Ginga 1839-04 280.450 -4.450 Kreykenbohm 1340013 1340013
Swift J1842.5-1124 280.500 -11.400 Belloni 1340010 1340010
Swift J1842.5-1124 280.500 -11.400 Kalemci 1340009 1340009
AX J1844-0258 281.229 -2.948 Götz 1340012 1340012
PSR J1846-0258 281.602 -2.974 Götz 1340012 1340012
3A 1845-024 282.074 -2.420 Kreykenbohm 1340013 1340013
TXS 1846+322 282.095 32.317 Pian 1340015 1340015
EXO 1846-031 282.317 -3.068 Belloni 1340010 1340010
S4 1849+67 282.320 67.095 Pian 1340015 1340015
EXO 1846-031 282.321 -3.062 Kalemci 1340009 1340009
3XMM J1852+0033 283.194 -0.556 Götz 1340012 1340012
XTE J1855-026 283.880 -2.607 Kreykenbohm 1340013 1340013
Ginga 1855-02 284.500 -2.733 Kreykenbohm 1340013 1340013
XTE J1859+226 284.673 22.658 Belloni 1340010 1340010
XTE J1859+226 284.673 22.658 Kalemci 1340009 1340009
XTE J1858+034 284.679 3.439 Kreykenbohm 1340013 1340013
HETE J1900.1-2455 285.036 -24.920 Ferrigno 1340020 1340020
4U 1901+03 285.905 3.192 Kreykenbohm 1340013 1340013
SGR 1900+14 286.810 9.323 Götz 1340012 1340012
XTE J1908+094 287.224 9.385 Belloni 1340010 1340010
XTE J1908+094 287.224 9.385 Kalemci 1340009 1340009
PKS 1908-201 287.790 -20.115 Pian 1340015 1340015
PMN J1913-3630 288.337 -36.505 Pian 1340015 1340015
PKS 1915-458 289.819 -45.727 Pian 1340015 1340015
OHIO V -235 290.884 -21.076 Pian 1340015 1340015
SGR 1935+2154 293.732 21.897 Götz 1340012 1340012
4U 1957+11 299.850 11.708 Belloni 1340010 1340010
4U 1957+11 299.850 11.708 Kalemci 1340009 1340009
1ES 1959+650 299.999 65.149 Pian 1340015 1340015
GS 2000+251 300.707 25.236 Kalemci 1340009 1340009
GS 2000+251 300.707 25.236 Belloni 1340010 1340010
PKS 2004-447 301.980 -44.579 Pian 1340015 1340015
PKS 2005-489 302.356 -48.832 Pian 1340015 1340015
XTE J2012+381 303.158 38.184 Belloni 1340010 1340010
XTE J2012+381 303.158 38.184 Kalemci 1340009 1340009
SGR 2013+34 303.487 34.330 Götz 1340012 1340012
GS 2023+338 306.016 33.868 Belloni 1340010 1340010
GS 2023+338 306.016 33.868 Kalemci 1340009 1340009
PKS B2022-077 306.418 -7.595 Pian 1340015 1340015
PKS 2052-474 314.068 -47.247 Pian 1340015 1340015
GRO J2058+42 314.750 41.717 Kreykenbohm 1340013 1340013
SAX J2103.5+4545 315.899 45.752 Kreykenbohm 1340013 1340013
PMN J2139-4235 324.851 -42.589 Pian 1340015 1340015
1FGL J2143.4+1742 325.898 17.730 Pian 1340015 1340015
PKS 2144+092 326.792 9.496 Pian 1340015 1340015
PKS 2142-75 326.803 -75.604 Pian 1340015 1340015
TXS 2155+312 329.370 31.450 Pian 1340015 1340015
PKS 2155-304 329.717 -30.226 Pian 1340015 1340015
PKS 2155-83 330.583 -83.637 Pian 1340015 1340015
BL Lac 330.680 42.278 Pian 1340015 1340015
PKS 2201+171 330.862 17.430 Pian 1340015 1340015
PKS 2204-54 331.932 -53.776 Pian 1340015 1340015
PHL 5225 337.420 -8.548 Pian 1340015 1340015
CTA 102 338.152 11.731 Pian 1340015 1340015
PMN J2250-2806 342.685 -28.111 Pian 1340015 1340015
3C 454.3 343.490 16.148 Pian 1340015 1340015
1E 2259+586 345.283 58.879 Götz 1340012 1340012
B2 2308+34 347.772 34.420 Pian 1340015 1340015
B3 2322+396 351.324 39.960 Pian 1340015 1340015
PKS 2325+093 351.890 9.669 Pian 1340015 1340015
PKS 2326-502 352.337 -49.928 Pian 1340015 1340015
PMN J2345-1555 356.302 -15.919 Pian 1340015 1340015
1ES 2344+514 356.770 51.705 Pian 1340015 1340015
H 2356-309 359.782 -30.627 Pian 1340015 1340015

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