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.
| SOURCE NAME | RA | DEC | PI | PROP ID | Open Time Proposals | TAC Data Rights Strategy |
|---|---|---|---|---|---|---|
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 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. |
| 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. |
| 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. |
| 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. |
| 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 1742-294 | 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| Scorpius-Centaurus | 234.476 | -23.916 | Diehl | 1330002 | 1320002 | Data rights for the study of diffuse emission in the Al26 line. |
| Scorpius-Centaurus | 226.468 | -29.398 | Diehl | 1330002 | 1320002 | Data rights for the study of diffuse emission in the Al26 line. |
| 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 | |
| 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. |
| Cas A | 350.866 | 58.812 | Diehl | 1330004 | 1320004 | |
| Tycho SNR | 6.308 | 64.144 | Diehl | 1330004 | 1320004 | |
| Tycho SNR | 6.308 | 64.144 | Diehl | 1330004 | 1320004 | |
| Cas A | 350.866 | 58.812 | Diehl | 1330004 | 1320004 | |
| Tycho SNR | 6.308 | 64.144 | Diehl | 1330004 | 1320004 | |
| 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). |
| GRS 1758-258 | 270.302 | -25.743 | Hirsch | 1330013 | 1320023 | |
| Her X-1 | 254.458 | 35.342 | Klochkov | 1330027 | 1320027 | |
| 1H 1538-522 | 235.597 | -52.386 | Klochkov | 1330027 | 1320027 | |
| Her X-1 | 254.458 | 35.342 | Klochkov | 1330027 | 1320027 | |
| Cen X-3 | 170.316 | -60.623 | Klochkov | 1330027 | 1320027 | |
| 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 |
| mkn110 | 141.304 | 52.286 | Panessa | 1330015 | 1320015 | All data |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 17+2 | 274.006 | -14.036 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| EXO 0748-676 | 117.139 | -67.750 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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 | 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 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. |
| GX 13+1 | 273.631 | -17.157 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | |
| 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. |
| 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 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. |
| 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 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. |
| HETE J1900.1-2455 | 285.036 | -24.920 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| IGR J17380-3749 | 264.475 | -37.783 | 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. |
| 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. |
| MXB 1658-298 | 255.527 | -29.946 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| MXB 1716-31 | 259.750 | -31.877 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| XB 1832-330 | 278.932 | -32.991 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 2S 0918-549 | 140.110 | -55.207 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| SAX J1828.5-1037 | 277.142 | -10.617 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| SAX J2224.9+5421 | 336.217 | 54.365 | 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. |
| XTE J1701-462 | 255.244 | -46.186 | 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. |
| 4U 1608-522 | 243.179 | -52.423 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 4U 1246-588 | 192.351 | -59.092 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 4U 1702-429 | 256.564 | -43.036 | 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. |
| 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 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. |
| 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. |
| 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. |
| 4U 1636-536 | 250.231 | -53.751 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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 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. |
| 4U 1812-12 | 273.776 | -12.096 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 4U 1705-44 | 257.227 | -44.102 | 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. |
| 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. |
| 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. |
| 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 1735-444 | 264.743 | -44.450 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| UW CrB | 241.441 | 25.863 | 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. |
| 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. |
| 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. |
| Cen X-4 | 224.591 | -31.669 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| Cir X-1 | 230.170 | -57.167 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 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. |
| 4U 1850-086 | 283.270 | -8.705 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| IGR J18245-2452 | 276.135 | -24.869 | Sanchez-Fernandez | 1330016 | 1320023 1320002 1320004 1320019 1320027 | Type-I X-ray bursts. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 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. |
| 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 | |
| IGR J18175-2419 | 274.470 | -24.329 | Sidoli | 1330012 | 1320023 | |
| IGR J17541-2252 | 268.525 | -22.867 | Sidoli | 1330012 | 1320023 | |
| IGR J18159-3353 | 273.988 | -33.890 | Sidoli | 1330012 | 1320023 | |
| SAX J1818.6–1703 | 274.658 | -17.047 | Sidoli | 1330012 | 1320023 | |
| IGR J17354-3255 | 263.854 | -32.938 | Sidoli | 1330012 | 1320023 | |
| 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 | |
| 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) |
| 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) |
| 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) |
| 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) |
| 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) |
| VelaX-1 | 135.529 | -40.555 | Watanabe | 1330003 | 1320004 1320002 1320027 1320019 1320023 | |
| 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) |
| 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) |
| 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) |
| 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) |
| 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) |
| 4U1626-67 | 248.070 | -67.462 | Watanabe | 1330003 | 1320004 1320002 1320027 1320019 1320023 | |
| 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) |
| 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) |
| 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) |
| 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) |
| 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) |
| 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) |
| 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) |
| 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) |
| 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) |
| GRS 1737-31 | 265.025 | -31.033 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| KS 1730-312 | 263.383 | -31.217 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| XTE J1755-324 | 268.887 | -32.495 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| GRS 1739-278 | 265.665 | -27.748 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| SAX J1711.6-3808 | 257.892 | -38.122 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| H 1743-322 | 266.567 | -32.234 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| XTE J1720-318 | 259.975 | -31.749 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| V4641 Sgr | 274.840 | -25.407 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| IGR J17285-2922 | 262.171 | -29.382 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| XTE J1817-330 | 274.431 | -33.019 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| XTE J1752-223 | 268.063 | -22.343 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| 4U 1755-338 | 269.667 | -33.808 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| XTE J1748-288 | 267.000 | -28.483 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| MAXI J1659-152 | 254.792 | -15.268 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| IGR J17091-3624 | 257.279 | -36.407 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| XTE J1818-245 | 274.603 | -24.538 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| GRS 1716-249 | 259.904 | -25.018 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| Swift J174510.8-262411 | 266.295 | -26.403 | Wilms | 1330010 | 1320002 1320027 1320023 | |
| SGR A* | 266.417 | -29.008 | Wilms | 1330023 | 1320023 |
| SOURCE NAME | RA | DEC | PI | PROP ID | Open Time Proposals | TAC Data Rights Strategy |
|---|---|---|---|---|---|---|
| H 1145-619 | 177.000 | -62.207 | Alfonso-Garzon | 1340028 | 1340028 | |
| New BH Transient | 0.000 | 0.000 | Belloni | 1340010 | 1340010 | |
| XTE J0421+560 | 64.925 | 56.000 | Belloni | 1340010 | 1340010 | |
| GRO J0422+32 | 65.428 | 32.909 | Belloni | 1340010 | 1340010 | |
| 1A 0620-00 | 95.685 | -0.346 | Belloni | 1340010 | 1340010 | |
| GRS 1009-45 | 153.401 | -45.076 | Belloni | 1340010 | 1340010 | |
| XTE J1118+480 | 169.545 | 48.037 | Belloni | 1340010 | 1340010 | |
| GS 1124-68 | 171.611 | -68.676 | Belloni | 1340010 | 1340010 | |
| GS 1354-645 | 209.540 | -64.735 | Belloni | 1340010 | 1340010 | |
| 4U 1524-617 | 232.070 | -61.883 | Belloni | 1340010 | 1340010 | |
| 4U 1543-475 | 236.786 | -47.669 | Belloni | 1340010 | 1340010 | |
| XTE J1550-564 | 237.745 | -56.477 | Belloni | 1340010 | 1340010 | |
| XTE J1650-500 | 252.504 | -49.962 | Belloni | 1340010 | 1340010 | |
| GRO J1655-40 | 253.500 | -39.846 | Belloni | 1340010 | 1340010 | |
| H 1705-250 | 257.069 | -25.091 | Belloni | 1340010 | 1340010 | |
| SAX J1711.6-3808 | 257.905 | -38.118 | Belloni | 1340010 | 1340010 | |
| GRS 1716-249 | 259.904 | -25.018 | Belloni | 1340010 | 1340010 | |
| XTE J1720-318 | 259.992 | -31.780 | Belloni | 1340010 | 1340010 | |
| KS 1730-312 | 263.407 | -31.220 | Belloni | 1340010 | 1340010 | |
| GRS 1737-31 | 265.038 | -31.040 | Belloni | 1340010 | 1340010 | |
| GRS 1739-278 | 265.667 | -27.748 | Belloni | 1340010 | 1340010 | |
| 1A 1742-289 | 266.405 | -29.018 | Belloni | 1340010 | 1340010 | |
| H1743-322 | 266.565 | -32.234 | Belloni | 1340010 | 1340010 | |
| XTE J1748-288 | 267.023 | -28.474 | Belloni | 1340010 | 1340010 | |
| SLX 1746-331 | 267.461 | -33.199 | Belloni | 1340010 | 1340010 | |
| XTE J1755-324 | 268.869 | -32.478 | Belloni | 1340010 | 1340010 | |
| 4U 1755-338 | 269.667 | -33.808 | Belloni | 1340010 | 1340010 | |
| XTE J1819-254 | 274.840 | -25.407 | Belloni | 1340010 | 1340010 | |
| EXO 1846-031 | 282.317 | -3.068 | Belloni | 1340010 | 1340010 | |
| XTE J1859+226 | 284.673 | 22.658 | Belloni | 1340010 | 1340010 | |
| XTE J1908+094 | 287.224 | 9.385 | Belloni | 1340010 | 1340010 | |
| 4U 1957+11 | 299.850 | 11.708 | Belloni | 1340010 | 1340010 | |
| GS 2000+251 | 300.707 | 25.236 | Belloni | 1340010 | 1340010 | |
| XTE J2012+381 | 303.158 | 38.184 | Belloni | 1340010 | 1340010 | |
| GS 2023+338 | 306.016 | 33.868 | Belloni | 1340010 | 1340010 | |
| XTE J1817-330 | 274.431 | -33.019 | Belloni | 1340010 | 1340010 | |
| GX 339-4 | 255.706 | -48.790 | Belloni | 1340010 | 1340010 | |
| Swift J1753.5-0127 | 268.368 | -1.452 | Belloni | 1340010 | 1340010 | |
| Swift J1539.2-6227 | 234.800 | -62.467 | Belloni | 1340010 | 1340010 | |
| Swift J1842.5-1124 | 280.500 | -11.400 | Belloni | 1340010 | 1340010 | |
| XTE J1652-453 | 253.085 | -45.344 | Belloni | 1340010 | 1340010 | |
| XTE J1752-223 | 268.000 | -22.300 | Belloni | 1340010 | 1340010 | |
| XTE J1818-245 | 274.605 | -24.542 | Belloni | 1340010 | 1340010 | |
| IGR J17497-2821 | 267.409 | -28.355 | Belloni | 1340010 | 1340010 | |
| MAXI J1659-152 | 254.756 | -15.258 | Belloni | 1340010 | 1340010 | |
| Swift J1357.2-0933 | 209.320 | -9.544 | Belloni | 1340010 | 1340010 | |
| Swift J17091-3624 | 257.282 | -36.407 | Belloni | 1340010 | 1340010 | |
| MAXI J1543-564 | 235.823 | -56.414 | Belloni | 1340010 | 1340010 | |
| MAXI J1836-194 | 278.931 | -19.320 | Belloni | 1340010 | 1340010 | |
| MAXI J1828-249 | 277.118 | -24.906 | Belloni | 1340010 | 1340010 | |
| MAXI J1305-704 | 196.731 | -70.450 | Belloni | 1340010 | 1340010 | |
| Swift J174510.8-2624 | 266.295 | -26.405 | Belloni | 1340010 | 1340010 | |
| MAXI J1421-613 | 215.413 | -61.345 | 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 | |
| SAX J1808.4-3658 | 272.115 | -36.979 | Ferrigno | 1340020 | 1340020 | |
| XTE J1751-305 | 267.806 | -30.623 | Ferrigno | 1340020 | 1340020 | |
| XTE J0929-314 | 142.334 | -31.384 | Ferrigno | 1340020 | 1340020 | |
| XTE J1807-294 | 271.749 | -29.408 | Ferrigno | 1340020 | 1340020 | |
| XTE J1814-338 | 273.413 | -33.773 | Ferrigno | 1340020 | 1340020 | |
| IGR J00291+5934 | 7.263 | 59.572 | Ferrigno | 1340020 | 1340020 | |
| HETE J1900.1-2455 | 285.036 | -24.920 | Ferrigno | 1340020 | 1340020 | |
| swift J1756.9-2508 | 269.238 | -25.107 | Ferrigno | 1340020 | 1340020 | |
| IGR J17498-2921 | 267.450 | -29.350 | Ferrigno | 1340020 | 1340020 | |
| SWIFT J1749.4-2807 | 267.383 | -28.135 | Ferrigno | 1340020 | 1340020 | |
| IGR J17511-3057 | 267.786 | -30.961 | Ferrigno | 1340020 | 1340020 | |
| IGR J18245-2452 | 276.111 | -24.857 | 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 | |
| XTE J1810-197 | 272.462 | -19.731 | Götz | 1340012 | 1340012 | |
| CXO J164710.2-455216 | 251.792 | -45.871 | Götz | 1340012 | 1340012 | |
| CXOU 010043-7211 | 17.679 | -72.193 | Götz | 1340012 | 1340012 | |
| 4U 0142+614 | 26.592 | 61.751 | Götz | 1340012 | 1340012 | |
| 1E 1048.1-5937 | 162.529 | -59.889 | Götz | 1340012 | 1340012 | |
| 1RXS J170849-400910 | 257.192 | -40.148 | Götz | 1340012 | 1340012 | |
| 1E 1841-045 | 280.333 | -4.936 | Götz | 1340012 | 1340012 | |
| AX J1844-0258 | 281.229 | -2.948 | Götz | 1340012 | 1340012 | |
| 1E 2259+586 | 345.283 | 58.879 | Götz | 1340012 | 1340012 | |
| 1E 1547.0–5408 | 237.729 | -54.322 | Götz | 1340012 | 1340012 | |
| SGR 0501+4516 | 75.265 | 45.272 | Götz | 1340012 | 1340012 | |
| SGR 1900+14 | 286.810 | 9.323 | Götz | 1340012 | 1340012 | |
| SGR 1806-20 | 272.164 | -20.411 | Götz | 1340012 | 1340012 | |
| SGR 0525-66 | 81.504 | -66.077 | Götz | 1340012 | 1340012 | |
| SGR 1627-41 | 248.966 | -47.590 | Götz | 1340012 | 1340012 | |
| SGR 1801-23 | 269.488 | -22.947 | Götz | 1340012 | 1340012 | |
| SGR 0418+5729 | 64.642 | 57.540 | Götz | 1340012 | 1340012 | |
| SGR 1833-0832 | 278.435 | -8.519 | Götz | 1340012 | 1340012 | |
| CXOUJ171405.7-381031 | 258.524 | -38.175 | Götz | 1340012 | 1340012 | |
| PSR J1846-0258 | 281.602 | -2.974 | Götz | 1340012 | 1340012 | |
| PSR J1622-4950 | 245.687 | -49.848 | Götz | 1340012 | 1340012 | |
| Swift J1822.3-1606 | 275.576 | -16.074 | Götz | 1340012 | 1340012 | |
| Swift J1834.9-0846 | 278.725 | -8.767 | Götz | 1340012 | 1340012 | |
| AX J1818.8-1559 | 274.717 | -15.989 | Götz | 1340012 | 1340012 | |
| SGR 2013+34 | 303.487 | 34.330 | Götz | 1340012 | 1340012 | |
| SGR J1745-2900 | 266.417 | -29.008 | Götz | 1340012 | 1340012 | |
| 3XMM J1852+0033 | 283.194 | -0.556 | Götz | 1340012 | 1340012 | |
| SGR 1935+2154 | 293.732 | 21.897 | Götz | 1340012 | 1340012 | |
| Classical Nova | 0.000 | 0.000 | Hernanz | 1340026 | 1340026 | |
| FermiTransient1 | 0.000 | 0.000 | Hill | 1340029 | 1340029 | |
| GRS 1758-258 | 270.303 | -25.741 | Hirsch | 1340018 | 1340018 | |
| 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 | |
| GRO J0422+32 | 65.428 | 32.909 | Kalemci | 1340009 | 1340009 | |
| A0620-00 | 95.685 | -0.346 | Kalemci | 1340009 | 1340009 | |
| GRS 1009-45 | 153.401 | -45.076 | Kalemci | 1340009 | 1340009 | |
| XTE J1118+480 | 169.545 | 48.037 | Kalemci | 1340009 | 1340009 | |
| GS 1124-68 | 171.611 | -68.676 | Kalemci | 1340009 | 1340009 | |
| GS 1354-645 | 209.540 | -64.735 | Kalemci | 1340009 | 1340009 | |
| X 1524-617 | 232.070 | -61.883 | Kalemci | 1340009 | 1340009 | |
| 4U 1543-475 | 236.786 | -47.669 | Kalemci | 1340009 | 1340009 | |
| XTE J1550-564 | 237.745 | -56.477 | Kalemci | 1340009 | 1340009 | |
| XTE J1650-500 | 252.504 | -49.962 | Kalemci | 1340009 | 1340009 | |
| GRO J1655-40 | 253.500 | -39.846 | Kalemci | 1340009 | 1340009 | |
| H 1705-250 | 257.069 | -25.091 | Kalemci | 1340009 | 1340009 | |
| SAX J1711.6-3808 | 257.905 | -38.118 | Kalemci | 1340009 | 1340009 | |
| GRS 1716-249 | 259.904 | -25.018 | Kalemci | 1340009 | 1340009 | |
| XTE J1720-318 | 259.992 | -31.780 | Kalemci | 1340009 | 1340009 | |
| KS 1730-312 | 263.386 | -31.217 | Kalemci | 1340009 | 1340009 | |
| GRS 1737-31 | 265.038 | -31.040 | Kalemci | 1340009 | 1340009 | |
| GRS 1739-278 | 265.667 | -27.748 | Kalemci | 1340009 | 1340009 | |
| A 1742-289 | 266.405 | -29.018 | Kalemci | 1340009 | 1340009 | |
| H1743-322 | 266.565 | -32.234 | Kalemci | 1340009 | 1340009 | |
| XTE J1748-288 | 267.023 | -28.474 | Kalemci | 1340009 | 1340009 | |
| SLX 1746-331 | 267.461 | -33.199 | Kalemci | 1340009 | 1340009 | |
| XTE J1755-324 | 268.869 | -32.478 | Kalemci | 1340009 | 1340009 | |
| 4U 1755-338 | 269.667 | -33.808 | Kalemci | 1340009 | 1340009 | |
| X 1819-25 | 274.840 | -25.407 | Kalemci | 1340009 | 1340009 | |
| EXO 1846-031 | 282.321 | -3.062 | Kalemci | 1340009 | 1340009 | |
| XTE J1859+226 | 284.673 | 22.658 | Kalemci | 1340009 | 1340009 | |
| XTE J1908+094 | 287.224 | 9.385 | Kalemci | 1340009 | 1340009 | |
| 4U 1957+11 | 299.850 | 11.708 | Kalemci | 1340009 | 1340009 | |
| GS 2000+251 | 300.707 | 25.236 | Kalemci | 1340009 | 1340009 | |
| XTE J2012+381 | 303.158 | 38.184 | Kalemci | 1340009 | 1340009 | |
| GS 2023+338 | 306.016 | 33.868 | Kalemci | 1340009 | 1340009 | |
| XTE J1817-330 | 274.431 | -33.019 | Kalemci | 1340009 | 1340009 | |
| SWIFT J1753.5-0127 | 268.368 | -1.452 | Kalemci | 1340009 | 1340009 | |
| IGR J17497-2821 | 267.409 | -28.355 | Kalemci | 1340009 | 1340009 | |
| XTE J1752-322 | 268.000 | -22.300 | Kalemci | 1340009 | 1340009 | |
| Swift J1539.2-6227 | 234.800 | -62.467 | Kalemci | 1340009 | 1340009 | |
| Swift J1842.5-1124 | 280.500 | -11.400 | Kalemci | 1340009 | 1340009 | |
| XTE J1652-453 | 253.085 | -45.344 | Kalemci | 1340009 | 1340009 | |
| XTE J1818-245 | 274.605 | -24.542 | Kalemci | 1340009 | 1340009 | |
| XTE J1752-223 | 268.000 | -22.300 | Kalemci | 1340009 | 1340009 | |
| IGR J17091-3624 | 257.283 | -36.407 | Kalemci | 1340009 | 1340009 | |
| IGR J17177-3656 | 259.427 | -36.935 | Kalemci | 1340009 | 1340009 | |
| MAXI J1659-152 | 254.792 | -15.268 | Kalemci | 1340009 | 1340009 | |
| MAXI J1836-194 | 278.931 | -19.320 | Kalemci | 1340009 | 1340009 | |
| MAXI J1543-564 | 235.823 | -56.414 | Kalemci | 1340009 | 1340009 | |
| SWIFT J1357.2-0933 | 209.325 | -9.552 | Kalemci | 1340009 | 1340009 | |
| SWIFT J174510.8-2624 | 266.295 | -26.400 | Kalemci | 1340009 | 1340009 | |
| Mrk 421 | 166.114 | 38.209 | Kreikenbohm | 1340027 | 1340027 | |
| Mrk 501 | 253.468 | 39.760 | Kreikenbohm | 1340027 | 1340027 | |
| New Transient Pulsar | 0.000 | 0.000 | Kreykenbohm | 1340013 | 1340013 | |
| AX J0049-729 | 12.275 | -72.847 | Kreykenbohm | 1340013 | 1340013 | |
| AX J0051-722 | 12.732 | -72.232 | Kreykenbohm | 1340013 | 1340013 | |
| 2E 0050.1-7247 | 12.972 | -72.530 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0052.1-7319 | 13.058 | -73.320 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0053.8-7226 | 13.479 | -72.446 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0052.9-7158 | 13.230 | -71.968 | 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 | |
| PSR J0111-7317 | 17.785 | -73.279 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0117.6-7330 | 19.422 | -73.514 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0502.9-6626 | 75.715 | -66.440 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0529.8-6556 | 82.452 | -65.948 | Kreykenbohm | 1340013 | 1340013 | |
| EXO 053109-6609.2 | 82.805 | -66.118 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0535.6-6651 | 83.919 | -66.865 | Kreykenbohm | 1340013 | 1340013 | |
| AX J0544.1-7100 | 86.026 | -71.014 | Kreykenbohm | 1340013 | 1340013 | |
| 3A 0726-260 | 112.222 | -26.108 | Kreykenbohm | 1340013 | 1340013 | |
| RX J0812.4-3114 | 123.118 | -31.248 | Kreykenbohm | 1340013 | 1340013 | |
| Ginga 0834-430 | 128.979 | -43.185 | Kreykenbohm | 1340013 | 1340013 | |
| H 1145-619 | 177.000 | -62.207 | Kreykenbohm | 1340013 | 1340013 | |
| H 1417-624 | 215.304 | -62.698 | Kreykenbohm | 1340013 | 1340013 | |
| AX J1749.2-2725 | 267.292 | -27.421 | Kreykenbohm | 1340013 | 1340013 | |
| Sct X-1 | 278.858 | -7.614 | Kreykenbohm | 1340013 | 1340013 | |
| Ginga 1839-04 | 280.450 | -4.450 | Kreykenbohm | 1340013 | 1340013 | |
| 3A 1845-024 | 282.074 | -2.420 | Kreykenbohm | 1340013 | 1340013 | |
| Ginga 1855-02 | 284.500 | -2.733 | Kreykenbohm | 1340013 | 1340013 | |
| XTE J1858+034 | 284.679 | 3.439 | Kreykenbohm | 1340013 | 1340013 | |
| GRO J2058+42 | 314.750 | 41.717 | Kreykenbohm | 1340013 | 1340013 | |
| XTE J1543-568 | 236.008 | -56.712 | Kreykenbohm | 1340013 | 1340013 | |
| IGR J16358-4726 | 248.974 | -47.428 | Kreykenbohm | 1340013 | 1340013 | |
| GRO J1744-28 | 266.138 | -28.741 | Kreykenbohm | 1340013 | 1340013 | |
| 1A 1744-361 | 267.080 | -36.121 | Kreykenbohm | 1340013 | 1340013 | |
| XTE J1855-026 | 283.880 | -2.607 | Kreykenbohm | 1340013 | 1340013 | |
| 4U 1901+03 | 285.905 | 3.192 | Kreykenbohm | 1340013 | 1340013 | |
| SAX J2103.5+4545 | 315.899 | 45.752 | Kreykenbohm | 1340013 | 1340013 | |
| 4U 1036-56 | 159.398 | -56.803 | Kreykenbohm | 1340013 | 1340013 | |
| V0332+53 | 53.750 | 53.173 | Lutovinov | 1340023 | 1340023 | |
| GRB041219 | 6.112 | 62.843 | Martin-Carrillo | 1340030 | 1340030 | |
| XTE J 1701-462 | 255.244 | -46.186 | Paizis | 1340014 | 1340014 | |
| TDE | 0.000 | 0.000 | Panessa | 1340003 | 1340003 | |
| PSR J1723-2837 | 260.847 | -28.633 | Papitto | 1340024 | 1340024 | |
| PMN J0017-0512 | 4.399 | -5.212 | Pian | 1340015 | 1340015 | |
| RBS 0076 | 8.393 | -19.359 | Pian | 1340015 | 1340015 | |
| 1ES 0033+595 | 8.969 | 59.835 | Pian | 1340015 | 1340015 | |
| PKS 0048-097 | 12.672 | -9.485 | Pian | 1340015 | 1340015 | |
| PKS 0048-071 | 12.784 | -6.834 | Pian | 1340015 | 1340015 | |
| S2 0109+22 | 18.024 | 22.744 | Pian | 1340015 | 1340015 | |
| 4C 31.03 | 18.210 | 32.138 | Pian | 1340015 | 1340015 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| PKS B0528+134 | 82.735 | 13.532 | Pian | 1340015 | 1340015 | |
| PMN J0531-4827 | 82.994 | -48.460 | Pian | 1340015 | 1340015 | |
| PMN J0532+0732 | 83.162 | 7.545 | Pian | 1340015 | 1340015 | |
| PKS 0537-441 | 84.710 | -44.086 | Pian | 1340015 | 1340015 | |
| PKS 0548-322 | 87.670 | -32.272 | Pian | 1340015 | 1340015 | |
| H 0557-385 | 89.508 | -38.335 | Pian | 1340015 | 1340015 | |
| B2 0619+33 | 95.718 | 33.436 | Pian | 1340015 | 1340015 | |
| 1ES 0647+250 | 102.694 | 25.050 | Pian | 1340015 | 1340015 | |
| CJ2 0650+453 | 103.599 | 45.240 | Pian | 1340015 | 1340015 | |
| GB6 J0654+5042 | 103.595 | 50.707 | 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| RBS 0958 | 169.276 | 20.236 | Pian | 1340015 | 1340015 | |
| PKS 1118-056 | 170.355 | -5.899 | Pian | 1340015 | 1340015 | |
| 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 | |
| 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 | |
| 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 | |
| PKS 1406-076 | 212.235 | -7.874 | Pian | 1340015 | 1340015 | |
| 1E 1415.6+2557 | 214.486 | 25.724 | Pian | 1340015 | 1340015 | |
| 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 | |
| 1ES 1544+820 | 235.067 | 81.918 | Pian | 1340015 | 1340015 | |
| GB6 J1542+6129 | 235.737 | 61.499 | Pian | 1340015 | 1340015 | |
| PKS 1551+130 | 238.386 | 12.948 | Pian | 1340015 | 1340015 | |
| PG 1553+113 | 238.930 | 11.190 | Pian | 1340015 | 1340015 | |
| 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 | |
| Mkn 501 | 253.468 | 39.760 | Pian | 1340015 | 1340015 | |
| GB6 J1700+6830 | 255.039 | 68.502 | Pian | 1340015 | 1340015 | |
| B3 1708+433 | 257.424 | 43.312 | Pian | 1340015 | 1340015 | |
| PKS 1717+177 | 259.806 | 17.752 | Pian | 1340015 | 1340015 | |
| 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 | |
| 1ES 1741+196 | 265.991 | 19.586 | Pian | 1340015 | 1340015 | |
| S4 1749+70 | 267.137 | 70.097 | Pian | 1340015 | 1340015 | |
| PKS 1749+096 | 267.887 | 9.650 | Pian | 1340015 | 1340015 | |
| S5 1803+784 | 270.192 | 78.468 | Pian | 1340015 | 1340015 | |
| PMN J1802-3940 | 270.678 | -39.669 | Pian | 1340015 | 1340015 | |
| PKS 1830-21 | 278.416 | -21.061 | Pian | 1340015 | 1340015 | |
| TXS 1846+322 | 282.095 | 32.317 | Pian | 1340015 | 1340015 | |
| S4 1849+67 | 282.320 | 67.095 | Pian | 1340015 | 1340015 | |
| 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 | |
| 1ES 1959+650 | 299.999 | 65.149 | Pian | 1340015 | 1340015 | |
| PKS 2004-447 | 301.980 | -44.579 | Pian | 1340015 | 1340015 | |
| PKS 2005-489 | 302.356 | -48.832 | Pian | 1340015 | 1340015 | |
| PKS B2022-077 | 306.418 | -7.595 | Pian | 1340015 | 1340015 | |
| PKS 2052-474 | 314.068 | -47.247 | Pian | 1340015 | 1340015 | |
| 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 | |
| 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 | |
| GRB1 | 0.000 | 0.000 | Pozanenko | 1340007 | 1340007 | |
| GRB outside the FoV | 0.000 | 0.000 | Savchenko | 1340021 | 1340021 |
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