Cygnus
| Source | ID | Flux, mCrab | Sign. |
|---|---|---|---|
| IGR J17303-0601 | 057 | 2.92 ± 0.29 PHA | 10.21 |
| M 1812-12 | 095 | 24.53 ± 0.24 PHA | 100.93 |
| GX 17+2 | 096 | 52.52 ± 0.26 PHA | 201.76 |
| SNR 021.5-00.9 | 104 | 2.63 ± 0.25 PHA | 10.41 |
| AX J1838.0-0655 | 107 | 1.79 ± 0.25 PHA | 7.27 |
| Ser X-1 | 108 | 7.84 ± 0.24 PHA | 32.16 |
| 1E1841-045 | 109 | 2.49 ± 0.25 PHA | 9.92 |
| PSR J1846-0258 | 111 | 1.71 ± 0.26 PHA | 6.64 |
| IGR J18483-0311 | 112 | 1.80 ± 0.26 PHA | 6.89 |
| 4U 1850-087 | 113 | 3.44 ± 0.28 PHA | 12.16 |
| XTE J1855-026 | 115 | 7.59 ± 0.27 PHA | 28.36 |
| XTE J1901+014 | 116 | 2.10 ± 0.24 PHA | 8.73 |
| 4U 1907+097 | 118 | 7.70 ± 0.22 PHA | 34.49 |
| X1908+075 | 119 | 10.68 ± 0.22 PHA | 49.39 |
| SS 433 | 120 | 10.24 ± 0.22 PHA | 46.65 |
| IGR J19140+0951 | 121 | 9.95 ± 0.23 PHA | 44.17 |
| GRS 1915+105 | 122 | 212.45 ± 0.23 PHA | 910.71 |
| 4U 1916-053 | 123 | 9.16 ± 0.29 PHA | 31.60 |
| RX J1940.2-1025 | 124 | 2.36 ± 0.25 PHA | 9.37 |
| Cyg X-1 | 126 | 814.12 ± 0.28 PHA | 2958.50 |
| EXO 2030+375 | 127 | 41.49 ± 0.21 PHA | 200.57 |
| Cyg X-3 | 128 | 49.80 ± 0.20 PHA | 251.30 |
| Cygnus A | 174 | 4.38 ± 0.25 PHA | 17.35 |
| NGC 6814 | 178 | 3.66 ± 0.25 PHA | 14.49 |
| IGR J18214-1318 | 186 | 1.26 ± 0.26 PHA | 4.92 |
| IGR J18490-0000 | 213 | 1.29 ± 0.25 PHA | 5.17 |
| 4U1954+319 | 230 | 24.57 ± 0.32 PHA | 77.51 |
| IGR J20187+4041 | 297 | 1.10 ± 0.21 PHA | 5.23 |
| SWIFT J1753.5-0127 | 333 | 73.80 ± 0.23 PHA | 319.74 |
| SWIFT J2000.6+3210 | 396 | 3.20 ± 0.30 PHA | 10.66 |
| IGR J20159+3713 | 620 | 1.28 ± 0.22 PHA | 5.78 |
| Swift j1842.5-1124 | 872 | 1.30 ± 0.27 PHA | 4.76 |
Description
- The map above is movable. The image is shown in significance with a squared root color map ranging from 0 to 25. The black and blue colors correspond to pixel values from 0 to 2. The red pixels have values of around 5. The yellow to white color transition corresponds to 15 and more.
- The regions of high systematic noise are shown with yellow circles.
- Clean button loads sky mosaics made without pointings on bright sources to suppress systematics. Original shows mosaics with all data available.
Download FITS files
- Flux mapError mapSignificanceExposure
Flux and error maps are in mCrab units. All maps are convolved with instrumental point spread function (PSF) which is Gaussian (σ=5'). Exposure maps are in ksec.
Reference