Cygnus
| Source | ID | Flux, mCrab | Sign. |
|---|---|---|---|
| M 1812-12 | 095 | 25.83 ± 0.32 PHA | 80.22 |
| GX 17+2 | 096 | 82.06 ± 0.34 PHA | 238.16 |
| 4U 1822-000 | 100 | 2.16 ± 0.32 PHA | 6.84 |
| SNR 021.5-00.9 | 104 | 3.47 ± 0.27 PHA | 12.78 |
| AX J1838.0-0655 | 107 | 1.57 ± 0.26 PHA | 6.16 |
| Ser X-1 | 108 | 11.62 ± 0.35 PHA | 33.03 |
| 1E1841-045 | 109 | 1.76 ± 0.26 PHA | 6.75 |
| GS 1843+00 | 110 | 14.94 ± 0.31 PHA | 48.95 |
| PSR J1846-0258 | 111 | 2.09 ± 0.28 PHA | 7.60 |
| IGR J18483-0311 | 112 | 5.66 ± 0.28 PHA | 20.51 |
| 4U 1850-087 | 113 | 2.92 ± 0.27 PHA | 10.71 |
| XTE J1855-026 | 115 | 9.68 ± 0.29 PHA | 33.44 |
| XTE J1901+014 | 116 | 2.15 ± 0.32 PHA | 6.76 |
| 4U 1907+097 | 118 | 9.19 ± 0.33 PHA | 27.47 |
| X1908+075 | 119 | 17.18 ± 0.33 PHA | 52.60 |
| SS 433 | 120 | 5.30 ± 0.33 PHA | 16.02 |
| IGR J19140+0951 | 121 | 6.68 ± 0.34 PHA | 19.83 |
| GRS 1915+105 | 122 | 360.85 ± 0.34 PHA | 1049.96 |
| 4U 1916-053 | 123 | 9.13 ± 0.37 PHA | 24.85 |
| RX J1940.2-1025 | 124 | 3.09 ± 0.46 PHA | 6.77 |
| Cyg X-1 | 126 | 791.49 ± 0.40 PHA | 1957.68 |
| EXO 2030+375 | 127 | 33.30 ± 0.34 PHA | 98.04 |
| Cyg X-3 | 128 | 162.26 ± 0.33 PHA | 493.00 |
| Cygnus A | 174 | 4.83 ± 0.39 PHA | 12.46 |
| Aql X-1 | 175 | 5.71 ± 0.34 PHA | 17.03 |
| NGC 6814 | 178 | 2.52 ± 0.45 PHA | 5.61 |
| IGR J18214-1318 | 186 | 1.73 ± 0.32 PHA | 5.40 |
| 4U1954+319 | 230 | 8.30 ± 0.45 PHA | 18.26 |
| IGR J20187+4041 | 297 | 1.93 ± 0.34 PHA | 5.67 |
| SWIFT J1753.5-0127 | 333 | 100.04 ± 0.42 PHA | 236.59 |
| SWIFT J2000.6+3210 | 396 | 3.14 ± 0.44 PHA | 7.16 |
| IGR J18284-0345 | 489 | 2.03 ± 0.27 PHA | 7.47 |
| IGR J19294+1816 | 820 | 2.63 ± 0.55 PHA | 4.80 |
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