Perseus Arm
Source | ID | Flux, mCrab | Sign. |
---|---|---|---|
1A 0114+650 | 001 | 9.00 ± 0.27 PHA | 33.30 |
IGR J21247+5058 | 130 | 6.77 ± 0.25 PHA | 26.73 |
SS Cyg | 131 | 3.84 ± 0.30 PHA | 12.68 |
Cyg X-2 | 132 | 20.59 ± 0.39 PHA | 53.00 |
4U 2206+543 | 133 | 4.60 ± 0.51 PHA | 9.06 |
Gamma Cas | 160 | 2.94 ± 0.30 PHA | 9.88 |
V709 Cas | 162 | 3.65 ± 0.37 PHA | 9.78 |
IGR J21335+5105 | 173 | 2.63 ± 0.28 PHA | 9.50 |
4U 0241+61 | 222 | 3.20 ± 0.45 PHA | 7.07 |
4U0142+61 | 263 | 2.37 ± 0.29 PHA | 8.12 |
IGR J21178+5139 | 294 | 1.29 ± 0.24 PHA | 5.30 |
IGR J21277+5656 | 298 | 1.95 ± 0.29 PHA | 6.72 |
4U0115+63 | 366 | 141.67 ± 0.27 PHA | 523.68 |
IGR J21358+4729 | 616 | 1.31 ± 0.27 PHA | 4.82 |
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