Perseus Arm
Source | ID | Flux, mCrab | Sign. |
---|---|---|---|
SAX J2103.5+4545 | 129 | 12.95 ± 0.20 PHA | 63.29 |
IGR J21247+5058 | 130 | 7.04 ± 0.17 PHA | 42.60 |
SS Cyg | 131 | 2.74 ± 0.23 PHA | 11.87 |
Cyg X-2 | 132 | 26.86 ± 0.41 PHA | 65.31 |
4U 2206+543 | 133 | 7.03 ± 0.17 PHA | 40.36 |
Gamma Cas | 160 | 6.57 ± 0.52 PHA | 12.75 |
Cas A | 161 | 3.31 ± 0.49 PHA | 6.76 |
V709 Cas | 162 | 3.48 ± 0.71 PHA | 4.92 |
IGR J21335+5105 | 173 | 2.83 ± 0.16 PHA | 17.40 |
IGR J21277+5656 | 298 | 2.19 ± 0.18 PHA | 12.37 |
IGR J21358+4729 | 616 | 0.92 ± 0.18 PHA | 5.09 |
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