Table A.2
Properties of the X-ray instruments.
| Satellite | Detector | Field of view | Energy (keV) | PSF (FWHM) | Data link | Catalog names |
|---|---|---|---|---|---|---|
| Chandra | ACIS | 17′ × 17′ | 0.5–7.0 | 1″ | [1]* | CSC2(a) |
| Suzaku | XIS | 19′ × 19′ | 0.2–12.0 | <1.5′ | [2] | – |
| XMM-Newton | EPIC (MOS1-2) | 30′ × 30′ | 0.2–12.0 | 6″ | [3]* | 4XMM-DR9(b) |
| EPIC (PN) | 30′ × 30′ | 0.2–12.0 | 6″ | |||
| ASCA | SIS | 22′ × 22′ | 0.4–12.0 | 1′ | [4]* | GIS/SIS/Galactic Plane Survey(c) |
| GIS | 20′ × 20′ | 0.6–12.0 | 1′ | |||
| Swift | XRT | 23.6′ × 23.6′ | 0.2–10.0 | 18″* | [5]* | 1SWXRT/2SXPS(d) |
| BAT | 5400′ × 3000′ | 14–195 | 17′ | [6]* | BS105 months(e) | |
| Integral | IBIS | 1140′ × 1140′ | 17–60 | 12′ | [7]* | 8-1 yr All sky and 9-14 Galactic sky(f) |
| NuSTAR | – | 13′ × 13′ | 5–80 | 7.5″ | [8]* | Survey source catalog (Fornasini et al. 2017) |
| ROSAT | PSPC | 114′ × 114′ | 0.1–2.4 | 45″ | [9]* | 1RXS (Voges et al. 1999) |
| 2RXS (Boller et al. 2016) |
Notes. The Swift/XRT PSF (noted with an asterisk) corresponds to the half-power diameter. The links to retrieve these data are labeled with numbers and given below. Numbers followed by an asterisk indicate that a source catalog, associated with the instrument, is available and used. (a) http://cxc.cfa.harvard.edu/csc2/. (b) http://xmmssc.irap.omp.eu/Catalogue/4XMM-DR9/4XMM_DR9.html, Webb et al. (2020). (c) https://heasarc.gsfc.nasa.gov/W3Browse/all/ascasis.html (same for ascagis.html and ascagps.html). (d) http://www.asdc.asi.it/1swxrt/, http://www.swift.ac.uk/2SXPS/, D’Elia et al. (2013), Evans et al. (2020). (e) https://swift.gsfc.nasa.gov/results/bs105mon/. (f) https://heasarc.gsfc.nasa.gov/W3Browse/integral/ibiscat.html, https://heasarc.gsfc.nasa.gov/w3browse/all/intibisvhd.html, https://heasarc.gsfc.nasa.gov/w3browse/all/intibisgal.html, http://hea.iki.rssi.ru/integral/fourteen-years-galactic-survey/.
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