5XMM J174750.2-283737
5XMM-DR15 stacked source · SRCID 3003054010101140
Position:
17h47m50.25s -28d37m37.3s
(266.95937°, -28.62702°)
EP flux
1.39e-13
± 1.4e-14
erg cm-2 s-1
CLASSX
Gal_XRB
(0.937)
Detections
11
| SRCID | 3003054010101140 |
|---|---|
| IAUNAME | 5XMM J174750.2-283737 |
| SC_RA | 17h47m50.25s (266.95937°) |
| SC_DEC | -28d37m37.3s (-28.62702°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 0.5164° / -0.2548° |
| N_CONTRIB | 11 (detections) |
| N_OBS | 308 (observations covering the position) |
| MJD_FIRST | 51802.795 (2000-09-15 19:04:46.000 UTC) |
| MJD_LAST | 59120.587 (2020-09-28 14:05:30.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.39e-13 ± 1.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.07
± 0.96
0.2-0.5 / 0.5-1.0 keV
HR2
0.93
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
0.75
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
0.23
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 3.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 5.87
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.20e-13 (+1.4e-13 / −1.1e-13) erg cm−2 s−1 |
|---|---|
| NH | 5.82e+22 (+7.8e+22 / −4.3e+22) cm−2 |
| Photon index (Γ) | 1.32 (+1.73 / −1.08) |
| DoF | 246 |
| p-value | 0.228 |
| Inter-instrument norm. | 1.07 (0.86–1.27) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 17.000 (approximate flux variability amplitude) |
|---|
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.