5XMM J181906.7-121016
5XMM-DR15 stacked source · SRCID 3000882030100016
Position:
18h19m06.76s -12d10m16.3s
(274.77815°, -12.17120°)
EP flux
5.13e-14
± 7.7e-15
erg cm-2 s-1
CLASSX
AGN
(0.902)
Detections
6
| SRCID | 3000882030100016 |
|---|---|
| IAUNAME | 5XMM J181906.7-121016 |
| SC_RA | 18h19m06.76s (274.77815°) |
| SC_DEC | -12d10m16.3s (-12.17120°) |
| RADEC_ERR | 0.44 arcsec |
| LII / BII | 18.4316° / 1.4993° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 7 (observations covering the position) |
| MJD_FIRST | 52371.983 (2002-04-07 23:35:06.000 UTC) |
| MJD_LAST | 60042.022 (2023-04-08 00:31:05.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.13e-14 ± 7.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.20
± 0.83
0.2-0.5 / 0.5-1.0 keV
HR2
0.93
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.10
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
0.38
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 2.87
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 | 9.89e-14 (+1.1e-13 / −8.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.90e+21 (+9.0e+21 / −3.9e+21) cm−2 |
| Photon index (Γ) | 1.19 (+1.44 / −1.06) |
| DoF | 138 |
| p-value | 0.475 |
| Inter-instrument norm. | 1.58 (1.29–1.83) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 15.200 (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.