5XMM J053904.6-694052
5XMM-DR15 stacked source · SRCID 3002394040100571
Position:
05h39m04.68s -69d40m52.8s
(84.76949°, -69.68133°)
EP flux
1.99e-14
± 4.9e-15
erg cm-2 s-1
CLASSX
AGN
(0.903)
Detections
4
| SRCID | 3002394040100571 |
|---|---|
| IAUNAME | 5XMM J053904.6-694052 |
| SC_RA | 05h39m04.68s (84.76949°) |
| SC_DEC | -69d40m52.8s (-69.68133°) |
| RADEC_ERR | 1.19 arcsec |
| LII / BII | 280.1377° / -31.5721° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 336 (observations covering the position) |
| MJD_FIRST | 51838.662 (2000-10-21 15:53:07.000 UTC) |
| MJD_LAST | 56971.170 (2014-11-10 04:05:09.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.99e-14 ± 4.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.74
± 0.47
0.2-0.5 / 0.5-1.0 keV
HR2
0.78
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31
± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.67
± 0.19
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.4)
SUM_FLAG:
3
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.39
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.
Optical Monitor (OM)
- OM Source ID
- 2017884
- Match probability
- 0.756
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.197 | 0.173 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.66e-14 (+9.4e-14 / −7.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.06e+22 (+1.2e+22 / −8.9e+21) cm−2 |
| Photon index (Γ) | 2.78 (+2.93 / −2.54) |
| DoF | 318 |
| p-value | 0.871 |
| Quality flag | 0 |
No variability data available for this source.
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.