5XMM J125245.3-291553
5XMM-DR15 stacked source · SRCID 3005774030100177
Position:
12h52m45.37s -29d15m53.0s
(193.18904°, -29.26472°)
EP flux
2.20e-15
± 2.4e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.732)
Detections
4
| SRCID | 3005774030100177 |
|---|---|
| IAUNAME | 5XMM J125245.3-291553 |
| SC_RA | 12h52m45.37s (193.18904°) |
| SC_DEC | -29d15m53.0s (-29.26472°) |
| RADEC_ERR | 1.58 arcsec |
| LII / BII | 303.2771° / 33.6061° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 14 (observations covering the position) |
| MJD_FIRST | 51726.363 (2000-07-01 08:42:20.000 UTC) |
| MJD_LAST | 52650.824 (2003-01-11 19:46:07.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.20e-15 ± 2.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.70
± 0.26
0.2-0.5 / 0.5-1.0 keV
HR2
-0.28
± 0.28
0.5-1.0 / 1.0-2.0 keV
HR3
-0.19
± 0.40
1.0-2.0 / 2.0-4.5 keV
HR4
0.31
± 0.46
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 3.2)
SUM_FLAG:
3
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.27
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
- 3318118
- Match probability
- 0.715
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.177 | 0.074 |
| U | — | — |
| B | — | — |
| V | 17.961 | 0.063 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.97e-14 (+2.6e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.77e+20 (+1.7e+21 / −3.5e+19) cm−2 |
| Photon index (Γ) | 2.13 (+2.59 / −1.80) |
| DoF | 74 |
| p-value | 0.869 |
| 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.