5XMM J125223.2-292518
5XMM-DR15 stacked source · SRCID 3005774030100106
Position:
12h52m23.22s -29d25m18.5s
(193.09675°, -29.42181°)
EP flux
9.24e-15
± 2.3e-15
erg cm-2 s-1
CLASSX
AGN
(0.913)
Detections
4
| SRCID | 3005774030100106 |
|---|---|
| IAUNAME | 5XMM J125223.2-292518 |
| SC_RA | 12h52m23.22s (193.09675°) |
| SC_DEC | -29d25m18.5s (-29.42181°) |
| RADEC_ERR | 0.53 arcsec |
| LII / BII | 303.1796° / 33.4495° |
| 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): 9.24e-15 ± 2.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.76
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.29
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.56
± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.19
± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.625
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
- 3316967
- Match probability
- 0.987
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.823 | 0.261 |
| U | 21.515 | 0.178 |
| B | 21.131 | 0.277 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.51e-15 (+1.0e-14 / −4.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 7.37e+19 (+4.4e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 1.81 (+2.31 / −1.42) |
| DoF | 58 |
| p-value | 0.582 |
| 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.