5XMM J125313.0-293444
5XMM-DR15 stacked source · SRCID 3005774030100064
Position:
12h53m13.04s -29d34m44.3s
(193.30432°, -29.57897°)
EP flux
2.80e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.85)
Detections
2
| SRCID | 3005774030100064 |
|---|---|
| IAUNAME | 5XMM J125313.0-293444 |
| SC_RA | 12h53m13.04s (193.30432°) |
| SC_DEC | -29d34m44.3s (-29.57897°) |
| RADEC_ERR | 0.45 arcsec |
| LII / BII | 303.3947° / 33.2912° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 14 (observations covering the position) |
| MJD_FIRST | 52642.080 (2003-01-03 01:54:58.000 UTC) |
| MJD_LAST | 52650.824 (2003-01-11 19:46:07.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.80e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.50
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.08
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.24
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
0.00
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.6)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.27
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
- 3319897
- Match probability
- 0.992
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.480 | 0.122 |
| U | 19.722 | 0.099 |
| B | 18.347 | 0.047 |
| V | 17.474 | 0.051 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.98e-14 (+2.3e-14 / −1.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.50e+20 (+7.1e+20 / −2.5e+19) cm−2 |
| Photon index (Γ) | 1.32 (+1.53 / −1.17) |
| DoF | 151 |
| p-value | 0.644 |
| 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.