5XMM J125238.6-293101
5XMM-DR15 stacked source · SRCID 3005774030100142
Position:
12h52m38.69s -29d31m01.4s
(193.16120°, -29.51706°)
EP flux
2.68e-15
± 9.7e-16
erg cm-2 s-1
CLASSX
Star
(1)
Detections
2
| SRCID | 3005774030100142 |
|---|---|
| IAUNAME | 5XMM J125238.6-293101 |
| SC_RA | 12h52m38.69s (193.16120°) |
| SC_DEC | -29d31m01.4s (-29.51706°) |
| RADEC_ERR | 0.68 arcsec |
| LII / BII | 303.2462° / 33.3539° |
| 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): 2.68e-15 ± 9.7e-16 erg cm-2 s-1
Hardness ratios
HR1
0.55
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.68
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.77
± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
-0.30
± 1.27
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.15
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
- 3317797
- Match probability
- 0.983
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 13.988 | 0.004 |
| UVM2 | 13.731 | 0.004 |
| UVW1 | 12.510 | 0.002 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.17e-15 (+5.4e-15 / −3.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 5.68e+20 (+1.4e+21 / −4.6e+19) cm−2 |
| Photon index (Γ) | 2.38 (+2.79 / −1.98) |
| DoF | 97 |
| p-value | 0.096 |
| 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.