5XMM J124846.7-054852
5XMM-DR15 stacked source · SRCID 3006037020100010
Position:
12h48m46.76s -05d48m52.7s
(192.19485°, -5.81463°)
EP flux
7.08e-14
± 4.1e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.627)
Detections
3
| SRCID | 3006037020100010 |
|---|---|
| IAUNAME | 5XMM J124846.7-054852 |
| SC_RA | 12h48m46.76s (192.19485°) |
| SC_DEC | -05d48m52.7s (-5.81463°) |
| RADEC_ERR | 0.20 arcsec |
| LII / BII | 301.7162° / 57.0508° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 12 (observations covering the position) |
| MJD_FIRST | 52101.640 (2001-07-11 15:22:08.000 UTC) |
| MJD_LAST | 53201.820 (2004-07-15 19:41:14.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.08e-14 ± 4.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.14
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.15
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.14
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.49
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 1.98
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
- 3301072
- Match probability
- 0.979
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 18.785 | 0.083 |
| UVM2 | 18.905 | 0.067 |
| UVW1 | 19.000 | 0.062 |
| U | — | — |
| B | 18.797 | 0.073 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.11e-14 (+7.8e-14 / −6.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.90e+19 (+1.4e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 1.84 (+1.96 / −1.73) |
| DoF | 314 |
| p-value | 0.428 |
| 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.