5XMM J124642.0+021306
| SRCID | 3005176010100058 |
|---|---|
| IAUNAME | 5XMM J124642.0+021306 |
| SC_RA | 12h46m42.07s (191.67529°) |
| SC_DEC | +02d13m06.5s (2.21848°) |
| RADEC_ERR | 0.64 arcsec |
| LII / BII | 300.1243° / 65.0644° |
| N_CONTRIB | 7 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52077.875 (2001-06-17 20:59:59.000 UTC) |
| MJD_LAST | 57038.758 (2015-01-16 18:11:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.46e-15 ± 3.0e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.524
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.
- OM Source ID
- 3284419
- Match probability
- 0.866
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.829 | 0.334 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J124642.05+021307.0
- Match probability
- 0.994
| Band | Mag | Err |
|---|---|---|
| W1 | 16.701 | 0.094 |
| W2 | 16.553 | 0.282 |
| W3 | 12.308 | — |
| W4 | 8.652 | — |
- Class
- Star
| Photometric (TPZ) | 0.7758 (conf 0.37) |
|---|---|
| Photometric (Le Phare) | 1.1050 (conf 0.38) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 9.42e-15 (+1.2e-14 / −7.6e-15) erg cm−2 s−1 |
|---|---|
| NH | 7.27e+19 (+2.9e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 2.53 (+2.82 / −2.23) |
| DoF | 111 |
| p-value | 0.189 |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.900 (approximate flux variability amplitude) |
|---|
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.