5XMM J120109.6-033709
| SRCID | 3005602070100009 |
|---|---|
| IAUNAME | 5XMM J120109.6-033709 |
| SC_RA | 12h01m09.62s (180.29010°) |
| SC_DEC | -03d37m09.2s (-3.61923°) |
| RADEC_ERR | 0.34 arcsec |
| LII / BII | 279.4676° / 56.9444° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 52254.813 (2001-12-11 19:30:15.000 UTC) |
| MJD_LAST | 58487.542 (2019-01-04 13:00:41.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.82e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.587
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
- 3127307
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.763 | 0.141 |
| U | 22.145 | 0.272 |
| B | — | — |
| V | — | — |
- Name
- J120109.56-033707.4
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.645 | 0.095 |
| W2 | 15.916 | 0.173 |
| W3 | 11.720 | — |
| W4 | 8.824 | — |
- Class
- QSO
| Photometric (TPZ) | 2.2254 (conf 0.24) |
|---|---|
| Photometric (Le Phare) | 2.3880 (conf 0.80) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 4.11e-14 (+4.7e-14 / −3.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.56e+19 (+1.2e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 1.89 (+2.02 / −1.76) |
| DoF | 312 |
| p-value | 0.644 |
| Inter-instrument norm. | 0.73 (0.61–0.86) |
| 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.