5XMM J044759.6-063122
| SRCID | 3001474060100011 |
|---|---|
| IAUNAME | 5XMM J044759.6-063122 |
| SC_RA | 04h47m59.67s (71.99864°) |
| SC_DEC | -06d31m22.6s (-6.52295°) |
| RADEC_ERR | 0.35 arcsec |
| LII / BII | 204.1810° / -30.3558° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52525.021 (2002-09-08 00:30:04.000 UTC) |
| MJD_LAST | 53975.011 (2006-08-28 00:16:07.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.81e-14 ± 4.4e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.329
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
- 1097728
- Match probability
- 0.994
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.589 | 0.149 |
| U | 22.364 | 0.310 |
| B | — | — |
| V | — | — |
- Name
- J044759.66-063122.2
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.147 | 0.055 |
| W2 | 15.464 | 0.098 |
| W3 | 11.732 | — |
| W4 | 8.667 | — |
- Class
- QSO
| Photometric (TPZ) | 1.2756 (conf 0.39) |
|---|---|
| Photometric (Le Phare) | 1.2650 (conf 0.57) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.81e-14 (+3.3e-14 / −2.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.24e+20 (+7.0e+20 / −3.1e+19) cm−2 |
| Photon index (Γ) | 1.48 (+1.68 / −1.35) |
| DoF | 648 |
| p-value | 0.979 |
| Inter-instrument norm. | 0.83 (0.71–0.97) |
| 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.