5XMM J022205.5-034923
| SRCID | 3003798010105674 |
|---|---|
| IAUNAME | 5XMM J022205.5-034923 |
| SC_RA | 02h22m05.55s (35.52313°) |
| SC_DEC | -03d49m23.0s (-3.82306°) |
| RADEC_ERR | 0.98 arcsec |
| LII / BII | 169.7745° / -58.1944° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52285.186 (2002-01-11 04:27:23.000 UTC) |
| MJD_LAST | 55054.626 (2009-08-11 15:02:02.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.14e-14 ± 3.1e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.061
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
- 792034
- Match probability
- 0.958
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.911 | 0.122 |
| U | 21.593 | 0.120 |
| B | — | — |
| V | — | — |
- Name
- J022205.58-034925.0
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 15.505 | 0.041 |
| W2 | 14.721 | 0.058 |
| W3 | 11.793 | 0.224 |
| W4 | 8.660 | — |
- Class
- QSO
| Spectroscopic (zsp) | 0.37200 |
|---|---|
| Photometric (TPZ) | 0.2759 (conf 0.66) |
| Photometric (Le Phare) | 0.2650 (conf 0.96) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 6.66e-15 (+9.9e-15 / −4.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.35e+20 (+2.9e+21 / −3.5e+19) cm−2 |
| Photon index (Γ) | 1.52 (+2.18 / −1.17) |
| DoF | 355 |
| p-value | 0.341 |
| 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.