5XMM J022237.9-041140
| SRCID | 3003798220102071 |
|---|---|
| IAUNAME | 5XMM J022237.9-041140 |
| SC_RA | 02h22m37.93s (35.65803°) |
| SC_DEC | -04d11m40.0s (-4.19445°) |
| RADEC_ERR | 0.52 arcsec |
| LII / BII | 170.4305° / -58.3872° |
| N_CONTRIB | 7 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52303.370 (2002-01-29 08:52:41.000 UTC) |
| MJD_LAST | 57758.217 (2017-01-05 05:11:54.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.68e-14 ± 3.2e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.403
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
- 796385
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.462 | 0.059 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J022237.87-041139.3
- Match probability
- 0.993
| Band | Mag | Err |
|---|---|---|
| W1 | 17.844 | 0.202 |
| W2 | 16.896 | 0.319 |
| W3 | 12.863 | — |
| W4 | 9.171 | — |
- Class
- QSO
| Spectroscopic (zsp) | 1.49600 |
|---|---|
| Photometric (TPZ) | 1.2756 (conf 0.77) |
| Photometric (Le Phare) | 1.4290 (conf 0.43) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 1.32e-14 (+1.7e-14 / −9.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.93e+19 (+2.5e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 1.89 (+2.22 / −1.62) |
| DoF | 72 |
| p-value | 0.751 |
| 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.