5XMM J022250.6-041050
| SRCID | 3003798220100748 |
|---|---|
| IAUNAME | 5XMM J022250.6-041050 |
| SC_RA | 02h22m50.67s (35.71113°) |
| SC_DEC | -04d10m50.1s (-4.18059°) |
| RADEC_ERR | 0.43 arcsec |
| LII / BII | 170.4891° / -58.3419° |
| N_CONTRIB | 5 (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): 2.92e-14 ± 3.9e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.109
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
- 798123
- Match probability
- 0.955
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.755 | 0.120 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J022250.59-041051.3
- Match probability
- 0.993
| Band | Mag | Err |
|---|---|---|
| W1 | 17.017 | 0.101 |
| W2 | 16.894 | 0.334 |
| W3 | 12.862 | — |
| W4 | 8.602 | — |
- Class
- Star
| Spectroscopic (zsp) | 0.94800 |
|---|---|
| Photometric (TPZ) | 0.8758 (conf 0.48) |
| Photometric (Le Phare) | 2.3480 (conf 0.58) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.06e-14 (+2.4e-14 / −1.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.17e+20 (+4.5e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 2.08 (+2.29 / −1.91) |
| DoF | 651 |
| p-value | 0.96 |
| Inter-instrument norm. | 1.51 (1.27–1.73) |
| 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.