5XMM J022214.6-043132
| SRCID | 3003798210103719 |
|---|---|
| IAUNAME | 5XMM J022214.6-043132 |
| SC_RA | 02h22m14.63s (35.56096°) |
| SC_DEC | -04d31m32.5s (-4.52569°) |
| RADEC_ERR | 0.77 arcsec |
| LII / BII | 170.7097° / -58.7000° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52305.549 (2002-01-31 13:11:01.000 UTC) |
| MJD_LAST | 57756.635 (2017-01-03 15:14:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.76e-15 ± 2.6e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.579
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
- 793163
- Match probability
- 0.926
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.432 | 0.301 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J022214.63-043132.5
- Match probability
- 0.994
| Band | Mag | Err |
|---|---|---|
| W1 | 17.235 | 0.113 |
| W2 | 16.176 | 0.183 |
| W3 | 12.438 | — |
| W4 | 8.960 | — |
- Class
- QSO
| Spectroscopic (zsp) | 1.81700 |
|---|---|
| Photometric (TPZ) | 0.0010 (conf 0.10) |
| Photometric (Le Phare) | 0.8678 (conf 0.75) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 8.64e-15 (+1.2e-14 / −6.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.28e+20 (+6.7e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.24 (+2.66 / −1.94) |
| DoF | 50 |
| p-value | 0.821 |
| 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.