5XMM J022000.1-041744
| SRCID | 3003798230100984 |
|---|---|
| IAUNAME | 5XMM J022000.1-041744 |
| SC_RA | 02h20m00.11s (35.00044°) |
| SC_DEC | -04d17m44.0s (-4.29556°) |
| RADEC_ERR | 0.38 arcsec |
| LII / BII | 169.6037° / -58.8923° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52664.245 (2003-01-25 05:52:27.000 UTC) |
| MJD_LAST | 57756.119 (2017-01-03 02:51:26.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.02e-14 ± 5.4e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.0209
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
- 778495
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 21.055 | 0.205 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J022000.13-041745.4
- Match probability
- 0.993
| Band | Mag | Err |
|---|---|---|
| W1 | 17.121 | 0.117 |
| W2 | 16.574 | 0.263 |
| W3 | 12.455 | — |
| W4 | 9.206 | — |
- Class
- QSO
| Spectroscopic (zsp) | 0.92000 |
|---|---|
| Photometric (TPZ) | 0.6758 (conf 0.70) |
| Photometric (Le Phare) | 2.0480 (conf 0.27) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 4.25e-14 (+5.3e-14 / −3.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.20e+19 (+2.9e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 1.43 (+1.63 / −1.26) |
| DoF | 98 |
| p-value | 0.808 |
| 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.