5XMM J004319.2-204106
| SRCID | 3004234020100010 |
|---|---|
| IAUNAME | 5XMM J004319.2-204106 |
| SC_RA | 00h43m19.29s (10.83039°) |
| SC_DEC | -20d41m06.8s (-20.68521°) |
| RADEC_ERR | 0.43 arcsec |
| LII / BII | 106.4489° / -83.2957° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52278.767 (2002-01-04 18:23:55.000 UTC) |
| MJD_LAST | 58644.428 (2019-06-10 10:16:11.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.88e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.537
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
- 149467
- Match probability
- 0.98
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 20.759 | 0.182 |
| UVM2 | 21.006 | 0.193 |
| UVW1 | 20.808 | 0.085 |
| U | — | — |
| B | — | — |
| V | — | — |
- Source ID
- 2350654395878234624
- Match probability
- 0.99
- Magnitudes
- G=20.77, BP=20.61, RP=20.56
- Class
- QSO
| Spectroscopic (zsp) | 0.91500 |
|---|---|
| Photometric (TPZ) | 2.4253 (conf 0.49) |
| Photometric (Le Phare) | 0.7465 (conf 0.37) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 3.07e-14 (+3.7e-14 / −2.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.53e+20 (+6.1e+20 / −2.7e+19) cm−2 |
| Photon index (Γ) | 2.18 (+2.43 / −1.98) |
| DoF | 329 |
| p-value | 0.819 |
| Inter-instrument norm. | 0.88 (0.72–1.06) |
| 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.