5XMM J022034.3-041503
| SRCID | 3003798240100790 |
|---|---|
| IAUNAME | 5XMM J022034.3-041503 |
| SC_RA | 02h20m34.36s (35.14318°) |
| SC_DEC | -04d15m03.0s (-4.25084°) |
| RADEC_ERR | 0.46 arcsec |
| LII / BII | 169.7565° / -58.7658° |
| N_CONTRIB | 6 (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): 3.33e-14 ± 4.3e-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
- 781977
- Match probability
- 0.966
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.528 | 0.080 |
| U | — | — |
| B | — | — |
| V | — | — |
- Source ID
- 2489821167448533632
- Match probability
- 0.993
- Magnitudes
- G=20.78, BP=20.73, RP=20.18
- Class
- QSO
| Spectroscopic (zsp) | 1.88500 |
|---|---|
| Photometric (TPZ) | 1.8255 (conf 0.89) |
| Photometric (Le Phare) | 1.8330 (conf 0.61) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.24e-14 (+2.8e-14 / −1.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.89e+19 (+4.0e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.04 (+2.31 / −1.79) |
| DoF | 114 |
| p-value | 0.797 |
| 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.