5XMM J022029.0-040727
| SRCID | 3003798240100939 |
|---|---|
| IAUNAME | 5XMM J022029.0-040727 |
| SC_RA | 02h20m29.01s (35.12086°) |
| SC_DEC | -04d07m27.6s (-4.12434°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 169.5656° / -58.6841° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52664.245 (2003-01-25 05:52:27.000 UTC) |
| MJD_LAST | 57754.394 (2017-01-01 09:27:25.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.81e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.495
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
- 781477
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.565 | 0.082 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J022029.04-040728.6
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.303 | 0.059 |
| W2 | 15.363 | 0.090 |
| W3 | 12.364 | — |
| W4 | 8.992 | — |
- Class
- QSO
| Spectroscopic (zsp) | 1.24300 |
|---|---|
| Photometric (TPZ) | 1.1757 (conf 0.84) |
| Photometric (Le Phare) | 1.2600 (conf 0.79) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 1.90e-14 (+2.2e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.64e+20 (+8.7e+20 / −2.6e+19) cm−2 |
| Photon index (Γ) | 2.14 (+2.46 / −1.93) |
| DoF | 112 |
| p-value | 0.35 |
| 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.