5XMM J022152.9-040546
| SRCID | 3003798220101126 |
|---|---|
| IAUNAME | 5XMM J022152.9-040546 |
| SC_RA | 02h21m52.97s (35.47072°) |
| SC_DEC | -04d05m46.5s (-4.09626°) |
| RADEC_ERR | 0.38 arcsec |
| LII / BII | 170.0383° / -58.4356° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52667.803 (2003-01-28 19:16:33.000 UTC) |
| MJD_LAST | 57758.217 (2017-01-05 05:11:54.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.60e-14 ± 3.2e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.497
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
- 790649
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.872 | 0.086 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J022152.93-040546.6
- Match probability
- 0.994
| Band | Mag | Err |
|---|---|---|
| W1 | 15.816 | 0.045 |
| W2 | 15.521 | 0.099 |
| W3 | 12.250 | — |
| W4 | 9.441 | — |
- Class
- Galaxy
| Spectroscopic (zsp) | 0.43100 |
|---|---|
| Photometric (TPZ) | 0.4259 (conf 0.74) |
| Photometric (Le Phare) | 0.4886 (conf 0.96) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.03e-14 (+2.4e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.61e+20 (+6.6e+20 / −2.6e+19) cm−2 |
| Photon index (Γ) | 1.91 (+2.20 / −1.71) |
| DoF | 116 |
| p-value | 0.706 |
| 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.