5XMM J020735.6+021219
| SRCID | 3005214030100009 |
|---|---|
| IAUNAME | 5XMM J020735.6+021219 |
| SC_RA | 02h07m35.64s (31.89852°) |
| SC_DEC | +02d12m19.3s (2.20537°) |
| RADEC_ERR | 0.30 arcsec |
| LII / BII | 157.9646° / -55.3996° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52284.757 (2002-01-10 18:09:23.000 UTC) |
| MJD_LAST | 56877.491 (2014-08-08 11:46:56.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.59e-14 ± 3.6e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.88
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
- 736922
- Match probability
- 0.991
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.236 | 0.200 |
| B | — | — |
| V | — | — |
- Name
- J020735.56+021218.8
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.912 | 0.101 |
| W2 | 16.615 | 0.312 |
| W3 | 11.943 | — |
| W4 | 8.616 | — |
- Class
- Galaxy
| Photometric (TPZ) | 0.5758 (conf 0.70) |
|---|---|
| Photometric (Le Phare) | 0.6467 (conf 0.91) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.31e-14 (+2.6e-14 / −2.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.33e+20 (+4.5e+20 / −2.5e+19) cm−2 |
| Photon index (Γ) | 1.97 (+2.13 / −1.86) |
| DoF | 475 |
| p-value | 0.792 |
| Inter-instrument norm. | 0.96 (0.86–1.09) |
| 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.