5XMM J020717.8+021303
| SRCID | 3005214030100027 |
|---|---|
| IAUNAME | 5XMM J020717.8+021303 |
| SC_RA | 02h07m17.89s (31.82455°) |
| SC_DEC | +02d13m03.9s (2.21774°) |
| RADEC_ERR | 0.49 arcsec |
| LII / BII | 157.8416° / -55.4267° |
| 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): 2.99e-14 ± 5.5e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.544
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
- 735397
- Match probability
- 0.996
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.137 | 0.222 |
| U | 21.855 | 0.143 |
| B | — | — |
| V | — | — |
- Name
- J020717.78+021303.5
- Match probability
- 0.996
| Band | Mag | Err |
|---|---|---|
| W1 | 15.842 | 0.047 |
| W2 | 15.443 | 0.099 |
| W3 | 12.505 | 0.400 |
| W4 | 9.170 | — |
- Class
- QSO
| Photometric (TPZ) | 0.1260 (conf 0.52) |
|---|---|
| Photometric (Le Phare) | 0.5545 (conf 0.94) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.44e-14 (+2.8e-14 / −2.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.61e+20 (+5.6e+20 / −2.6e+19) cm−2 |
| Photon index (Γ) | 1.52 (+1.69 / −1.39) |
| DoF | 275 |
| p-value | 0.858 |
| Inter-instrument norm. | 1.00 (0.84–1.18) |
| 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.