5XMM J020713.5+020244
| SRCID | 3005214030100067 |
|---|---|
| IAUNAME | 5XMM J020713.5+020244 |
| SC_RA | 02h07m13.51s (31.80628°) |
| SC_DEC | +02d02m44.7s (2.04575°) |
| RADEC_ERR | 1.12 arcsec |
| LII / BII | 157.9689° / -55.5839° |
| 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): 3.85e-15 ± 2.5e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.16
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
- 735025
- Match probability
- 0.977
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.388 | 0.179 |
| U | 20.998 | 0.125 |
| B | — | — |
| V | — | — |
- Name
- J020713.41+020245.4
- Match probability
- 0.994
| Band | Mag | Err |
|---|---|---|
| W1 | 14.386 | 0.028 |
| W2 | 13.332 | 0.030 |
| W3 | 10.417 | 0.060 |
| W4 | 8.323 | 0.202 |
- Class
- QSO
| Photometric (TPZ) | 0.2259 (conf 0.21) |
|---|---|
| Photometric (Le Phare) | 0.2542 (conf 1.00) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 4.30e-15 (+5.5e-15 / −3.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.08e+20 (+3.9e+20 / −2.0e+19) cm−2 |
| Photon index (Γ) | 2.65 (+2.88 / −2.35) |
| DoF | 144 |
| p-value | 0.91 |
| Inter-instrument norm. | 0.69 (0.56–0.96) |
| 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.