5XMM J020720.3+020914
| SRCID | 3005214030100029 |
|---|---|
| IAUNAME | 5XMM J020720.3+020914 |
| SC_RA | 02h07m20.32s (31.83466°) |
| SC_DEC | +02d09m14.1s (2.15392°) |
| RADEC_ERR | 0.50 arcsec |
| LII / BII | 157.9143° / -55.4764° |
| 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): 1.79e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.566
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
- 735621
- Match probability
- 0.983
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.555 | 0.272 |
| B | — | — |
| V | — | — |
- Name
- J020720.24+020915.1
- Match probability
- 0.996
| Band | Mag | Err |
|---|---|---|
| W1 | 16.300 | 0.062 |
| W2 | 15.561 | 0.110 |
| W3 | 12.661 | 0.475 |
| W4 | 8.874 | — |
- Class
- QSO
| Photometric (TPZ) | 0.9257 (conf 0.25) |
|---|---|
| Photometric (Le Phare) | 1.2110 (conf 0.46) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 1.37e-14 (+1.6e-14 / −1.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.43e+19 (+1.9e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 1.84 (+1.99 / −1.71) |
| DoF | 208 |
| p-value | 0.931 |
| Inter-instrument norm. | 1.07 (0.87–1.32) |
| 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.