5XMM J020728.1+020329
| SRCID | 3005214030100017 |
|---|---|
| IAUNAME | 5XMM J020728.1+020329 |
| SC_RA | 02h07m28.17s (31.86738°) |
| SC_DEC | +02d03m29.7s (2.05824°) |
| RADEC_ERR | 0.37 arcsec |
| LII / BII | 158.0503° / -55.5419° |
| 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): 2.22e-14 ± 2.8e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.756
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
- 736336
- Match probability
- 0.986
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.841 | 0.175 |
| U | 21.695 | 0.117 |
| B | — | — |
| V | — | — |
- Name
- J020728.02+020328.9
- Match probability
- 0.996
| Band | Mag | Err |
|---|---|---|
| W1 | 16.912 | 0.098 |
| W2 | 15.538 | 0.102 |
| W3 | 12.665 | 0.475 |
| W4 | 8.591 | — |
- Class
- QSO
| Photometric (TPZ) | 0.1260 (conf 0.53) |
|---|---|
| Photometric (Le Phare) | 0.6178 (conf 0.89) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 3.62e-14 (+4.1e-14 / −3.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.60e+20 (+1.0e+21 / −7.0e+19) cm−2 |
| Photon index (Γ) | 1.44 (+1.68 / −1.28) |
| DoF | 545 |
| p-value | 0.539 |
| Inter-instrument norm. | 0.77 (0.65–0.89) |
| 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.