5XMM J020711.1+020727
| SRCID | 3005214030100023 |
|---|---|
| IAUNAME | 5XMM J020711.1+020727 |
| SC_RA | 02h07m11.13s (31.79637°) |
| SC_DEC | +02d07m27.1s (2.12421°) |
| RADEC_ERR | 0.45 arcsec |
| LII / BII | 157.8830° / -55.5215° |
| 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): 1.67e-14 ± 4.7e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.517
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
- 734828
- Match probability
- 0.996
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 21.490 | 0.196 |
| UVW1 | 21.399 | 0.111 |
| U | 21.104 | 0.105 |
| B | — | — |
| V | — | — |
- Name
- J020711.11+020727.3
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.278 | 0.062 |
| W2 | 16.015 | 0.169 |
| W3 | 12.225 | — |
| W4 | 8.994 | — |
- Class
- Galaxy
| Photometric (TPZ) | 0.2259 (conf 0.49) |
|---|---|
| Photometric (Le Phare) | 0.3782 (conf 0.93) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 7.89e-15 (+9.7e-15 / −6.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.75e+19 (+2.9e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.31 (+2.54 / −2.09) |
| DoF | 187 |
| p-value | 0.282 |
| Inter-instrument norm. | 1.71 (1.44–1.90) |
| 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.