5XMM J140610.1+221619
| SRCID | 3005176020100030 |
|---|---|
| IAUNAME | 5XMM J140610.1+221619 |
| SC_RA | 14h06m10.12s (211.54218°) |
| SC_DEC | +22d16m19.4s (22.27206°) |
| RADEC_ERR | 0.67 arcsec |
| LII / BII | 21.0406° / 72.3663° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52078.071 (2001-06-18 01:41:59.000 UTC) |
| MJD_LAST | 57413.657 (2016-01-26 15:46:24.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.28e-14 ± 1.0e-14 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.86
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
- 3611493
- Match probability
- 0.851
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 23.136 | 0.260 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J140610.11+221621.9
- Match probability
- 0.994
| Band | Mag | Err |
|---|---|---|
| W1 | 15.318 | 0.035 |
| W2 | 14.867 | 0.057 |
| W3 | 12.409 | 0.338 |
| W4 | 8.876 | — |
- Class
- Galaxy
| Photometric (TPZ) | 0.7758 (conf 0.60) |
|---|---|
| Photometric (Le Phare) | 1.4150 (conf 0.98) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 5.27e-14 (+6.3e-14 / −4.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.74e+19 (+2.0e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 1.50 (+1.66 / −1.38) |
| DoF | 580 |
| p-value | 0.039 |
| Inter-instrument norm. | 1.00 (0.85–1.18) |
| 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.