5XMM J150610.3+013005
| SRCID | 3002154010100028 |
|---|---|
| IAUNAME | 5XMM J150610.3+013005 |
| SC_RA | 15h06m10.35s (226.54313°) |
| SC_DEC | +01d30m05.6s (1.50155°) |
| RADEC_ERR | 0.43 arcsec |
| LII / BII | 0.2283° / 48.7869° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 51934.595 (2001-01-25 14:16:08.000 UTC) |
| MJD_LAST | 56679.394 (2014-01-22 09:26:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.19e-14 ± 2.4e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.51
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
- 3850470
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.837 | 0.165 |
| U | 22.052 | 0.211 |
| B | 21.563 | 0.196 |
| V | 20.504 | 0.204 |
- Name
- J150610.40+013005.2
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 17.136 | 0.130 |
| W2 | 16.151 | 0.219 |
| W3 | 12.322 | — |
| W4 | 9.223 | — |
- Class
- QSO
| Photometric (TPZ) | 0.0010 (conf 0.14) |
|---|---|
| Photometric (Le Phare) | 0.4011 (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 | 1.31e-14 (+1.5e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.78e+19 (+1.7e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 2.89 (+2.97 / −2.75) |
| DoF | 84 |
| p-value | 0.849 |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 14.100 (approximate flux variability amplitude) |
|---|
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.