5XMM J230510.3+122239
| SRCID | 3002554100100016 |
|---|---|
| IAUNAME | 5XMM J230510.3+122239 |
| SC_RA | 23h05m10.33s (346.29305°) |
| SC_DEC | +12d22m39.4s (12.37760°) |
| RADEC_ERR | 0.30 arcsec |
| LII / BII | 86.3751° / -42.8261° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52079.650 (2001-06-19 15:36:24.000 UTC) |
| MJD_LAST | 58269.479 (2018-05-31 11:29:14.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.25e-14 ± 2.7e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.269
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
- 6526797
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.580 | 0.318 |
| B | — | — |
| V | — | — |
- Name
- J230510.39+122238.9
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.588 | 0.088 |
| W2 | 15.715 | 0.140 |
| W3 | 12.196 | — |
| W4 | 8.955 | — |
- Class
- QSO
| Photometric (TPZ) | 1.3256 (conf 0.71) |
|---|---|
| Photometric (Le Phare) | 3.0130 (conf 0.22) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 3.34e-14 (+3.6e-14 / −3.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.02e+20 (+3.5e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.61 (+1.72 / −1.53) |
| DoF | 651 |
| p-value | 0.839 |
| Inter-instrument norm. | 0.77 (0.68–0.85) |
| 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.