5XMM J133806.4+481756
| SRCID | 3005599050100196 |
|---|---|
| IAUNAME | 5XMM J133806.4+481756 |
| SC_RA | 13h38m06.44s (204.52682°) |
| SC_DEC | +48d17m56.9s (48.29915°) |
| RADEC_ERR | 1.35 arcsec |
| LII / BII | 102.8216° / 66.9662° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52409.392 (2002-05-15 09:23:59.000 UTC) |
| MJD_LAST | 59025.341 (2020-06-25 08:10:27.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.48e-14 ± 3.3e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.00179
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
- 3523329
- Match probability
- 0.974
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.441 | 0.197 |
| B | — | — |
| V | — | — |
- Name
- J133806.52+481757.7
- Match probability
- 0.994
| Band | Mag | Err |
|---|---|---|
| W1 | 15.902 | 0.046 |
| W2 | 15.214 | 0.074 |
| W3 | 12.367 | — |
| W4 | 9.419 | — |
- Class
- QSO
| Spectroscopic (zsp) | 0.18800 |
|---|---|
| Photometric (TPZ) | 0.1760 (conf 0.52) |
| Photometric (Le Phare) | 0.2592 (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 | 1.55e-14 (+2.1e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.14e+23 (+3.0e+23 / −3.2e+22) cm−2 |
| Photon index (Γ) | 1.58 (+2.39 / −1.13) |
| DoF | 368 |
| p-value | 0.587 |
| 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.