5XMM J133137.5+111410
| SRCID | 3006194010100016 |
|---|---|
| IAUNAME | 5XMM J133137.5+111410 |
| SC_RA | 13h31m37.56s (202.90648°) |
| SC_DEC | +11d14m10.2s (11.23616°) |
| RADEC_ERR | 0.46 arcsec |
| LII / BII | 335.5896° / 71.5125° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 51912.417 (2001-01-03 10:00:44.000 UTC) |
| MJD_LAST | 55390.662 (2010-07-13 15:52:57.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.71e-14 ± 6.3e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.571
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
- 3501680
- Match probability
- 0.916
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.213 | 0.160 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J133137.46+111410.8
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.816 | 0.091 |
| W2 | 16.252 | 0.208 |
| W3 | 12.279 | — |
| W4 | 9.166 | — |
- Class
- Galaxy
| Photometric (TPZ) | 0.7258 (conf 0.15) |
|---|---|
| Photometric (Le Phare) | 0.7479 (conf 0.56) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.55e-14 (+3.0e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.43e+19 (+2.8e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 1.95 (+2.10 / −1.82) |
| DoF | 229 |
| p-value | 0.972 |
| Inter-instrument norm. | 1.33 (1.11–1.55) |
| 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.