5XMM J133728.9+482028
| SRCID | 3005599050100185 |
|---|---|
| IAUNAME | 5XMM J133728.9+482028 |
| SC_RA | 13h37m28.90s (204.37042°) |
| SC_DEC | +48d20m28.2s (48.34117°) |
| RADEC_ERR | 0.62 arcsec |
| LII / BII | 103.1072° / 66.9764° |
| 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): 6.05e-15 ± 1.2e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.48
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
- 3521320
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.295 | 0.180 |
| U | 21.816 | 0.113 |
| B | — | — |
| V | — | — |
- Name
- J133728.94+482028.2
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 17.207 | 0.109 |
| W2 | 16.360 | 0.181 |
| W3 | 12.206 | — |
| W4 | 9.102 | — |
- Class
- QSO
| Spectroscopic (zsp) | 2.05200 |
|---|---|
| Photometric (TPZ) | 2.0254 (conf 0.59) |
| Photometric (Le Phare) | 1.9450 (conf 0.73) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 7.75e-15 (+9.2e-15 / −6.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 3.62e+19 (+1.2e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 1.90 (+2.06 / −1.78) |
| DoF | 530 |
| p-value | 0.772 |
| Inter-instrument norm. | 1.03 (0.88–1.22) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.400 (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.