5XMM J133835.0+482118
| SRCID | 3005599050100026 |
|---|---|
| IAUNAME | 5XMM J133835.0+482118 |
| SC_RA | 13h38m35.04s (204.64600°) |
| SC_DEC | +48d21m18.8s (48.35523°) |
| RADEC_ERR | 0.32 arcsec |
| LII / BII | 102.7083° / 66.8799° |
| 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): 3.57e-14 ± 5.3e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.134
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
- 3524169
- Match probability
- 0.992
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.162 | 0.157 |
| B | — | — |
| V | — | — |
- Name
- J133835.06+482117.9
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 17.256 | 0.114 |
| W2 | 16.447 | 0.192 |
| W3 | 12.625 | — |
| W4 | 9.317 | — |
- Class
- QSO
| Photometric (TPZ) | 1.3256 (conf 0.77) |
|---|---|
| Photometric (Le Phare) | 0.4549 (conf 0.30) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.20e-14 (+2.6e-14 / −1.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.80e+19 (+4.1e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 2.01 (+2.20 / −1.85) |
| DoF | 554 |
| p-value | 0.812 |
| Inter-instrument norm. | 1.16 (1.01–1.33) |
| 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.