5XMM J004206.1-091152
| SRCID | 3006514010100040 |
|---|---|
| IAUNAME | 5XMM J004206.1-091152 |
| SC_RA | 00h42m06.18s (10.52577°) |
| SC_DEC | -09d11m52.2s (-9.19783°) |
| RADEC_ERR | 0.30 arcsec |
| LII / BII | 115.4842° / -71.9345° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52281.557 (2002-01-07 13:21:35.000 UTC) |
| MJD_LAST | 56831.338 (2014-06-23 08:06:18.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.11e-14 ± 2.4e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.705
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
- 126802
- Match probability
- 0.974
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 20.995 | 0.186 |
| UVW1 | 21.848 | 0.121 |
| U | 21.847 | 0.122 |
| B | 21.266 | 0.127 |
| V | 20.400 | 0.140 |
- Name
- J004206.29-091154.2
- Match probability
- 0.996
| Band | Mag | Err |
|---|---|---|
| W1 | 15.693 | 0.049 |
| W2 | 15.245 | 0.094 |
| W3 | 12.026 | 0.411 |
| W4 | 8.655 | 0.360 |
- Class
- QSO
| Photometric (TPZ) | 0.3759 (conf 0.77) |
|---|---|
| Photometric (Le Phare) | 0.3770 (conf 0.72) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 2.85e-14 (+3.4e-14 / −2.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.05e+19 (+1.5e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 1.88 (+2.01 / −1.78) |
| DoF | 359 |
| p-value | 0.972 |
| Inter-instrument norm. | 1.41 (1.21–1.65) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.000 (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.