5XMM J004118.9-091659
| SRCID | 3006514010100136 |
|---|---|
| IAUNAME | 5XMM J004118.9-091659 |
| SC_RA | 00h41m18.92s (10.32882°) |
| SC_DEC | -09d16m59.1s (-9.28309°) |
| RADEC_ERR | 0.77 arcsec |
| LII / BII | 114.8274° / -71.9954° |
| 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): 1.36e-14 ± 3.4e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.236
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
- 117148
- Match probability
- 0.984
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.869 | 0.165 |
| B | — | — |
| V | — | — |
- Name
- J004118.93-091659.9
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 16.676 | 0.092 |
| W2 | 16.089 | 0.192 |
| W3 | 12.502 | — |
| W4 | 8.034 | — |
- Class
- QSO
| Photometric (TPZ) | 0.7758 (conf 0.71) |
|---|---|
| Photometric (Le Phare) | 0.3974 (conf 0.35) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 1.21e-14 (+1.8e-14 / −6.9e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.12e+19 (+3.2e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 1.72 (+2.14 / −1.36) |
| DoF | 236 |
| p-value | 0.837 |
| Inter-instrument norm. | 0.93 (0.66–1.42) |
| 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.