5XMM J004148.8-091011
| SRCID | 3006514010100111 |
|---|---|
| IAUNAME | 5XMM J004148.8-091011 |
| SC_RA | 00h41m48.85s (10.45352°) |
| SC_DEC | -09d10m11.8s (-9.16995°) |
| RADEC_ERR | 0.56 arcsec |
| LII / BII | 115.2667° / -71.8983° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52281.557 (2002-01-07 13:21:35.000 UTC) |
| MJD_LAST | 57035.007 (2015-01-13 00:10:33.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.13e-14 ± 2.4e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.335
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
- 122824
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.824 | 0.234 |
| U | — | — |
| B | — | — |
| V | — | — |
- Name
- J004148.88-091012.9
- Match probability
- 0.99
| Band | Mag | Err |
|---|---|---|
| W1 | 16.968 | 0.117 |
| W2 | 16.950 | 0.470 |
| W3 | 12.461 | 0.454 |
| W4 | 9.105 | — |
- Class
- Star
| Photometric (TPZ) | 0.4259 (conf 0.34) |
|---|---|
| Photometric (Le Phare) | 0.8461 (conf 0.83) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 1.46e-14 (+1.6e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.37e+19 (+2.0e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 1.90 (+2.05 / −1.79) |
| DoF | 495 |
| p-value | 0.478 |
| Inter-instrument norm. | 1.82 (1.67–1.94) |
| 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.