5XMM J005525.1-011506
| SRCID | 3001244010100088 |
|---|---|
| IAUNAME | 5XMM J005525.1-011506 |
| SC_RA | 00h55m25.11s (13.85463°) |
| SC_DEC | -01d15m06.0s (-1.25166°) |
| RADEC_ERR | 0.78 arcsec |
| LII / BII | 125.2106° / -64.1058° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 51923.975 (2001-01-14 23:23:18.000 UTC) |
| MJD_LAST | 57210.407 (2015-07-07 09:46:43.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.08e-15 ± 1.3e-15 erg cm-2 s-1
Hardness ratios
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.414
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
- 325747
- Match probability
- 0.984
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.968 | 0.219 |
| B | — | — |
| V | — | — |
- Name
- J005524.91-011505.8
- Match probability
- 0.995
| Band | Mag | Err |
|---|---|---|
| W1 | 17.153 | 0.150 |
| W2 | 16.626 | — |
| W3 | 11.490 | — |
| W4 | 8.512 | — |
- Class
- QSO
| Photometric (TPZ) | 1.8255 (conf 0.58) |
|---|---|
| Photometric (Le Phare) | 1.4330 (conf 0.53) |
Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.
Stacked power-law fit
| Unabsorbed flux | 7.59e-15 (+9.1e-15 / −6.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 4.71e+19 (+1.8e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 1.89 (+2.06 / −1.71) |
| DoF | 324 |
| p-value | 0.698 |
| Inter-instrument norm. | 0.90 (0.69–1.14) |
| 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.