5XMM J011134.9-375716
5XMM-DR15 stacked source · SRCID 3000294230100019
Position:
01h11m34.96s -37d57m16.6s
(17.89565°, -37.95460°)
EP flux
1.89e-14
± 4.9e-15
erg cm-2 s-1
CLASSX
AGN
(0.929)
Detections
2
| SRCID | 3000294230100019 |
|---|---|
| IAUNAME | 5XMM J011134.9-375716 |
| SC_RA | 01h11m34.96s (17.89565°) |
| SC_DEC | -37d57m16.6s (-37.95460°) |
| RADEC_ERR | 0.50 arcsec |
| LII / BII | 282.8391° / -78.3763° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52253.198 (2001-12-10 04:44:57.000 UTC) |
| MJD_LAST | 54809.311 (2008-12-09 07:28:24.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.89e-14 ± 4.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.21
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.08
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.28
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.30
± 0.27
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.349
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.
Optical Monitor (OM)
- OM Source ID
- 541548
- Match probability
- 0.956
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 23.028 | 0.249 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.99e-14 (+2.3e-14 / −1.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.76e+20 (+6.4e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.66 (+1.88 / −1.52) |
| DoF | 783 |
| p-value | 0.935 |
| Inter-instrument norm. | 1.00 (0.87–1.17) |
| 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.