5XMM J011141.1-380750
5XMM-DR15 stacked source · SRCID 3000294230100039
Position:
01h11m41.14s -38d07m50.4s
(17.92143°, -38.13065°)
EP flux
1.04e-14
± 2.2e-15
erg cm-2 s-1
CLASSX
AGN
(0.935)
Detections
2
| SRCID | 3000294230100039 |
|---|---|
| IAUNAME | 5XMM J011141.1-380750 |
| SC_RA | 01h11m41.14s (17.92143°) |
| SC_DEC | -38d07m50.4s (-38.13065°) |
| RADEC_ERR | 0.62 arcsec |
| LII / BII | 283.0817° / -78.2060° |
| 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): 1.04e-14 ± 2.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.28
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.16
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.28
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.17
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.652
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
- 542412
- Match probability
- 0.989
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 23.027 | 0.306 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.73e-15 (+8.8e-15 / −4.8e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.61e+19 (+4.0e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 1.83 (+2.16 / −1.59) |
| DoF | 565 |
| p-value | 0.792 |
| 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.