5XMM J004311.6-093814
5XMM-DR15 stacked source · SRCID 3006514020100019
Position:
00h43m11.62s -09d38m14.7s
(10.79842°, -9.63740°)
EP flux
6.79e-13
± 4.7e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.904)
Detections
1
| SRCID | 3006514020100019 |
|---|---|
| IAUNAME | 5XMM J004311.6-093814 |
| SC_RA | 00h43m11.62s (10.79842°) |
| SC_DEC | -09d38m14.7s (-9.63740°) |
| RADEC_ERR | 0.26 arcsec |
| LII / BII | 116.1973° / -72.4013° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52281.739 (2002-01-07 17:43:45.000 UTC) |
| MJD_LAST | 52281.884 (2002-01-07 21:12:30.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.79e-13 ± 4.7e-14 erg cm-2 s-1
Hardness ratios
HR1
0.14
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.02
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.22
± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.32
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.51e-13 (+4.8e-13 / −4.3e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.35e+19 (+1.3e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 1.92 (+1.99 / −1.87) |
| DoF | 625 |
| p-value | 0.799 |
| Inter-instrument norm. | 1.11 (1.02–1.19) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 11.100 (approximate flux variability amplitude) |
|---|
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.