5XMM J111200.6-604037
5XMM-DR15 stacked source · SRCID 3005155010100041
Position:
11h12m00.67s -60d40m37.1s
(168.00279°, -60.67697°)
EP flux
9.44e-15
± 1.9e-15
erg cm-2 s-1
CLASSX
Star
(0.96)
Detections
2
| SRCID | 3005155010100041 |
|---|---|
| IAUNAME | 5XMM J111200.6-604037 |
| SC_RA | 11h12m00.67s (168.00279°) |
| SC_DEC | -60d40m37.1s (-60.67697°) |
| RADEC_ERR | 0.71 arcsec |
| LII / BII | 291.0521° / -0.1192° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52311.055 (2002-02-06 01:19:43.000 UTC) |
| MJD_LAST | 57188.569 (2015-06-15 13:38:48.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.44e-15 ± 1.9e-15 erg cm-2 s-1
Hardness ratios
HR1
-1.00
± 2.30
0.2-0.5 / 0.5-1.0 keV
HR2
1.00
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
0.46
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.52
± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.61
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 | 1.44e-14 (+1.9e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.05e+21 (+1.1e+22 / −3.2e+21) cm−2 |
| Photon index (Γ) | 1.56 (+2.12 / −1.19) |
| DoF | 1031 |
| p-value | 0.692 |
| Inter-instrument norm. | 1.56 (1.22–1.86) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 33.100 (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.