5XMM J124941.1-412827
5XMM-DR15 stacked source · SRCID 3004634010100163
Position:
12h49m41.15s -41d28m27.0s
(192.42148°, -41.47418°)
EP flux
1.68e-14
± 2.3e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.66)
Detections
8
| SRCID | 3004634010100163 |
|---|---|
| IAUNAME | 5XMM J124941.1-412827 |
| SC_RA | 12h49m41.15s (192.42148°) |
| SC_DEC | -41d28m27.0s (-41.47418°) |
| RADEC_ERR | 0.45 arcsec |
| LII / BII | 302.5794° / 21.3964° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 12 (observations covering the position) |
| MJD_FIRST | 52277.006 (2002-01-03 00:08:36.000 UTC) |
| MJD_LAST | 58666.366 (2019-07-02 08:46:52.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.68e-14 ± 2.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.72
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.48
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.19
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.27
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 3.4)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.87
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 | 2.88e-14 (+3.3e-14 / −2.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.18e+20 (+9.8e+20 / −3.6e+19) cm−2 |
| Photon index (Γ) | 1.38 (+1.57 / −1.22) |
| DoF | 583 |
| p-value | 0.546 |
| Inter-instrument norm. | 0.86 (0.71–1.03) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 6.500 (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.