5XMM J005846.0-715810
5XMM-DR15 stacked source · SRCID 3001854010100746
Position:
00h58m46.09s -71d58m10.0s
(14.69202°, -71.96946°)
EP flux
2.27e-14
± 3.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.745)
Detections
15
| SRCID | 3001854010100746 |
|---|---|
| IAUNAME | 5XMM J005846.0-715810 |
| SC_RA | 00h58m46.09s (14.69202°) |
| SC_DEC | -71d58m10.0s (-71.96946°) |
| RADEC_ERR | 0.50 arcsec |
| LII / BII | 302.1278° / -45.1473° |
| N_CONTRIB | 15 (detections) |
| N_OBS | 182 (observations covering the position) |
| MJD_FIRST | 51834.632 (2000-10-17 15:10:35.000 UTC) |
| MJD_LAST | 57725.009 (2016-12-03 00:13:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.27e-14 ± 3.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.81
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.47
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.30
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43
± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.748
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 | 1.57e-14 (+2.0e-14 / −1.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.83e+21 (+4.9e+21 / −1.6e+20) cm−2 |
| Photon index (Γ) | 1.51 (+2.06 / −1.15) |
| DoF | 217 |
| p-value | 0.869 |
| Inter-instrument norm. | 1.04 (0.77–1.42) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 12.600 (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.