5XMM J005802.5-721207
5XMM-DR15 stacked source · SRCID 3001854010100093
Position:
00h58m02.56s -72d12m07.4s
(14.51065°, -72.20206°)
EP flux
6.44e-14
± 3.9e-15
erg cm-2 s-1
CLASSX
AGN
(0.723)
Detections
19
| SRCID | 3001854010100093 |
|---|---|
| IAUNAME | 5XMM J005802.5-721207 |
| SC_RA | 00h58m02.56s (14.51065°) |
| SC_DEC | -72d12m07.4s (-72.20206°) |
| RADEC_ERR | 0.15 arcsec |
| LII / BII | 302.2193° / -44.9171° |
| N_CONTRIB | 19 (detections) |
| N_OBS | 182 (observations covering the position) |
| MJD_FIRST | 51834.632 (2000-10-17 15:10:35.000 UTC) |
| MJD_LAST | 58925.579 (2020-03-17 13:54:08.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.44e-14 ± 3.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.83
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.38
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.41
± 0.06
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.326
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 | 5.58e-14 (+6.2e-14 / −5.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.89e+21 (+2.3e+21 / −1.5e+21) cm−2 |
| Photon index (Γ) | 1.83 (+1.95 / −1.72) |
| DoF | 1010 |
| p-value | 0.746 |
| Inter-instrument norm. | 1.76 (1.61–1.91) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 21.900 (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.