5XMM J005912.6-722229
5XMM-DR15 stacked source · SRCID 3001854010100907
Position:
00h59m12.67s -72d22m29.7s
(14.80279°, -72.37492°)
EP flux
1.52e-13
± 1.8e-14
erg cm-2 s-1
CLASSX
Extended
(0.997)
Detections
21
| SRCID | 3001854010100907 |
|---|---|
| IAUNAME | 5XMM J005912.6-722229 |
| SC_RA | 00h59m12.67s (14.80279°) |
| SC_DEC | -72d22m29.7s (-72.37492°) |
| RADEC_ERR | 3.37 arcsec |
| LII / BII | 302.1037° / -44.7408° |
| N_CONTRIB | 21 (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): 1.52e-13 ± 1.8e-14 erg cm-2 s-1
Hardness ratios
HR1
0.65
± 0.50
0.2-0.5 / 0.5-1.0 keV
HR2
0.89
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
0.17
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.22
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
39.93
± 5.76
arcsec
(ML 35.8)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.97
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 | 9.64e-14 (+1.0e-13 / −9.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.06e+21 (+5.8e+21 / −4.5e+21) cm−2 |
| Photon index (Γ) | 1.83 (+1.95 / −1.71) |
| DoF | 786 |
| p-value | 0.001 |
| Inter-instrument norm. | 1.98 (1.94–1.99) |
| Quality flag | 5 |
| APPROX_SOURCE_VAR | 25.500 (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.