5XMM J010023.2-721129
5XMM-DR15 stacked source · SRCID 3001854010100187
Position:
01h00m23.29s -72d11m29.7s
(15.09703°, -72.19157°)
EP flux
2.04e-14
± 2.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.807)
Detections
14
| SRCID | 3001854010100187 |
|---|---|
| IAUNAME | 5XMM J010023.2-721129 |
| SC_RA | 01h00m23.29s (15.09703°) |
| SC_DEC | -72d11m29.7s (-72.19157°) |
| RADEC_ERR | 0.24 arcsec |
| LII / BII | 301.9657° / -44.9199° |
| N_CONTRIB | 14 (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): 2.04e-14 ± 2.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.13
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.04
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.50
± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.727
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 | 1.36e-14 (+1.6e-14 / −1.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.39e+19 (+1.3e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 2.75 (+2.91 / −2.59) |
| DoF | 305 |
| p-value | 0.379 |
| Inter-instrument norm. | 0.73 (0.60–0.88) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 7.100 (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.