5XMM J101127.3-044427
5XMM-DR15 stacked source · SRCID 3002634020100012
Position:
10h11m27.39s -04d44m27.7s
(152.86413°, -4.74103°)
EP flux
3.76e-14
± 1.7e-14
erg cm-2 s-1
CLASSX
AGN
(0.952)
Detections
1
| SRCID | 3002634020100012 |
|---|---|
| IAUNAME | 5XMM J101127.3-044427 |
| SC_RA | 10h11m27.39s (152.86413°) |
| SC_DEC | -04d44m27.7s (-4.74103°) |
| RADEC_ERR | 1.21 arcsec |
| LII / BII | 246.2909° / 39.9259° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52240.189 (2001-11-27 04:31:28.000 UTC) |
| MJD_LAST | 52240.410 (2001-11-27 09:50:23.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.76e-14 ± 1.7e-14 erg cm-2 s-1
Hardness ratios
HR1
0.50
± 0.37
0.2-0.5 / 0.5-1.0 keV
HR2
0.60
± 0.17
0.5-1.0 / 1.0-2.0 keV
HR3
-0.18
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.56
± 0.28
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.207
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.
Optical Monitor (OM)
- OM Source ID
- 2834814
- Match probability
- 0.979
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 19.733 | 0.202 |
| UVM2 | — | — |
| UVW1 | 19.454 | 0.094 |
| U | 19.675 | 0.098 |
| B | 19.261 | 0.113 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.62e-14 (+9.0e-14 / −4.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.31e+20 (+8.0e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.29 (+1.65 / −1.09) |
| DoF | 175 |
| p-value | 0.131 |
| Quality flag | 0 |
No variability data available for this source.
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.