5XMM J092257.7-631459
5XMM-DR15 stacked source · SRCID 3005159010100047
Position:
09h22m57.74s -63d14m59.7s
(140.74058°, -63.24991°)
EP flux
2.26e-14
± 9.0e-15
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
2
| SRCID | 3005159010100047 |
|---|---|
| IAUNAME | 5XMM J092257.7-631459 |
| SC_RA | 09h22m57.74s (140.74058°) |
| SC_DEC | -63d14m59.7s (-63.24991°) |
| RADEC_ERR | 2.80 arcsec |
| LII / BII | 281.8338° / -9.2775° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 51898.315 (2000-12-20 07:32:54.000 UTC) |
| MJD_LAST | 51899.141 (2000-12-21 03:23:20.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.26e-14 ± 9.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.61
± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.38
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.82
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
26.38
± 2.41
arcsec
(ML 41.7)
SUM_FLAG:
3
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.41
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
- 2739860
- Match probability
- 0.655
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.143 | 0.127 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.40e-14 (+1.9e-14 / −1.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.92e+20 (+3.3e+21 / −6.8e+19) cm−2 |
| Photon index (Γ) | 1.57 (+2.13 / −1.22) |
| DoF | 213 |
| p-value | 0.973 |
| 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.