5XMM J092251.1-632405
5XMM-DR15 stacked source · SRCID 3005159010100107
Position:
09h22m51.16s -63d24m05.3s
(140.71316°, -63.40148°)
EP flux
1.60e-14
± 3.9e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.592)
Detections
2
| SRCID | 3005159010100107 |
|---|---|
| IAUNAME | 5XMM J092251.1-632405 |
| SC_RA | 09h22m51.16s (140.71316°) |
| SC_DEC | -63d24m05.3s (-63.40148°) |
| RADEC_ERR | 1.19 arcsec |
| LII / BII | 281.9344° / -9.3926° |
| 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): 1.60e-14 ± 3.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.83
± 0.22
0.2-0.5 / 0.5-1.0 keV
HR2
-0.20
± 0.25
0.5-1.0 / 1.0-2.0 keV
HR3
0.48
± 0.19
1.0-2.0 / 2.0-4.5 keV
HR4
-0.07
± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 7.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.21
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
- 2739677
- Match probability
- 0.899
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.489 | 0.126 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.13e-15 (+6.5e-15 / −2.2e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.50e+20 (+1.1e+21 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.52 (+2.02 / −1.17) |
| DoF | 100 |
| p-value | 0.106 |
| 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.