5XMM J092217.9-631522
5XMM-DR15 stacked source · SRCID 3005159010100009
Position:
09h22m17.98s -63d15m22.2s
(140.57494°, -63.25618°)
EP flux
1.86e-14
± 1.7e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
2
| SRCID | 3005159010100009 |
|---|---|
| IAUNAME | 5XMM J092217.9-631522 |
| SC_RA | 09h22m17.98s (140.57494°) |
| SC_DEC | -63d15m22.2s (-63.25618°) |
| RADEC_ERR | 0.31 arcsec |
| LII / BII | 281.7853° / -9.3350° |
| 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): 1.86e-14 ± 1.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.77
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
-0.69
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-1.00
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
0.60
± 1.80
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 0.976
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
- 2738465
- Match probability
- 0.987
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 14.528 | 0.009 |
| UVM2 | 14.179 | 0.005 |
| UVW1 | 12.223 | 0.001 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.04e-14 (+2.3e-14 / −1.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.53e+20 (+1.2e+21 / −2.6e+20) cm−2 |
| Photon index (Γ) | 2.88 (+2.97 / −2.72) |
| DoF | 109 |
| p-value | 0.007 |
| Quality flag | 5 |
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.