5XMM J022250.9+425918
5XMM-DR15 stacked source · SRCID 3000297020100381
Position:
02h22m50.92s +42d59m18.4s
(35.71216°, 42.98845°)
EP flux
6.73e-15
± 3.2e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.975)
Detections
1
| SRCID | 3000297020100381 |
|---|---|
| IAUNAME | 5XMM J022250.9+425918 |
| SC_RA | 02h22m50.92s (35.71216°) |
| SC_DEC | +42d59m18.4s (42.98845°) |
| RADEC_ERR | 2.03 arcsec |
| LII / BII | 140.1942° / -16.7984° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 9 (observations covering the position) |
| MJD_FIRST | 52310.692 (2002-02-05 16:35:53.000 UTC) |
| MJD_LAST | 52310.949 (2002-02-05 22:46:20.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.73e-15 ± 3.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.73
± 0.18
0.2-0.5 / 0.5-1.0 keV
HR2
-0.58
± 0.23
0.5-1.0 / 1.0-2.0 keV
HR3
-0.04
± 0.41
1.0-2.0 / 2.0-4.5 keV
HR4
-0.60
± 0.50
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 1.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.05
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
- 798167
- Match probability
- 0.965
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.192 | 0.093 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.12e-14 (+1.6e-14 / −6.6e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.37e+20 (+7.6e+20 / −2.6e+19) cm−2 |
| Photon index (Γ) | 1.60 (+2.20 / −1.25) |
| DoF | 85 |
| p-value | 0.48 |
| 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.