5XMM J022311.4+425932
5XMM-DR15 stacked source · SRCID 3000297020100012
Position:
02h23m11.48s +42d59m32.0s
(35.79782°, 42.99222°)
EP flux
5.10e-13
± 1.3e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.96)
Detections
1
| SRCID | 3000297020100012 |
|---|---|
| IAUNAME | 5XMM J022311.4+425932 |
| SC_RA | 02h23m11.48s (35.79782°) |
| SC_DEC | +42d59m32.0s (42.99222°) |
| RADEC_ERR | 0.13 arcsec |
| LII / BII | 140.2538° / -16.7722° |
| 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): 5.10e-13 ± 1.3e-14 erg cm-2 s-1
Hardness ratios
HR1
0.49
± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
-0.10
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.52
± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.62
± 0.03
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 73.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.44
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
- 800816
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 17.737 | 0.017 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.91e-13 (+4.0e-13 / −3.8e-13) erg cm−2 s−1 |
|---|---|
| NH | 1.65e+21 (+1.8e+21 / −1.5e+21) cm−2 |
| Photon index (Γ) | 2.71 (+2.79 / −2.63) |
| DoF | 713 |
| p-value | 0.004 |
| 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.