5XMM J223125.7+392904
5XMM-DR15 stacked source · SRCID 3000297010100009
Position:
22h31m25.74s +39d29m04.9s
(337.85724°, 39.48470°)
EP flux
9.03e-14
± 1.5e-14
erg cm-2 s-1
CLASSX
AGN
(0.929)
Detections
1
| SRCID | 3000297010100009 |
|---|---|
| IAUNAME | 5XMM J223125.7+392904 |
| SC_RA | 22h31m25.74s (337.85724°) |
| SC_DEC | +39d29m04.9s (39.48470°) |
| RADEC_ERR | 0.59 arcsec |
| LII / BII | 95.5352° / -15.8252° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52252.872 (2001-12-09 20:56:07.000 UTC) |
| MJD_LAST | 52253.117 (2001-12-10 02:48:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.03e-14 ± 1.5e-14 erg cm-2 s-1
Hardness ratios
HR1
0.36
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.25
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.33
± 0.16
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.391
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
- 6469290
- Match probability
- 0.984
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.345 | 0.318 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.20e-14 (+9.5e-14 / −7.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.66e+20 (+5.8e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.52 (+1.70 / −1.40) |
| DoF | 201 |
| p-value | 0.898 |
| Inter-instrument norm. | 0.82 (0.70–0.96) |
| 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.