5XMM J222056.5-244200
5XMM-DR15 stacked source · SRCID 3004934020100011
Position:
22h20m56.53s -24d42m00.9s
(335.23554°, -24.70026°)
EP flux
3.86e-14
± 6.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.976)
Detections
1
| SRCID | 3004934020100011 |
|---|---|
| IAUNAME | 5XMM J222056.5-244200 |
| SC_RA | 22h20m56.53s (335.23554°) |
| SC_DEC | -24d42m00.9s (-24.70026°) |
| RADEC_ERR | 0.58 arcsec |
| LII / BII | 28.4176° / -56.1964° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52226.944 (2001-11-13 22:38:42.000 UTC) |
| MJD_LAST | 52227.263 (2001-11-14 06:18:58.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.86e-14 ± 6.1e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.03
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.14
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.50
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.58
± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.622
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
- 6453556
- Match probability
- 0.99
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.346 | 0.130 |
| U | 20.431 | 0.115 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.64e-14 (+3.1e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.82e+19 (+3.7e+20 / −2.0e+19) cm−2 |
| Photon index (Γ) | 2.17 (+2.42 / −1.97) |
| DoF | 99 |
| p-value | 0.842 |
| 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.