5XMM J223655.6-152247
5XMM-DR15 stacked source · SRCID 3005602160100010
Position:
22h36m55.67s -15d22m47.6s
(339.23196°, -15.37988°)
EP flux
1.70e-14
± 4.3e-15
erg cm-2 s-1
CLASSX
AGN
(0.939)
Detections
1
| SRCID | 3005602160100010 |
|---|---|
| IAUNAME | 5XMM J223655.6-152247 |
| SC_RA | 22h36m55.67s (339.23196°) |
| SC_DEC | -15d22m47.6s (-15.37988°) |
| RADEC_ERR | 0.67 arcsec |
| LII / BII | 46.6192° / -56.6627° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52241.253 (2001-11-28 06:04:43.000 UTC) |
| MJD_LAST | 52241.535 (2001-11-28 12:50:55.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.70e-14 ± 4.3e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.24
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.29
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.55
± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00
± 0.46
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.428
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
- 6474626
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.691 | 0.120 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.14e-14 (+1.3e-14 / −9.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 5.44e+19 (+2.3e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 2.77 (+2.92 / −2.56) |
| DoF | 106 |
| p-value | 0.283 |
| 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.