5XMM J233833.2+270212
5XMM-DR15 stacked source · SRCID 3000296010100019
Position:
23h38m33.23s +27d02m12.0s
(354.63846°, 27.03668°)
EP flux
1.43e-13
± 3.6e-14
erg cm-2 s-1
CLASSX
Extended
(0.999)
Detections
4
| SRCID | 3000296010100019 |
|---|---|
| IAUNAME | 5XMM J233833.2+270212 |
| SC_RA | 23h38m33.23s (354.63846°) |
| SC_DEC | +27d02m12.0s (27.03668°) |
| RADEC_ERR | 6.22 arcsec |
| LII / BII | 103.5197° / -33.0728° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 52447.215 (2002-06-22 05:09:35.000 UTC) |
| MJD_LAST | 57944.424 (2017-07-10 10:10:45.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.43e-13 ± 3.6e-14 erg cm-2 s-1
Hardness ratios
HR1
0.80
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.04
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.66
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.51
± 0.36
2.0-4.5 / 4.5-12.0 keV
Extent:
40.41
± 3.26
arcsec
(ML 30.0)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.07
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
- 6608440
- Match probability
- 0.764
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 16.889 | 0.020 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.62e-14 (+3.0e-14 / −6.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.07e+20 (+2.7e+21 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.68 (+2.38 / −1.21) |
| DoF | 97 |
| p-value | 0.476 |
| 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.