5XMM J223604.2+340745
5XMM-DR15 stacked source · SRCID 3002114020100066
Position:
22h36m04.24s +34d07m45.8s
(339.01768°, 34.12938°)
EP flux
1.60e-14
± 6.9e-15
erg cm-2 s-1
CLASSX
Star
(0.342)
Detections
1
| SRCID | 3002114020100066 |
|---|---|
| IAUNAME | 5XMM J223604.2+340745 |
| SC_RA | 22h36m04.24s (339.01768°) |
| SC_DEC | +34d07m45.8s (34.12938°) |
| RADEC_ERR | 0.94 arcsec |
| LII / BII | 93.3730° / -20.8583° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52250.890 (2001-12-07 21:22:09.000 UTC) |
| MJD_LAST | 52251.416 (2001-12-08 09:59:17.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.60e-14 ± 6.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.59
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.33
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.73
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
0.63
± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.26
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
- 6473133
- Match probability
- 0.963
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 20.565 | 0.154 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.18e-14 (+1.5e-14 / −9.6e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.00e+21 (+1.7e+21 / −1.9e+20) cm−2 |
| Photon index (Γ) | 2.47 (+2.83 / −2.01) |
| DoF | 129 |
| p-value | 0.491 |
| 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.