5XMM J230754.1-020817
5XMM-DR15 stacked source · SRCID 3004234120100003
Position:
23h07m54.18s -02d08m17.2s
(346.97576°, -2.13810°)
EP flux
9.77e-14
± 2.1e-14
erg cm-2 s-1
CLASSX
Star
(0.902)
Detections
2
| SRCID | 3004234120100003 |
|---|---|
| IAUNAME | 5XMM J230754.1-020817 |
| SC_RA | 23h07m54.18s (346.97576°) |
| SC_DEC | -02d08m17.2s (-2.13810°) |
| RADEC_ERR | 0.57 arcsec |
| LII / BII | 73.7467° / -54.8016° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52070.285 (2001-06-10 06:49:52.000 UTC) |
| MJD_LAST | 53161.188 (2004-06-05 04:30:57.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.77e-14 ± 2.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.75
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.33
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.90
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
0.37
± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.38
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
- 6530050
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 19.565 | 0.144 |
| UVM2 | 19.816 | 0.172 |
| UVW1 | 16.874 | 0.011 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 9.35e-14 (+1.0e-13 / −8.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.06e+21 (+2.3e+21 / −1.8e+21) cm−2 |
| Photon index (Γ) | 2.92 (+2.98 / −2.79) |
| DoF | 249 |
| p-value | 0.035 |
| 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.