5XMM J233949.8-121305
5XMM-DR15 stacked source · SRCID 3005599030100011
Position:
23h39m49.83s -12d13m05.0s
(354.95762°, -12.21804°)
EP flux
7.25e-14
± 1.1e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
1
| SRCID | 3005599030100011 |
|---|---|
| IAUNAME | 5XMM J233949.8-121305 |
| SC_RA | 23h39m49.83s (354.95762°) |
| SC_DEC | -12d13m05.0s (-12.21804°) |
| RADEC_ERR | 1.63 arcsec |
| LII / BII | 71.0514° / -67.5506° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52241.584 (2001-11-28 14:00:26.000 UTC) |
| MJD_LAST | 52241.750 (2001-11-28 17:59:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.25e-14 ± 1.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.54
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.23
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.95
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.76
± 0.61
2.0-4.5 / 4.5-12.0 keV
Extent:
13.60
± 1.08
arcsec
(ML 131.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.18
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
- 6611915
- Match probability
- 0.988
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 20.030 | 0.116 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.66e-14 (+3.1e-14 / −2.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.94e+21 (+2.5e+21 / −1.3e+21) cm−2 |
| Photon index (Γ) | 2.78 (+2.95 / −2.49) |
| DoF | 76 |
| p-value | 0.254 |
| 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.