5XMM J133628.3-342108
5XMM-DR15 stacked source · SRCID 3002974010100160
Position:
13h36m28.33s -34d21m08.5s
(204.11804°, -34.35237°)
EP flux
4.14e-15
± 1.5e-15
erg cm-2 s-1
CLASSX
AGN
(0.806)
Detections
8
| SRCID | 3002974010100160 |
|---|---|
| IAUNAME | 5XMM J133628.3-342108 |
| SC_RA | 13h36m28.33s (204.11804°) |
| SC_DEC | -34d21m08.5s (-34.35237°) |
| RADEC_ERR | 0.73 arcsec |
| LII / BII | 313.4114° / 27.6013° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 10 (observations covering the position) |
| MJD_FIRST | 51736.296 (2000-07-11 07:06:18.000 UTC) |
| MJD_LAST | 56326.065 (2013-02-03 01:33:27.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.14e-15 ± 1.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.64
± 0.54
0.2-0.5 / 0.5-1.0 keV
HR2
0.57
± 0.20
0.5-1.0 / 1.0-2.0 keV
HR3
-0.02
± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.57
± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.922
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
- 3514840
- Match probability
- 0.977
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.844 | 0.185 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.73e-15 (+1.3e-14 / −5.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.70e+20 (+9.5e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.83 (+2.37 / −1.42) |
| DoF | 125 |
| p-value | 0.258 |
| 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.