5XMM J133542.1-341811
5XMM-DR15 stacked source · SRCID 3002974010100016
Position:
13h35m42.14s -34d18m11.6s
(203.92558°, -34.30321°)
EP flux
2.56e-14
± 1.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.758)
Detections
5
| SRCID | 3002974010100016 |
|---|---|
| IAUNAME | 5XMM J133542.1-341811 |
| SC_RA | 13h35m42.14s (203.92558°) |
| SC_DEC | -34d18m11.6s (-34.30321°) |
| RADEC_ERR | 0.28 arcsec |
| LII / BII | 313.2462° / 27.6804° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 10 (observations covering the position) |
| MJD_FIRST | 51736.296 (2000-07-11 07:06:18.000 UTC) |
| MJD_LAST | 52126.638 (2001-08-05 15:18:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.56e-14 ± 1.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.32
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.02
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.51
± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.923
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
- 3511914
- Match probability
- 0.981
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.315 | 0.062 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.17e-14 (+2.5e-14 / −1.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.09e+19 (+2.8e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 1.65 (+1.79 / −1.53) |
| DoF | 772 |
| p-value | 0.689 |
| Inter-instrument norm. | 1.74 (1.55–1.92) |
| 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.