5XMM J131539.9-162757
5XMM-DR15 stacked source · SRCID 3003795010100149
Position:
13h15m39.98s -16d27m57.8s
(198.91657°, -16.46605°)
EP flux
1.37e-14
± 2.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.923)
Detections
2
| SRCID | 3003795010100149 |
|---|---|
| IAUNAME | 5XMM J131539.9-162757 |
| SC_RA | 13h15m39.98s (198.91657°) |
| SC_DEC | -16d27m57.8s (-16.46605°) |
| RADEC_ERR | 0.65 arcsec |
| LII / BII | 311.3098° / 46.0112° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 51921.880 (2001-01-12 21:07:12.000 UTC) |
| MJD_LAST | 54829.307 (2008-12-29 07:22:25.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.37e-14 ± 2.8e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.10
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.46
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.50
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
0.17
± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.254
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
- 3444825
- Match probability
- 0.986
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.961 | 0.203 |
| B | — | — |
| V | 20.716 | 0.262 |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.29e-14 (+1.7e-14 / −9.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 8.43e+19 (+4.4e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 1.53 (+1.78 / −1.32) |
| DoF | 601 |
| p-value | 0.782 |
| 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.