5XMM J182816.0-115433
5XMM-DR15 stacked source · SRCID 3005194040100122
Position:
18h28m16.00s -11d54m33.8s
(277.06665°, -11.90938°)
EP flux
1.56e-13
± 2.6e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.517)
Detections
1
| SRCID | 3005194040100122 |
|---|---|
| IAUNAME | 5XMM J182816.0-115433 |
| SC_RA | 18h28m16.00s (277.06665°) |
| SC_DEC | -11d54m33.8s (-11.90938°) |
| RADEC_ERR | 0.67 arcsec |
| LII / BII | 19.7114° / -0.3555° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 71 (observations covering the position) |
| MJD_FIRST | 51978.670 (2001-03-10 16:04:14.000 UTC) |
| MJD_LAST | 51978.775 (2001-03-10 18:36:42.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.56e-13 ± 2.6e-14 erg cm-2 s-1
Hardness ratios
HR1
0.91
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.76
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.17
± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.38
± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 5.25
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
- 5430283
- Match probability
- 0.887
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 17.654 | 0.083 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.74e-13 (+2.1e-13 / −1.4e-13) erg cm−2 s−1 |
|---|---|
| NH | 4.35e+21 (+6.3e+21 / −2.7e+21) cm−2 |
| Photon index (Γ) | 1.60 (+1.95 / −1.28) |
| DoF | 350 |
| p-value | 0.982 |
| 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.