5XMM J183543.8-343125
5XMM-DR15 stacked source · SRCID 3005094040100003
Position:
18h35m43.81s -34d31m25.0s
(278.93253°, -34.52361°)
EP flux
3.19e-14
± 5.4e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.542)
Detections
2
| SRCID | 3005094040100003 |
|---|---|
| IAUNAME | 5XMM J183543.8-343125 |
| SC_RA | 18h35m43.81s (278.93253°) |
| SC_DEC | -34d31m25.0s (-34.52361°) |
| RADEC_ERR | 0.57 arcsec |
| LII / BII | 0.1118° / -12.0175° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52347.471 (2002-03-14 11:18:21.000 UTC) |
| MJD_LAST | 53282.698 (2004-10-04 16:44:32.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.19e-14 ± 5.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.66
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.85
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.38
± 0.47
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.6)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.64
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
- 5550143
- Match probability
- 0.876
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.130 | 0.051 |
| U | 17.905 | 0.017 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.61e-14 (+3.1e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.78e+20 (+1.6e+21 / −3.0e+20) cm−2 |
| Photon index (Γ) | 2.76 (+2.93 / −2.42) |
| DoF | 89 |
| p-value | 0.195 |
| 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.