5XMM J183609.8-591803
5XMM-DR15 stacked source · SRCID 3002294010100025
Position:
18h36m09.84s -59d18m03.7s
(279.04100°, -59.30103°)
EP flux
2.46e-14
± 4.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.803)
Detections
5
| SRCID | 3002294010100025 |
|---|---|
| IAUNAME | 5XMM J183609.8-591803 |
| SC_RA | 18h36m09.84s (279.04100°) |
| SC_DEC | -59d18m03.7s (-59.30103°) |
| RADEC_ERR | 0.34 arcsec |
| LII / BII | 336.0534° / -21.2123° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 51973.598 (2001-03-05 14:20:50.000 UTC) |
| MJD_LAST | 58005.921 (2017-09-09 22:05:47.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.46e-14 ± 4.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.36
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.28
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.51
± 0.16
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.678
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
- 5556200
- Match probability
- 0.585
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.040 | 0.070 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.69e-14 (+4.3e-14 / −3.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 9.15e+19 (+4.4e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.78 (+2.00 / −1.64) |
| DoF | 195 |
| p-value | 0.973 |
| 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.