5XMM J183621.4-591740
5XMM-DR15 stacked source · SRCID 3002294010100063
Position:
18h36m21.41s -59d17m40.2s
(279.08922°, -59.29450°)
EP flux
1.13e-14
± 3.1e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.762)
Detections
5
| SRCID | 3002294010100063 |
|---|---|
| IAUNAME | 5XMM J183621.4-591740 |
| SC_RA | 18h36m21.41s (279.08922°) |
| SC_DEC | -59d17m40.2s (-59.29450°) |
| RADEC_ERR | 1.04 arcsec |
| LII / BII | 336.0681° / -21.2337° |
| 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): 1.13e-14 ± 3.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.17
± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
0.26
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.68
± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 12.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.73
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
- 5557933
- Match probability
- 0.947
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.710 | 0.183 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.28e-14 (+1.7e-14 / −9.9e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.48e+20 (+1.1e+21 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.72 (+2.09 / −1.41) |
| DoF | 80 |
| p-value | 0.74 |
| 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.