5XMM J183601.7-592045
5XMM-DR15 stacked source · SRCID 3002294010100113
Position:
18h36m01.74s -59d20m45.1s
(279.00726°, -59.34587°)
EP flux
1.12e-15
± 1.4e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.439)
Detections
5
| SRCID | 3002294010100113 |
|---|---|
| IAUNAME | 5XMM J183601.7-592045 |
| SC_RA | 18h36m01.74s (279.00726°) |
| SC_DEC | -59d20m45.1s (-59.34587°) |
| RADEC_ERR | 2.22 arcsec |
| LII / BII | 336.0019° / -21.2095° |
| 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): 1.12e-15 ± 1.4e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.01
± 0.38
0.2-0.5 / 0.5-1.0 keV
HR2
-0.73
± 0.65
0.5-1.0 / 1.0-2.0 keV
HR3
0.00
± 1.69
1.0-2.0 / 2.0-4.5 keV
HR4
0.13
± 1.48
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.35
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
- 5554654
- Match probability
- 0.593
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 23.430 | 0.363 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.19e-15 (+9.1e-15 / −5.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 4.79e+19 (+1.9e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 2.83 (+2.96 / −2.62) |
| DoF | 194 |
| p-value | 0.06 |
| 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.