5XMM J183703.1-593056
5XMM-DR15 stacked source · SRCID 3002294010100005
Position:
18h37m03.12s -59d30m56.1s
(279.26302°, -59.51559°)
EP flux
9.70e-14
± 5.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.77)
Detections
5
| SRCID | 3002294010100005 |
|---|---|
| IAUNAME | 5XMM J183703.1-593056 |
| SC_RA | 18h37m03.12s (279.26302°) |
| SC_DEC | -59d30m56.1s (-59.51559°) |
| RADEC_ERR | 0.25 arcsec |
| LII / BII | 335.8705° / -21.3848° |
| 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): 9.70e-14 ± 5.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.40
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.23
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.36
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.52
± 0.06
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 25.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 2.27
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
- 5561231
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.195 | 0.028 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 9.65e-14 (+1.0e-13 / −9.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.88e+20 (+1.0e+21 / −3.4e+20) cm−2 |
| Photon index (Γ) | 1.79 (+1.92 / −1.65) |
| DoF | 460 |
| p-value | 0.36 |
| 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.