5XMM J185137.3-000332
5XMM-DR15 stacked source · SRCID 3001774040100005
Position:
18h51m37.31s -00d03m32.1s
(282.90545°, -0.05890°)
EP flux
1.17e-13
± 9.0e-15
erg cm-2 s-1
CLASSX
Gal_XRB
(0.449)
Detections
3
| SRCID | 3001774040100005 |
|---|---|
| IAUNAME | 5XMM J185137.3-000332 |
| SC_RA | 18h51m37.31s (282.90545°) |
| SC_DEC | -00d03m32.1s (-0.05890°) |
| RADEC_ERR | 0.31 arcsec |
| LII / BII | 32.9005° / -0.0678° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 7 (observations covering the position) |
| MJD_FIRST | 52917.050 (2003-10-05 01:12:10.000 UTC) |
| MJD_LAST | 56005.114 (2012-03-19 02:43:28.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.17e-13 ± 9.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.87
± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
0.86
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.03
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.30
± 0.06
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 3.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 5.73
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.24e-13 (+1.3e-13 / −1.1e-13) erg cm−2 s−1 |
|---|---|
| NH | 9.50e+21 (+1.1e+22 / −8.2e+21) cm−2 |
| Photon index (Γ) | 1.87 (+2.03 / −1.72) |
| DoF | 1006 |
| p-value | 0.883 |
| Inter-instrument norm. | 1.02 (0.94–1.10) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 7.200 (approximate flux variability amplitude) |
|---|
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.