5XMM J185146.2+000258
5XMM-DR15 stacked source · SRCID 3001774040100061
Position:
18h51m46.28s +00d02m58.2s
(282.94282°, 0.04950°)
EP flux
9.74e-14
± 1.6e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
3
| SRCID | 3001774040100061 |
|---|---|
| IAUNAME | 5XMM J185146.2+000258 |
| SC_RA | 18h51m46.28s (282.94282°) |
| SC_DEC | +00d02m58.2s (0.04950°) |
| RADEC_ERR | 2.15 arcsec |
| LII / BII | 33.0140° / -0.0516° |
| 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): 9.74e-14 ± 1.6e-14 erg cm-2 s-1
Hardness ratios
HR1
0.66
± 0.42
0.2-0.5 / 0.5-1.0 keV
HR2
0.94
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
0.25
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.48
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
16.17
± 1.22
arcsec
(ML 99.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.79
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
- 5681656
- Match probability
- 0.677
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.701 | 0.081 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.58e-14 (+2.4e-14 / −9.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.86e+22 (+1.1e+24 / −4.8e+21) cm−2 |
| Photon index (Γ) | 1.54 (+2.33 / −1.12) |
| DoF | 60 |
| p-value | 0.321 |
| 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.