5XMM J184444.3+005124
5XMM-DR15 stacked source · SRCID 3001774020100004
Position:
18h44m44.39s +00d51m24.5s
(281.18496°, 0.85681°)
EP flux
1.40e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
Star
(0.991)
Detections
3
| SRCID | 3001774020100004 |
|---|---|
| IAUNAME | 5XMM J184444.3+005124 |
| SC_RA | 18h44m44.39s (281.18496°) |
| SC_DEC | +00d51m24.5s (0.85681°) |
| RADEC_ERR | 0.55 arcsec |
| LII / BII | 32.9311° / 1.8809° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52921.032 (2003-10-09 00:45:48.000 UTC) |
| MJD_LAST | 52925.324 (2003-10-13 07:46:48.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.40e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.50
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.41
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.90
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
0.60
± 0.56
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.14
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
- 5630962
- Match probability
- 0.939
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 17.623 | 0.017 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.61e-14 (+1.9e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.05e+21 (+1.6e+21 / −2.9e+20) cm−2 |
| Photon index (Γ) | 2.70 (+2.93 / −2.35) |
| DoF | 83 |
| p-value | 0.434 |
| 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.