5XMM J105003.6+325534
5XMM-DR15 stacked source · SRCID 3005599020100018
Position:
10h50m03.69s +32d55m34.4s
(162.51536°, 32.92622°)
EP flux
4.15e-14
± 4.5e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.425)
Detections
1
| SRCID | 3005599020100018 |
|---|---|
| IAUNAME | 5XMM J105003.6+325534 |
| SC_RA | 10h50m03.69s (162.51536°) |
| SC_DEC | +32d55m34.4s (32.92622°) |
| RADEC_ERR | 0.41 arcsec |
| LII / BII | 193.0377° / 63.1950° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52226.012 (2001-11-13 00:17:04.000 UTC) |
| MJD_LAST | 52226.450 (2001-11-13 10:48:00.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.15e-14 ± 4.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.56
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.27
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.73
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.98
± 0.31
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 3.97
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
- 2942214
- Match probability
- 0.989
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.909 | 0.261 |
| U | 20.855 | 0.120 |
| B | — | — |
| V | 17.021 | 0.033 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.64e-14 (+5.4e-14 / −4.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.53e+20 (+1.5e+21 / −1.5e+20) cm−2 |
| Photon index (Γ) | 2.62 (+2.89 / −2.22) |
| DoF | 453 |
| p-value | 0.31 |
| 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.