5XMM J105128.0+573503
5XMM-DR15 stacked source · SRCID 3002274010100058
Position:
10h51m28.03s +57d35m03.5s
(162.86679°, 57.58432°)
EP flux
8.21e-15
± 1.4e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.939)
Detections
15
| SRCID | 3002274010100058 |
|---|---|
| IAUNAME | 5XMM J105128.0+573503 |
| SC_RA | 10h51m28.03s (162.86679°) |
| SC_DEC | +57d35m03.5s (57.58432°) |
| RADEC_ERR | 0.33 arcsec |
| LII / BII | 149.3409° / 52.9520° |
| N_CONTRIB | 15 (detections) |
| N_OBS | 21 (observations covering the position) |
| MJD_FIRST | 51661.158 (2000-04-27 03:47:47.000 UTC) |
| MJD_LAST | 52615.196 (2002-12-07 04:41:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.21e-15 ± 1.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.34
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.02
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.67
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
0.15
± 0.19
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.81
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
- 2949972
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 19.213 | 0.030 |
| UVM2 | 19.027 | 0.020 |
| UVW1 | 18.815 | 0.013 |
| U | 18.616 | 0.009 |
| B | 17.778 | 0.008 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.16e-14 (+1.4e-14 / −9.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 3.64e+20 (+1.1e+21 / −4.0e+19) cm−2 |
| Photon index (Γ) | 2.18 (+2.62 / −1.93) |
| DoF | 286 |
| p-value | 0.979 |
| Inter-instrument norm. | 1.02 (0.83–1.24) |
| 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.