5XMM J105126.1+572206
5XMM-DR15 stacked source · SRCID 3002274010100253
Position:
10h51m26.12s +57d22m06.7s
(162.85883°, 57.36852°)
EP flux
2.10e-15
± 8.6e-16
erg cm-2 s-1
CLASSX
Star
(0.881)
Detections
15
| SRCID | 3002274010100253 |
|---|---|
| IAUNAME | 5XMM J105126.1+572206 |
| SC_RA | 10h51m26.12s (162.85883°) |
| SC_DEC | +57d22m06.7s (57.36852°) |
| RADEC_ERR | 0.69 arcsec |
| LII / BII | 149.6111° / 53.0941° |
| 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): 2.10e-15 ± 8.6e-16 erg cm-2 s-1
Hardness ratios
HR1
0.77
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.46
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.25
± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
-0.59
± 0.53
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.38
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
- 2949748
- Match probability
- 0.979
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 23.134 | 0.346 |
| B | 19.810 | 0.028 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.88e-15 (+4.1e-15 / −2.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.98e+19 (+2.6e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.72 (+2.92 / −2.39) |
| DoF | 280 |
| p-value | 0.617 |
| 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.