5XMM J105151.6+573216
5XMM-DR15 stacked source · SRCID 3002274010100289
Position:
10h51m51.66s +57d32m16.9s
(162.96525°, 57.53803°)
EP flux
6.54e-15
± 2.1e-15
erg cm-2 s-1
CLASSX
Extended
(0.999)
Detections
16
| SRCID | 3002274010100289 |
|---|---|
| IAUNAME | 5XMM J105151.6+573216 |
| SC_RA | 10h51m51.66s (162.96525°) |
| SC_DEC | +57d32m16.9s (57.53803°) |
| RADEC_ERR | 1.58 arcsec |
| LII / BII | 149.3384° / 53.0222° |
| N_CONTRIB | 16 (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): 6.54e-15 ± 2.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.34
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.54
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.56
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
0.14
± 0.43
2.0-4.5 / 4.5-12.0 keV
Extent:
12.24
± 0.85
arcsec
(ML 78.2)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.62
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
- 2952550
- Match probability
- 0.732
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 22.015 | 0.114 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.52e-15 (+3.9e-15 / −1.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.15e+20 (+7.4e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 2.18 (+2.70 / −1.69) |
| DoF | 135 |
| p-value | 0.831 |
| 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.