5XMM J105244.0+571723
5XMM-DR15 stacked source · SRCID 3002274010100292
Position:
10h52m44.06s +57d17m23.7s
(163.18359°, 57.28991°)
EP flux
1.41e-14
± 3.6e-15
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
14
| SRCID | 3002274010100292 |
|---|---|
| IAUNAME | 5XMM J105244.0+571723 |
| SC_RA | 10h52m44.06s (163.18359°) |
| SC_DEC | +57d17m23.7s (57.28991°) |
| RADEC_ERR | 1.48 arcsec |
| LII / BII | 149.5109° / 53.2766° |
| N_CONTRIB | 14 (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): 1.41e-14 ± 3.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.47
± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.30
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.25
± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent:
8.29
± 0.63
arcsec
(ML 18.6)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.29
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
- 2958131
- Match probability
- 0.959
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.353 | 0.184 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.36e-15 (+1.0e-14 / −4.8e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.11e+20 (+2.3e+21 / −4.5e+19) cm−2 |
| Photon index (Γ) | 1.80 (+2.45 / −1.38) |
| DoF | 152 |
| p-value | 0.856 |
| 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.