5XMM J105337.1+573257
5XMM-DR15 stacked source · SRCID 3002274010100197
Position:
10h53m37.16s +57d32m57.4s
(163.40482°, 57.54929°)
EP flux
2.26e-15
± 8.8e-16
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.623)
Detections
15
| SRCID | 3002274010100197 |
|---|---|
| IAUNAME | 5XMM J105337.1+573257 |
| SC_RA | 10h53m37.16s (163.40482°) |
| SC_DEC | +57d32m57.4s (57.54929°) |
| RADEC_ERR | 1.45 arcsec |
| LII / BII | 149.0577° / 53.1877° |
| 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): 2.26e-15 ± 8.8e-16 erg cm-2 s-1
Hardness ratios
HR1
0.45
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
-0.23
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.53
± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
0.21
± 0.40
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 28.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.58
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
- 2961859
- Match probability
- 0.598
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 22.684 | 0.379 |
| UVW1 | 22.037 | 0.230 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.12e-15 (+3.4e-15 / −1.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.05e+20 (+1.1e+21 / −2.5e+19) cm−2 |
| Photon index (Γ) | 2.25 (+2.74 / −1.75) |
| DoF | 368 |
| p-value | 0.232 |
| 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.