5XMM J105340.1+572352
5XMM-DR15 stacked source · SRCID 3002274010100095
Position:
10h53m40.10s +57d23m52.4s
(163.41709°, 57.39789°)
EP flux
4.43e-15
± 9.6e-16
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.543)
Detections
16
| SRCID | 3002274010100095 |
|---|---|
| IAUNAME | 5XMM J105340.1+572352 |
| SC_RA | 10h53m40.10s (163.41709°) |
| SC_DEC | +57d23m52.4s (57.39789°) |
| RADEC_ERR | 0.31 arcsec |
| LII / BII | 149.2352° / 53.2958° |
| 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): 4.43e-15 ± 9.6e-16 erg cm-2 s-1
Hardness ratios
HR1
0.71
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.86
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.74
± 0.19
1.0-2.0 / 2.0-4.5 keV
HR4
0.53
± 0.47
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 60.6)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.8
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
- 2961983
- Match probability
- 0.792
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.696 | 0.181 |
| U | 21.701 | 0.072 |
| B | 20.123 | 0.033 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.32e-15 (+8.6e-15 / −3.8e-15) erg cm−2 s−1 |
|---|---|
| NH | 8.74e+19 (+4.0e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 2.35 (+2.79 / −1.77) |
| DoF | 162 |
| p-value | 0.092 |
| 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.