5XMM J105120.5+572701
5XMM-DR15 stacked source · SRCID 3002274010100068
Position:
10h51m20.53s +57d27m01.3s
(162.83555°, 57.45035°)
EP flux
1.14e-14
± 1.2e-15
erg cm-2 s-1
CLASSX
AGN
(0.777)
Detections
16
| SRCID | 3002274010100068 |
|---|---|
| IAUNAME | 5XMM J105120.5+572701 |
| SC_RA | 10h51m20.53s (162.83555°) |
| SC_DEC | +57d27m01.3s (57.45035°) |
| RADEC_ERR | 0.25 arcsec |
| LII / BII | 149.5242° / 53.0298° |
| 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): 1.14e-14 ± 1.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.14
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.04
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.42
± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.281
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
- 2949066
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.856 | 0.251 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.30e-14 (+1.6e-14 / −9.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 9.01e+19 (+5.0e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 1.73 (+2.06 / −1.46) |
| DoF | 121 |
| p-value | 0.855 |
| 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.