5XMM J103952.4+205048
5XMM-DR15 stacked source · SRCID 3005980010100012
Position:
10h39m52.47s +20d50m48.8s
(159.96861°, 20.84689°)
EP flux
4.87e-14
± 1.0e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.949)
Detections
1
| SRCID | 3005980010100012 |
|---|---|
| IAUNAME | 5XMM J103952.4+205048 |
| SC_RA | 10h39m52.47s (159.96861°) |
| SC_DEC | +20d50m48.8s (20.84689°) |
| RADEC_ERR | 0.96 arcsec |
| LII / BII | 217.5625° / 59.3926° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52245.743 (2001-12-02 17:50:38.000 UTC) |
| MJD_LAST | 52245.910 (2001-12-02 21:50:10.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.87e-14 ± 1.0e-14 erg cm-2 s-1
Hardness ratios
HR1
0.83
± 0.18
0.2-0.5 / 0.5-1.0 keV
HR2
0.22
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.16
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.32
± 0.19
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.41
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
- 2919690
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 18.376 | 0.030 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.96e-14 (+5.5e-14 / −2.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.73e+21 (+3.8e+21 / −1.8e+20) cm−2 |
| Photon index (Γ) | 1.40 (+1.96 / −1.12) |
| DoF | 60 |
| p-value | 0.613 |
| 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.