5XMM J115050.9+550834
5XMM-DR15 stacked source · SRCID 3004934030100037
Position:
11h50m50.91s +55d08m34.8s
(177.71213°, 55.14300°)
EP flux
1.71e-14
± 4.3e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.776)
Detections
1
| SRCID | 3004934030100037 |
|---|---|
| IAUNAME | 5XMM J115050.9+550834 |
| SC_RA | 11h50m50.91s (177.71213°) |
| SC_DEC | +55d08m34.8s (55.14300°) |
| RADEC_ERR | 1.19 arcsec |
| LII / BII | 140.2567° / 59.9004° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52391.391 (2002-04-27 09:23:11.000 UTC) |
| MJD_LAST | 52391.692 (2002-04-27 16:37:00.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.71e-14 ± 4.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.47
± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
-0.25
± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.21
± 0.19
1.0-2.0 / 2.0-4.5 keV
HR4
-0.30
± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.02
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
- 3101180
- Match probability
- 0.994
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 16.869 | 0.021 |
| U | 16.283 | 0.014 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.02e-14 (+1.4e-14 / −7.6e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.31e+20 (+9.5e+20 / −3.1e+19) cm−2 |
| Photon index (Γ) | 1.93 (+2.37 / −1.66) |
| DoF | 64 |
| p-value | 0.914 |
| 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.