5XMM J094130.1+711235
5XMM-DR15 stacked source · SRCID 3002634010100001
Position:
09h41m30.17s +71d12m35.1s
(145.37572°, 71.20974°)
EP flux
4.29e-13
± 2.3e-14
erg cm-2 s-1
CLASSX
AGN
(0.893)
Detections
1
| SRCID | 3002634010100001 |
|---|---|
| IAUNAME | 5XMM J094130.1+711235 |
| SC_RA | 09h41m30.17s (145.37572°) |
| SC_DEC | +71d12m35.1s (71.20974°) |
| RADEC_ERR | 0.20 arcsec |
| LII / BII | 140.6461° / 38.7125° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52352.952 (2002-03-19 22:50:54.000 UTC) |
| MJD_LAST | 52353.253 (2002-03-20 06:04:41.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.29e-13 ± 2.3e-14 erg cm-2 s-1
Hardness ratios
HR1
0.15
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.44
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.31
± 0.06
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -4.0)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.83
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
- 2760780
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.625 | 0.149 |
| U | 20.097 | 0.117 |
| B | 19.833 | 0.090 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.86e-13 (+3.0e-13 / −2.7e-13) erg cm−2 s−1 |
|---|---|
| NH | 3.55e+19 (+9.8e+19 / −1.5e+19) cm−2 |
| Photon index (Γ) | 1.97 (+2.04 / −1.90) |
| DoF | 401 |
| p-value | 0.414 |
| 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.