5XMM J094021.9+711909
5XMM-DR15 stacked source · SRCID 3002634010100004
Position:
09h40m21.92s +71d19m09.8s
(145.09133°, 71.31939°)
EP flux
6.69e-14
± 8.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.897)
Detections
1
| SRCID | 3002634010100004 |
|---|---|
| IAUNAME | 5XMM J094021.9+711909 |
| SC_RA | 09h40m21.92s (145.09133°) |
| SC_DEC | +71d19m09.8s (71.31939°) |
| RADEC_ERR | 0.41 arcsec |
| LII / BII | 140.5910° / 38.5764° |
| 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): 6.69e-14 ± 8.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.17
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.02
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.33
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.60
± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.553
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
- 2759190
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.010 | 0.157 |
| U | 21.349 | 0.191 |
| B | 20.917 | 0.210 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.48e-14 (+7.7e-14 / −5.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.59e+19 (+3.9e+20 / −1.9e+19) cm−2 |
| Photon index (Γ) | 1.91 (+2.11 / −1.73) |
| DoF | 103 |
| p-value | 0.95 |
| 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.