5XMM J065214.3+743229
5XMM-DR15 stacked source · SRCID 3006154010100002
Position:
06h52m14.36s +74d32m29.4s
(103.05982°, 74.54151°)
EP flux
3.22e-13
± 1.8e-14
erg cm-2 s-1
CLASSX
AGN
(0.904)
Detections
3
| SRCID | 3006154010100002 |
|---|---|
| IAUNAME | 5XMM J065214.3+743229 |
| SC_RA | 06h52m14.36s (103.05982°) |
| SC_DEC | +74d32m29.4s (74.54151°) |
| RADEC_ERR | 0.19 arcsec |
| LII / BII | 140.2014° / 26.1241° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 51995.780 (2001-03-27 18:43:49.000 UTC) |
| MJD_LAST | 53670.272 (2005-10-27 06:32:00.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.22e-13 ± 1.8e-14 erg cm-2 s-1
Hardness ratios
HR1
0.43
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.18
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.28
± 0.06
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.69
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
- 2289291
- Match probability
- 0.988
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 21.018 | 0.259 |
| UVM2 | — | — |
| UVW1 | 20.884 | 0.116 |
| U | 20.852 | 0.138 |
| B | 20.016 | 0.106 |
| V | 19.935 | 0.214 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.44e-13 (+2.6e-13 / −2.2e-13) erg cm−2 s−1 |
|---|---|
| NH | 8.59e+20 (+1.2e+21 / −6.1e+20) cm−2 |
| Photon index (Γ) | 1.91 (+2.06 / −1.78) |
| DoF | 746 |
| p-value | 0.656 |
| 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.