5XMM J065331.0+742257
5XMM-DR15 stacked source · SRCID 3006154010100034
Position:
06h53m31.06s +74d22m57.3s
(103.37942°, 74.38258°)
EP flux
1.08e-14
± 4.2e-15
erg cm-2 s-1
CLASSX
AGN
(0.919)
Detections
3
| SRCID | 3006154010100034 |
|---|---|
| IAUNAME | 5XMM J065331.0+742257 |
| SC_RA | 06h53m31.06s (103.37942°) |
| SC_DEC | +74d22m57.3s (74.38258°) |
| RADEC_ERR | 0.82 arcsec |
| LII / BII | 140.3893° / 26.1884° |
| 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): 1.08e-14 ± 4.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.49
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.27
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.62
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.01
± 0.36
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.9)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.506
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
- 2290538
- Match probability
- 0.987
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 20.851 | 0.205 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.48e-15 (+1.0e-14 / −4.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.18e+20 (+1.0e+21 / −3.0e+19) cm−2 |
| Photon index (Γ) | 1.97 (+2.49 / −1.52) |
| DoF | 234 |
| p-value | 0.54 |
| 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.