5XMM J065230.7+742303
5XMM-DR15 stacked source · SRCID 3006154010100046
Position:
06h52m30.71s +74d23m03.7s
(103.12794°, 74.38435°)
EP flux
2.90e-15
± 1.7e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.818)
Detections
3
| SRCID | 3006154010100046 |
|---|---|
| IAUNAME | 5XMM J065230.7+742303 |
| SC_RA | 06h52m30.71s (103.12794°) |
| SC_DEC | +74d23m03.7s (74.38435°) |
| RADEC_ERR | 1.20 arcsec |
| LII / BII | 140.3776° / 26.1215° |
| 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): 2.90e-15 ± 1.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.28
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
-0.38
± 0.21
0.5-1.0 / 1.0-2.0 keV
HR3
-0.81
± 0.34
1.0-2.0 / 2.0-4.5 keV
HR4
-0.14
± 0.82
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 3.48
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
- 2289916
- Match probability
- 0.969
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 21.112 | 0.246 |
| V | 19.443 | 0.147 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.90e-15 (+1.1e-14 / −5.8e-15) erg cm−2 s−1 |
|---|---|
| NH | 7.97e+20 (+1.7e+21 / −6.0e+19) cm−2 |
| Photon index (Γ) | 2.35 (+2.81 / −1.82) |
| DoF | 268 |
| p-value | 0.514 |
| 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.