5XMM J020717.5+645020
5XMM-DR15 stacked source · SRCID 3000401010100085
Position:
02h07m17.52s +64d50m20.5s
(31.82299°, 64.83902°)
EP flux
6.16e-15
± 3.3e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.327)
Detections
10
| SRCID | 3000401010100085 |
|---|---|
| IAUNAME | 5XMM J020717.5+645020 |
| SC_RA | 02h07m17.52s (31.82299°) |
| SC_DEC | +64d50m20.5s (64.83902°) |
| RADEC_ERR | 0.89 arcsec |
| LII / BII | 130.8856° / 3.1451° |
| N_CONTRIB | 10 (detections) |
| N_OBS | 12 (observations covering the position) |
| MJD_FIRST | 51614.582 (2000-03-11 13:58:36.000 UTC) |
| MJD_LAST | 52531.384 (2002-09-14 09:12:45.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.16e-15 ± 3.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.83
± 0.23
0.2-0.5 / 0.5-1.0 keV
HR2
0.27
± 0.21
0.5-1.0 / 1.0-2.0 keV
HR3
-0.67
± 0.23
1.0-2.0 / 2.0-4.5 keV
HR4
0.42
± 0.45
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 5.4
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
- 735408
- Match probability
- 0.516
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 18.520 | 0.117 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.47e-15 (+1.0e-14 / −3.9e-15) erg cm−2 s−1 |
|---|---|
| NH | 5.20e+20 (+1.8e+21 / −3.5e+19) cm−2 |
| Photon index (Γ) | 2.25 (+2.76 / −1.68) |
| DoF | 135 |
| p-value | 0.186 |
| 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.