5XMM J020730.7+021030
5XMM-DR15 stacked source · SRCID 3005214030100145
Position:
02h07m30.74s +02d10m30.3s
(31.87807°, 2.17509°)
EP flux
1.55e-15
± 1.6e-15
erg cm-2 s-1
CLASSX
Star
(0.455)
Detections
2
| SRCID | 3005214030100145 |
|---|---|
| IAUNAME | 5XMM J020730.7+021030 |
| SC_RA | 02h07m30.74s (31.87807°) |
| SC_DEC | +02d10m30.3s (2.17509°) |
| RADEC_ERR | 2.07 arcsec |
| LII / BII | 157.9610° / -55.4361° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52284.757 (2002-01-10 18:09:23.000 UTC) |
| MJD_LAST | 56877.491 (2014-08-08 11:46:56.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.55e-15 ± 1.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.41
± 0.28
0.2-0.5 / 0.5-1.0 keV
HR2
-0.29
± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.95
± 0.23
1.0-2.0 / 2.0-4.5 keV
HR4
0.51
± 0.77
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 0.7
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
- 736540
- Match probability
- 0.812
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 21.184 | 0.336 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.76e-15 (+2.7e-15 / −1.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 7.56e+19 (+4.0e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 2.66 (+2.91 / −2.19) |
| DoF | 103 |
| p-value | 0.223 |
| 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.