5XMM J020717.9+022043
5XMM-DR15 stacked source · SRCID 3005214030100015
Position:
02h07m17.90s +02d20m43.6s
(31.82460°, 2.34544°)
EP flux
3.20e-14
± 6.3e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
2
| SRCID | 3005214030100015 |
|---|---|
| IAUNAME | 5XMM J020717.9+022043 |
| SC_RA | 02h07m17.90s (31.82460°) |
| SC_DEC | +02d20m43.6s (2.34544°) |
| RADEC_ERR | 0.48 arcsec |
| LII / BII | 157.7273° / -55.3168° |
| 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): 3.20e-14 ± 6.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.53
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.62
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.92
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
0.14
± 0.79
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.66
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.29e-14 (+4.7e-14 / −3.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.53e+20 (+1.1e+21 / −5.5e+20) cm−2 |
| Photon index (Γ) | 2.90 (+2.98 / −2.75) |
| DoF | 251 |
| p-value | 0.012 |
| Inter-instrument norm. | 0.52 (0.51–0.56) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.200 (approximate flux variability amplitude) |
|---|
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.