5XMM J020517.4+644851
5XMM-DR15 stacked source · SRCID 3000401010100049
Position:
02h05m17.43s +64d48m51.5s
(31.32262°, 64.81431°)
EP flux
4.24e-15
± 1.3e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.542)
Detections
12
| SRCID | 3000401010100049 |
|---|---|
| IAUNAME | 5XMM J020517.4+644851 |
| SC_RA | 02h05m17.43s (31.32262°) |
| SC_DEC | +64d48m51.5s (64.81431°) |
| RADEC_ERR | 2.45 arcsec |
| LII / BII | 130.6884° / 3.0606° |
| N_CONTRIB | 12 (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): 4.24e-15 ± 1.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.88
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.83
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.22
± 0.53
1.0-2.0 / 2.0-4.5 keV
HR4
-0.01
± 0.53
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 7.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.67
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
- 723751
- Match probability
- 0.573
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.770 | 0.052 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.92e-14 (+8.6e-14 / −7.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.45e+21 (+2.8e+21 / −2.0e+21) cm−2 |
| Photon index (Γ) | 2.88 (+2.97 / −2.74) |
| DoF | 240 |
| p-value | 0.113 |
| 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.