5XMM J065305.0+741838
5XMM-DR15 stacked source · SRCID 3006154010100018
Position:
06h53m05.07s +74d18m38.0s
(103.27113°, 74.31056°)
EP flux
9.41e-15
± 3.3e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
3
| SRCID | 3006154010100018 |
|---|---|
| IAUNAME | 5XMM J065305.0+741838 |
| SC_RA | 06h53m05.07s (103.27113°) |
| SC_DEC | +74d18m38.0s (74.31056°) |
| RADEC_ERR | 0.64 arcsec |
| LII / BII | 140.4647° / 26.1501° |
| 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): 9.41e-15 ± 3.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.71
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.58
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.53
± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
-0.86
± 0.83
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.15
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
- 2290300
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 16.757 | 0.024 |
| UVM2 | — | — |
| UVW1 | 13.655 | 0.004 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.13e-14 (+1.3e-14 / −9.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.02e+21 (+1.5e+21 / −4.5e+20) cm−2 |
| Photon index (Γ) | 2.78 (+2.94 / −2.44) |
| DoF | 314 |
| p-value | 0.085 |
| Inter-instrument norm. | 1.58 (1.28–1.86) |
| 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.