5XMM J063837.2+820912
5XMM-DR15 stacked source · SRCID 3002934010100061
Position:
06h38m37.20s +82d09m12.6s
(99.65499°, 82.15350°)
EP flux
8.99e-15
± 5.4e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.528)
Detections
2
| SRCID | 3002934010100061 |
|---|---|
| IAUNAME | 5XMM J063837.2+820912 |
| SC_RA | 06h38m37.20s (99.65499°) |
| SC_DEC | +82d09m12.6s (82.15350°) |
| RADEC_ERR | 1.07 arcsec |
| LII / BII | 131.6864° / 26.4184° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 51996.601 (2001-03-28 14:25:24.000 UTC) |
| MJD_LAST | 52918.225 (2003-10-06 05:23:32.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.99e-15 ± 5.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.70
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
-0.26
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.69
± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
0.75
± 0.27
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: 3.65
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
- 2267113
- Match probability
- 0.987
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.614 | 0.029 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.39e-15 (+9.9e-15 / −5.4e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.40e+20 (+1.8e+21 / −6.6e+19) cm−2 |
| Photon index (Γ) | 2.42 (+2.83 / −1.98) |
| DoF | 254 |
| p-value | 0.074 |
| 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.