5XMM J064159.8+821537
5XMM-DR15 stacked source · SRCID 3002934010100004
Position:
06h41m59.87s +82d15m37.4s
(100.49944°, 82.26038°)
EP flux
4.13e-14
± 3.0e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.543)
Detections
2
| SRCID | 3002934010100004 |
|---|---|
| IAUNAME | 5XMM J064159.8+821537 |
| SC_RA | 06h41m59.87s (100.49944°) |
| SC_DEC | +82d15m37.4s (82.26038°) |
| RADEC_ERR | 0.40 arcsec |
| LII / BII | 131.5828° / 26.5446° |
| 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): 4.13e-14 ± 3.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.25
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.57
± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 26.0)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.58
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
- 2274551
- Match probability
- 0.996
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.878 | 0.050 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.34e-14 (+4.9e-14 / −3.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.40e+20 (+1.4e+21 / −8.2e+19) cm−2 |
| Photon index (Γ) | 2.06 (+2.38 / −1.81) |
| DoF | 221 |
| p-value | 0.977 |
| 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.