5XMM J064031.2+822344
5XMM-DR15 stacked source · SRCID 3002934010100039
Position:
06h40m31.22s +82d23m44.6s
(100.13006°, 82.39572°)
EP flux
2.80e-14
± 7.3e-15
erg cm-2 s-1
CLASSX
AGN
(0.899)
Detections
2
| SRCID | 3002934010100039 |
|---|---|
| IAUNAME | 5XMM J064031.2+822344 |
| SC_RA | 06h40m31.22s (100.13006°) |
| SC_DEC | +82d23m44.6s (82.39572°) |
| RADEC_ERR | 0.71 arcsec |
| LII / BII | 131.4263° / 26.5107° |
| 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): 2.80e-14 ± 7.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.34
± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
0.09
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.13
± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.141
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
- 2272824
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.936 | 0.074 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.95e-14 (+2.5e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.45e+20 (+8.8e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.43 (+1.76 / −1.18) |
| DoF | 80 |
| p-value | 0.601 |
| 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.