5XMM J063909.6+821453
5XMM-DR15 stacked source · SRCID 3002934010100025
Position:
06h39m09.69s +82d14m53.2s
(99.79039°, 82.24811°)
EP flux
2.23e-14
± 4.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.918)
Detections
2
| SRCID | 3002934010100025 |
|---|---|
| IAUNAME | 5XMM J063909.6+821453 |
| SC_RA | 06h39m09.69s (99.79039°) |
| SC_DEC | +82d14m53.2s (82.24811°) |
| RADEC_ERR | 0.45 arcsec |
| LII / BII | 131.5841° / 26.4483° |
| 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): 2.23e-14 ± 4.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.22
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.19
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.46
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.30
± 0.28
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.625
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
- 2268358
- Match probability
- 0.996
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.431 | 0.093 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.58e-14 (+1.9e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.22e+20 (+5.0e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 2.10 (+2.36 / −1.91) |
| DoF | 354 |
| p-value | 0.234 |
| 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.