5XMM J073956.7+854020
5XMM-DR15 stacked source · SRCID 3002234020100006
Position:
07h39m56.74s +85d40m20.2s
(114.98640°, 85.67229°)
EP flux
1.14e-13
± 1.1e-14
erg cm-2 s-1
CLASSX
AGN
(0.876)
Detections
1
| SRCID | 3002234020100006 |
|---|---|
| IAUNAME | 5XMM J073956.7+854020 |
| SC_RA | 07h39m56.74s (114.98640°) |
| SC_DEC | +85d40m20.2s (85.67229°) |
| RADEC_ERR | 0.33 arcsec |
| LII / BII | 127.7230° / 27.9559° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 51984.216 (2001-03-16 05:10:27.000 UTC) |
| MJD_LAST | 51984.843 (2001-03-16 20:13:43.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.14e-13 ± 1.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.29
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.17
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.25
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.31
± 0.09
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.31
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.74e-14 (+9.5e-14 / −8.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.48e+20 (+8.5e+20 / −2.1e+20) cm−2 |
| Photon index (Γ) | 1.65 (+1.77 / −1.51) |
| DoF | 577 |
| p-value | 0.711 |
| Inter-instrument norm. | 0.96 (0.87–1.05) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.900 (approximate flux variability amplitude) |
|---|
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.