5XMM J073031.2+854120
5XMM-DR15 stacked source · SRCID 3002234020100041
Position:
07h30m31.22s +85d41m20.3s
(112.63008°, 85.68896°)
EP flux
1.16e-14
± 1.7e-15
erg cm-2 s-1
CLASSX
AGN
(0.501)
Detections
1
| SRCID | 3002234020100041 |
|---|---|
| IAUNAME | 5XMM J073031.2+854120 |
| SC_RA | 07h30m31.22s (112.63008°) |
| SC_DEC | +85d41m20.3s (85.68896°) |
| RADEC_ERR | 0.74 arcsec |
| LII / BII | 127.7349° / 27.7780° |
| 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): 1.16e-14 ± 1.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.72
± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
0.04
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.20
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.89
± 0.09
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 2.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 2.29
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 | 1.15e-14 (+1.4e-14 / −9.2e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.03e+21 (+2.0e+21 / −1.7e+20) cm−2 |
| Photon index (Γ) | 1.67 (+2.00 / −1.37) |
| DoF | 221 |
| p-value | 0.432 |
| Inter-instrument norm. | 1.00 (0.76–1.31) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 13.400 (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.