5XMM J230254.4+083903

5XMM-DR15 stacked source · SRCID 3003214020100004
Position: 23h02m54.46s +08d39m03.7s (345.72692°, 8.65102°)
EP flux
2.23e-13 ± 1.1e-14 erg cm-2 s-1
CLASSX
AGN (0.846)
Detections
7

SRCID 3003214020100004
IAUNAME 5XMM J230254.4+083903
SC_RA 23h02m54.46s (345.72692°)
SC_DEC +08d39m03.7s (8.65102°)
RADEC_ERR 0.14 arcsec
LII / BII 82.8129° / -45.5981°
N_CONTRIB 7 (detections)
N_OBS 13 (observations covering the position)
MJD_FIRST 52070.070 (2001-06-10 01:40:05.000 UTC)
MJD_LAST 57386.034 (2015-12-30 00:49:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.23e-13 ± 1.1e-14 erg cm-2 s-1

Hardness ratios
HR1
0.44 ± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.25 ± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31 ± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.48 ± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -4.0) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.434

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
6523125
Match probability
0.996
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 20.371 0.112
B
V

Spectroscopic (zsp) 0.43700
Photometric (TPZ) 0.4259 (conf 0.58)
Photometric (Le Phare) 0.3945 (conf 0.83)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Stacked power-law fit
Unabsorbed flux 2.46e-13 (+2.7e-13 / −2.2e-13) erg cm−2 s−1
NH 9.86e+20 (+1.3e+21 / −7.4e+20) cm−2
Photon index (Γ) 1.88 (+2.00 / −1.76)
DoF 946
p-value 0.961
Inter-instrument norm. 0.97 (0.90–1.04)
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

The per-observation light curve is shown in the X-ray properties section above.