5XMM J230257.1+083152

5XMM-DR15 stacked source · SRCID 3003214020100086
Position: 23h02m57.13s +08d31m52.5s (345.73806°, 8.53126°)
EP flux
1.04e-13 ± 2.7e-14 erg cm-2 s-1
CLASSX
AGN (0.95)
Detections
1

SRCID 3003214020100086
IAUNAME 5XMM J230257.1+083152
SC_RA 23h02m57.13s (345.73806°)
SC_DEC +08d31m52.5s (8.53126°)
RADEC_ERR 0.99 arcsec
LII / BII 82.7263° / -45.7020°
N_CONTRIB 1 (detections)
N_OBS 13 (observations covering the position)
MJD_FIRST 52070.070 (2001-06-10 01:40:05.000 UTC)
MJD_LAST 52070.214 (2001-06-10 05:08:43.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.04e-13 ± 2.7e-14 erg cm-2 s-1

Hardness ratios
HR1
0.48 ± 0.29
0.2-0.5 / 0.5-1.0 keV
HR2
0.68 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.08 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
0.09 ± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.0) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.0902

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
6523198
Match probability
0.991
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 22.248 0.307
B
V

Photometric (TPZ) 1.0257 (conf 0.68)
Photometric (Le Phare) 1.0430 (conf 0.82)

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

Stacked power-law fit
Unabsorbed flux 7.28e-14 (+9.4e-14 / −5.3e-14) erg cm−2 s−1
NH 1.71e+21 (+4.6e+21 / −1.8e+20) cm−2
Photon index (Γ) 1.16 (+1.45 / −1.04)
DoF 230
p-value 0.462
Inter-instrument norm. 1.02 (0.71–1.43)
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.