5XMM J230220.2+082954

5XMM-DR15 stacked source · SRCID 3003214020100051
Position: 23h02m20.29s +08d29m54.0s (345.58455°, 8.49832°)
EP flux
1.01e-13 ± 2.2e-14 erg cm-2 s-1
CLASSX
AGN (0.863)
Detections
1

SRCID 3003214020100051
IAUNAME 5XMM J230220.2+082954
SC_RA 23h02m20.29s (345.58455°)
SC_DEC +08d29m54.0s (8.49832°)
RADEC_ERR 0.81 arcsec
LII / BII 82.5222° / -45.6404°
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): 1.01e-13 ± 2.2e-14 erg cm-2 s-1

Hardness ratios
HR1
0.27 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
-0.14 ± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.35 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.22 ± 0.22
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.4) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.536

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
6521903
Match probability
0.986
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 20.916 0.073
B
V

Photometric (TPZ) 0.4259 (conf 0.69)
Photometric (Le Phare) 0.4468 (conf 1.00)

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

Stacked power-law fit
Unabsorbed flux 8.73e-14 (+1.1e-13 / −7.1e-14) erg cm−2 s−1
NH 1.06e+20 (+5.3e+20 / −2.3e+19) cm−2
Photon index (Γ) 1.72 (+1.96 / −1.52)
DoF 375
p-value 0.397
Inter-instrument norm. 1.22 (0.97–1.52)
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.