5XMM J230240.2+083611

5XMM-DR15 stacked source · SRCID 3003214020100019
Position: 23h02m40.27s +08d36m11.6s (345.66778°, 8.60322°)
EP flux
1.58e-13 ± 1.4e-14 erg cm-2 s-1
CLASSX
AGN (0.897)
Detections
1

SRCID 3003214020100019
IAUNAME 5XMM J230240.2+083611
SC_RA 23h02m40.27s (345.66778°)
SC_DEC +08d36m11.6s (8.60322°)
RADEC_ERR 0.36 arcsec
LII / BII 82.7052° / -45.6031°
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): 1.58e-13 ± 1.4e-14 erg cm-2 s-1

Hardness ratios
HR1
0.40 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.17 ± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.30 ± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.54 ± 0.09
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.1) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 1.39

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
6522688
Match probability
0.983
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 21.343 0.146
B
V

Spectroscopic (zsp) 1.95700
Photometric (TPZ) 1.7255 (conf 0.46)
Photometric (Le Phare) 1.5440 (conf 0.93)

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

Stacked power-law fit
Unabsorbed flux 1.37e-13 (+1.6e-13 / −1.2e-13) erg cm−2 s−1
NH 2.07e+20 (+6.9e+20 / −3.5e+19) cm−2
Photon index (Γ) 1.60 (+1.80 / −1.47)
DoF 611
p-value 0.826
Inter-instrument norm. 1.19 (1.04–1.33)
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.