5XMM J230246.0+084522

5XMM-DR15 stacked source · SRCID 3003214020100002
Position: 23h02m46.07s +08d45m22.4s (345.69197°, 8.75623°)
EP flux
1.96e-13 ± 6.1e-15 erg cm-2 s-1
CLASSX
AGN (0.892)
Detections
13

SRCID 3003214020100002
IAUNAME 5XMM J230246.0+084522
SC_RA 23h02m46.07s (345.69197°)
SC_DEC +08d45m22.4s (8.75623°)
RADEC_ERR 0.09 arcsec
LII / BII 82.8598° / -45.4924°
N_CONTRIB 13 (detections)
N_OBS 13 (observations covering the position)
MJD_FIRST 51904.163 (2000-12-26 03:54:08.000 UTC)
MJD_LAST 59361.725 (2021-05-27 17:24:00.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.96e-13 ± 6.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.59 ± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
0.38 ± 0.01
0.5-1.0 / 1.0-2.0 keV
HR3
-0.26 ± 0.01
1.0-2.0 / 2.0-4.5 keV
HR4
-0.34 ± 0.03
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -4.4) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.815

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
6522894
Match probability
0.993
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 19.279 0.047
B
V

Spectroscopic (zsp) 1.94400
Photometric (TPZ) 1.9255 (conf 0.93)
Photometric (Le Phare) 1.9070 (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 1.46e-13 (+1.6e-13 / −1.3e-13) erg cm−2 s−1
NH 1.35e+21 (+1.8e+21 / −9.3e+20) cm−2
Photon index (Γ) 1.82 (+1.98 / −1.68)
DoF 463
p-value 0.7
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.