5XMM J230502.1+030952

5XMM-DR15 stacked source · SRCID 3003354100100012
Position: 23h05m02.13s +03d09m52.1s (346.25886°, 3.16448°)
EP flux
3.45e-14 ± 6.7e-15 erg cm-2 s-1
CLASSX
AGN (0.915)
Detections
1

SRCID 3003354100100012
IAUNAME 5XMM J230502.1+030952
SC_RA 23h05m02.13s (346.25886°)
SC_DEC +03d09m52.1s (3.16448°)
RADEC_ERR 0.56 arcsec
LII / BII 78.5116° / -50.2998°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52242.909 (2001-11-29 21:49:15.000 UTC)
MJD_LAST 52243.055 (2001-11-30 01:18:42.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.45e-14 ± 6.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.17 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.04 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.73 ± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 0.963

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
6526622
Match probability
0.999
FilterMag (AB)Err
UVW2
UVM2
UVW1 21.082 0.221
U
B
V

Spectroscopic (zsp) 1.16800
Photometric (TPZ) 1.1757 (conf 0.75)
Photometric (Le Phare) 1.0240 (conf 0.85)

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

Stacked power-law fit
Unabsorbed flux 4.58e-14 (+5.9e-14 / −3.7e-14) erg cm−2 s−1
NH 1.16e+20 (+6.9e+20 / −2.4e+19) cm−2
Photon index (Γ) 1.88 (+2.19 / −1.64)
DoF 58
p-value 0.752
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.