5XMM J230852.0-021148

5XMM-DR15 stacked source · SRCID 3004234120100001
Position: 23h08m52.07s -02d11m48.6s (347.21697°, -2.19682°)
EP flux
1.10e-12 ± 4.0e-14 erg cm-2 s-1
CLASSX
AGN (0.87)
Detections
2

SRCID 3004234120100001
IAUNAME 5XMM J230852.0-021148
SC_RA 23h08m52.07s (347.21697°)
SC_DEC -02d11m48.6s (-2.19682°)
RADEC_ERR 0.14 arcsec
LII / BII 73.9882° / -55.0072°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52070.285 (2001-06-10 06:49:52.000 UTC)
MJD_LAST 53161.188 (2004-06-05 04:30:57.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.10e-12 ± 4.0e-14 erg cm-2 s-1

Hardness ratios
HR1
0.19 ± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
-0.08 ± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.48 ± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.34 ± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -4.4) SUM_FLAG: 0
Long-term lightcurve

AGN

CLASSX outlier: 1.63

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
6530482
Match probability
1
FilterMag (AB)Err
UVW2 18.080 0.097
UVM2 18.505 0.091
UVW1 17.952 0.025
U — —
B — —
V — —

Photometric (TPZ) 0.1760 (conf 0.52)
Photometric (Le Phare) 0.1970 (conf 0.99)

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

Stacked power-law fit
Unabsorbed flux 7.50e-13 (+7.8e-13 / −7.2e-13) erg cm−2 s−1
NH 6.06e+20 (+7.5e+20 / −4.7e+20) cm−2
Photon index (Γ) 2.36 (+2.45 / −2.28)
DoF 714
p-value 0.676
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.