5XMM J022344.6-035808

5XMM-DR15 stacked source · SRCID 3003798020101785
Position: 02h23m44.66s -03d58m08.8s (35.93609°, -3.96911°)
EP flux
3.15e-14 ± 6.7e-15 erg cm-2 s-1
CLASSX
AGN (0.937)
Detections
3

SRCID 3003798020101785
IAUNAME 5XMM J022344.6-035808
SC_RA 02h23m44.66s (35.93609°)
SC_DEC -03d58m08.8s (-3.96911°)
RADEC_ERR 0.64 arcsec
LII / BII 170.5451° / -58.0350°
N_CONTRIB 3 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52285.602 (2002-01-11 14:26:33.000 UTC)
MJD_LAST 53373.039 (2005-01-03 00:56:27.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.15e-14 ± 6.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.69 ± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
0.27 ± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.28 ± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.35 ± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.3) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 0.13

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
803976
Match probability
0.89
FilterMag (AB)Err
UVW2
UVM2
UVW1 22.010 0.195
U
B
V

Spectroscopic (zsp) 1.07100
Photometric (TPZ) 1.0757 (conf 0.53)
Photometric (Le Phare) 1.2730 (conf 0.97)

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

Stacked power-law fit
Unabsorbed flux 1.23e-14 (+2.2e-14 / −5.4e-15) erg cm−2 s−1
NH 5.58e+20 (+5.0e+21 / −4.1e+19) cm−2
Photon index (Γ) 1.75 (+2.50 / −1.22)
DoF 109
p-value 0.762
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.