5XMM J023119.5-441922

5XMM-DR15 stacked source · SRCID 3004234030100171
Position: 02h31m19.51s -44d19m22.8s (37.83128°, -44.32299°)
EP flux
1.15e-14 ± 6.1e-15 erg cm-2 s-1
CLASSX
AGN (0.691)
Detections
2

SRCID 3004234030100171
IAUNAME 5XMM J023119.5-441922
SC_RA 02h31m19.51s (37.83128°)
SC_DEC -44d19m22.8s (-44.32299°)
RADEC_ERR 1.32 arcsec
LII / BII 260.1281° / -63.6092°
N_CONTRIB 2 (detections)
N_OBS 6 (observations covering the position)
MJD_FIRST 52466.430 (2002-07-11 10:18:36.000 UTC)
MJD_LAST 59215.542 (2021-01-01 13:00:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.15e-14 ± 6.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.57 ± 0.21
0.2-0.5 / 0.5-1.0 keV
HR2
0.16 ± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29 ± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.69 ± 0.47
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.6) 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
835999
Match probability
0.992
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 21.875 0.211
U — —
B — —
V — —
AllWISE
Name
J023119.52-441924.0
Match probability
0.993
BandMagErr
W1 15.151 0.031
W2 14.661 0.045
W3 11.400 0.112
W4 8.818 0.284
CLASSOPT
Class
Galaxy
Star
0.01
AGN
0.37
Galaxy
0.62

No redshift estimate available for this source.

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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.