5XMM J022052.8-045811

5XMM-DR15 stacked source · SRCID 3003798200106852
Position: 02h20m52.84s -04d58m11.0s (35.22015°, -4.96973°)
EP flux
4.20e-15 ± 1.7e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.94)
Detections
5

SRCID 3003798200106852
IAUNAME 5XMM J022052.8-045811
SC_RA 02h20m52.84s (35.22015°)
SC_DEC -04d58m11.0s (-4.96973°)
RADEC_ERR 1.19 arcsec
LII / BII 170.7858° / -59.2577°
N_CONTRIB 5 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52500.578 (2002-08-14 13:52:48.000 UTC)
MJD_LAST 57770.061 (2017-01-17 01:28:18.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.20e-15 ± 1.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.46 ± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
-0.09 ± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.66 ± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.72 ± 0.82
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.6) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.43

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
783952
Match probability
0.995
FilterMag (AB)Err
UVW2 20.144 0.128
UVM2 20.186 0.081
UVW1 19.173 0.017
U — —
B — —
V — —
Gaia DR3
Source ID
2489499113621115520
Match probability
0.989
Magnitudes
G=19.72, BP=18.55, RP=17.14
AllWISE
Name
J022052.91-045809.2
Match probability
0.995
BandMagErr
W1 13.575 0.036
W2 13.264 0.042
W3 9.097 0.040
W4 6.382 0.093
CLASSOPT
Class
Galaxy
Star
0.00
AGN
0.01
Galaxy
0.99

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.