5XMM J022208.4-040542

5XMM-DR15 stacked source · SRCID 3003798220111692
Position: 02h22m08.41s -04d05m42.6s (35.53505°, -4.09517°)
EP flux
1.31e-15 ± 1.7e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.642)
Detections
6

SRCID 3003798220111692
IAUNAME 5XMM J022208.4-040542
SC_RA 02h22m08.41s (35.53505°)
SC_DEC -04d05m42.6s (-4.09517°)
RADEC_ERR 1.80 arcsec
LII / BII 170.1296° / -58.3928°
N_CONTRIB 6 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52667.803 (2003-01-28 19:16:33.000 UTC)
MJD_LAST 57758.217 (2017-01-05 05:11:54.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.31e-15 ± 1.7e-15 erg cm-2 s-1

Hardness ratios
HR1
-0.31 ± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
-0.36 ± 0.33
0.5-1.0 / 1.0-2.0 keV
HR3
-0.68 ± 0.62
1.0-2.0 / 2.0-4.5 keV
HR4
-0.74 ± 6.30
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.0) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.54

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
792372
Match probability
0.946
FilterMag (AB)Err
UVW2 — —
UVM2 21.163 0.232
UVW1 20.908 0.039
U — —
B — —
V — —
AllWISE
Name
J022208.32-040546.4
Match probability
0.993
BandMagErr
W1 15.124 0.034
W2 14.782 0.059
W3 11.209 0.130
W4 8.516 0.246
CLASSOPT
Class
Galaxy
Star
0.02
AGN
0.09
Galaxy
0.90

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.