5XMM J022002.8-042542

5XMM-DR15 stacked source · SRCID 3003798230108795
Position: 02h20m02.83s -04d25m42.0s (35.01179°, -4.42834°)
EP flux
5.59e-15 ± 2.1e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.573)
Detections
5

SRCID 3003798230108795
IAUNAME 5XMM J022002.8-042542
SC_RA 02h20m02.83s (35.01179°)
SC_DEC -04d25m42.0s (-4.42834°)
RADEC_ERR 1.47 arcsec
LII / BII 169.7877° / -58.9859°
N_CONTRIB 5 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52665.809 (2003-01-26 19:24:42.000 UTC)
MJD_LAST 57756.119 (2017-01-03 02:51:26.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.59e-15 ± 2.1e-15 erg cm-2 s-1

Hardness ratios
HR1
0.80 ± 0.48
0.2-0.5 / 0.5-1.0 keV
HR2
0.54 ± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32 ± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
-0.55 ± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.3) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2

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
778752
Match probability
0.842
FilterMag (AB)Err
UVW2 19.699 0.087
UVM2 19.045 0.047
UVW1 — —
U — —
B — —
V — —
AllWISE
Name
J022002.76-042546.8
Match probability
0.991
BandMagErr
W1 15.218 0.035
W2 15.162 0.086
W3 12.241 0.320
W4 8.745 —
CLASSOPT
Class
Galaxy
Star
0.00
AGN
0.00
Galaxy
1.00

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.