5XMM J022108.6-043907

5XMM-DR15 stacked source · SRCID 3003798200111590
Position: 02h21m08.67s -04d39m07.7s (35.28614°, -4.65215°)
EP flux
2.44e-15 ± 1.7e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.631)
Detections
8

SRCID 3003798200111590
IAUNAME 5XMM J022108.6-043907
SC_RA 02h21m08.67s (35.28614°)
SC_DEC -04d39m07.7s (-4.65215°)
RADEC_ERR 2.19 arcsec
LII / BII 170.4732° / -58.9758°
N_CONTRIB 8 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52500.578 (2002-08-14 13:52:48.000 UTC)
MJD_LAST 57756.635 (2017-01-03 15:14:59.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 2.44e-15 ± 1.7e-15 erg cm-2 s-1

Hardness ratios
HR1
0.38 ± 0.21
0.2-0.5 / 0.5-1.0 keV
HR2
0.04 ± 0.20
0.5-1.0 / 1.0-2.0 keV
HR3
-0.48 ± 0.24
1.0-2.0 / 2.0-4.5 keV
HR4
-0.59 ± 0.85
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -0.9) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 3.64

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
785693
Match probability
0.995
FilterMag (AB)Err
UVW2 20.532 0.205
UVM2 19.030 0.056
UVW1 18.200 0.014
U — —
B — —
V — —
Gaia DR3
Source ID
2489789659568853504
Match probability
0.979
Magnitudes
G=19.99, BP=18.15, RP=16.78
AllWISE
Name
J022108.79-043908.3
Match probability
0.842
BandMagErr
W1 13.229 0.029
W2 13.150 0.035
W3 10.284 0.067
W4 8.261 0.336
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.