5XMM J225329.4-173416

5XMM-DR15 stacked source · SRCID 3001294010100165
Position: 22h53m29.48s -17d34m16.8s (343.37284°, -17.57134°)
EP flux
1.40e-15 ± 1.2e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.567)
Detections
10

SRCID 3001294010100165
IAUNAME 5XMM J225329.4-173416
SC_RA 22h53m29.48s (343.37284°)
SC_DEC -17d34m16.8s (-17.57134°)
RADEC_ERR 1.29 arcsec
LII / BII 46.0922° / -61.1897°
N_CONTRIB 10 (detections)
N_OBS 10 (observations covering the position)
MJD_FIRST 51877.756 (2000-11-29 18:08:56.000 UTC)
MJD_LAST 59199.874 (2020-12-16 20:58:40.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.40e-15 ± 1.2e-15 erg cm-2 s-1

Hardness ratios
HR1
0.61 ± 0.32
0.2-0.5 / 0.5-1.0 keV
HR2
-0.13 ± 0.32
0.5-1.0 / 1.0-2.0 keV
HR3
0.02 ± 0.34
1.0-2.0 / 2.0-4.5 keV
HR4
-0.70 ± 0.71
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.0) SUM_FLAG: 0
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 1.94

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
6503785
Match probability
0.992
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 21.242 0.138
B
V 19.910 0.214
AllWISE
Name
J225329.49-173416.8
Match probability
0.995
BandMagErr
W1 16.049 0.061
W2 15.655 0.131
W3 12.397 0.480
W4 8.424
CLASSOPT
Class
Galaxy
Star
0.02
AGN
0.03
Galaxy
0.95

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.