5XMM J131517.5-162909

5XMM-DR15 stacked source · SRCID 3003795010100016
Position: 13h15m17.50s -16d29m09.6s (198.82290°, -16.48599°)
EP flux
4.23e-13 ± 1.1e-14 erg cm-2 s-1
CLASSX
Bkg_AGN (0.962)
Detections
2

SRCID 3003795010100016
IAUNAME 5XMM J131517.5-162909
SC_RA 13h15m17.50s (198.82290°)
SC_DEC -16d29m09.6s (-16.48599°)
RADEC_ERR 0.16 arcsec
LII / BII 311.1778° / 46.0035°
N_CONTRIB 2 (detections)
N_OBS 6 (observations covering the position)
MJD_FIRST 51921.880 (2001-01-12 21:07:12.000 UTC)
MJD_LAST 54829.307 (2008-12-29 07:22:25.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.23e-13 ± 1.1e-14 erg cm-2 s-1

Hardness ratios
HR1
-0.94 ± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
0.93 ± 0.17
0.5-1.0 / 1.0-2.0 keV
HR3
0.97 ± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
0.38 ± 0.02
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 262.8) SUM_FLAG: 0
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.27

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
3443072
Match probability
0.98
FilterMag (AB)Err
UVW2
UVM2 20.907 0.202
UVW1 18.220 0.028
U 17.183 0.010
B 15.718 0.007
V 14.901 0.007
Gaia DR3
Source ID
3511397383823011968
Match probability
0.993
Magnitudes
G=21.00, BP=17.58, RP=16.17
AllWISE
Name
J131517.56-162909.7
Match probability
0.995
BandMagErr
W1 12.127 0.023
W2 11.970 0.023
W3 9.907 0.046
W4 7.602 0.158
CLASSOPT
Class
Galaxy
Star
0.04
AGN
0.01
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.

APPROX_SOURCE_VAR 36.900 (approximate flux variability amplitude)

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.