5XMM J173527.9-323947

5XMM-DR15 stacked source · SRCID 3000173020102322
Position: 17h35m27.92s -32d39m47.0s (263.86634°, -32.66305°)
EP flux
8.20e-15 ± 3.6e-15 erg cm-2 s-1
CLASSX
Star (1)
Detections
3

SRCID 3000173020102322
IAUNAME 5XMM J173527.9-323947
SC_RA 17h35m27.92s (263.86634°)
SC_DEC -32d39m47.0s (-32.66305°)
RADEC_ERR 0.85 arcsec
LII / BII 355.6844° / -0.1288°
N_CONTRIB 3 (detections)
N_OBS 180 (observations covering the position)
MJD_FIRST 51977.535 (2001-03-09 12:50:44.000 UTC)
MJD_LAST 60386.961 (2024-03-17 23:03:25.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 8.20e-15 ± 3.6e-15 erg cm-2 s-1

Hardness ratios
HR1
0.89 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.02 ± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.90 ± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
0.52 ± 0.63
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.9) SUM_FLAG: 1
Long-term lightcurve

Star

CLASSX outlier: 2.5

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
4721120
Match probability
0.995
FilterMag (AB)Err
UVW2 13.140 0.004
UVM2 13.145 0.002
UVW1
U
B
V
Gaia DR3
Source ID
4054567535397781248
Match probability
0.994
Parallax
0.806 ± 0.028 mas
Proper motion
(2.92, -1.38) mas/yr
Magnitudes
G=11.34, BP=11.44, RP=11.12
AllWISE
Name
J173527.89-323947.8
Match probability
0.996
BandMagErr
W1 10.566 0.058
W2 10.851 0.064
W3 8.889
W4 6.428
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
Galaxy
0.00

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.

APPROX_SOURCE_VAR 5.900 (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.