5XMM J174732.8-282104

5XMM-DR15 stacked source · SRCID 3003054010100466
Position: 17h47m32.83s -28d21m04.0s (266.88678°, -28.35110°)
EP flux
9.05e-15 ± 7.1e-16 erg cm-2 s-1
CLASSX
Star (0.995)
Detections
16

SRCID 3003054010100466
IAUNAME 5XMM J174732.8-282104
SC_RA 17h47m32.83s (266.88678°)
SC_DEC -28d21m04.0s (-28.35110°)
RADEC_ERR 0.26 arcsec
LII / BII 0.7196° / -0.0575°
N_CONTRIB 16 (detections)
N_OBS 308 (observations covering the position)
MJD_FIRST 51802.795 (2000-09-15 19:04:46.000 UTC)
MJD_LAST 59127.048 (2020-10-05 01:09:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 9.05e-15 ± 7.1e-16 erg cm-2 s-1

Hardness ratios
HR1
0.73 ± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03 ± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.83 ± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.92 ± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.9) SUM_FLAG: 1
Long-term lightcurve

Star

CLASSX outlier: 3.76

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
4880885
Match probability
0.997
FilterMag (AB)Err
UVW2 21.196 0.312
UVM2 20.826 0.078
UVW1 18.140 0.009
U 16.996 0.005
B 15.531 0.004
V 14.897 0.004
Gaia DR3
Source ID
4057530959741338112
Match probability
0.989
Parallax
1.060 ± 0.029 mas
Proper motion
(1.56, 4.34) mas/yr
Magnitudes
G=14.57, BP=15.09, RP=13.89
Distance
869 pc
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
Galaxy
0.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.22e-14 (+1.4e-14 / −1.1e-14) erg cm−2 s−1
NH 2.29e+21 (+2.6e+21 / −1.9e+21) cm−2
Photon index (Γ) 2.90 (+2.97 / −2.76)
DoF 201
p-value 0.089
Inter-instrument norm. 1.03 (0.85–1.24)
Quality flag 0

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.