VizieR Online Data Catalog: Exoplanet host stars SPHERE multiplicity survey (Ginski+, 2021)

All observations were conducted with SPHERE/IRDIS (Infra-Red Dual Imager and Spectrograph) at the ESO/VLT in field stabilized classical imaging mode with the broad-band Ks filter. The bright primary star was always placed behind an apodized Lyot coronagraph with an inner working angle of 120mas. Individual frame exposure times (3s-16s) were adjusted such that the residual light from the primary star does not reach saturation levels. The total integration time for all targets was between 3.2 and 6 min.

(2 data files).