HERE WE PROPOSE BOTH 20S AND 2MIN CADENCE TESS OBSERVATIONS OF KNOWN BINARY AND PULSATING HOT SUBDWARF STARS VISIBLE IN CYCLE 3. WE HAVE ALSO IDENTIFIED A LARGE NUMBER OF CANDIDATE VARIABLE HOT SUBDWARFS FROM THEIR ANOMALOUSLY HIGH GAIA FLUX ERRORS
$41,168FY2021National Aeronautics and Space AdministrationNASA
High Point University, High Point NC