MINERVA-Australis: Two years of TESS follow-up
Creators
- 1. University of Southern Queensland
- 2. University of Florida
- 3. Sydney University
- 4. University of Texas at Austin
- 5. University of California Riverside
- 6. University of Louisville
- 7. Nanjing University
- 8. George Mason University
- 9. MIT
- 10. UNSW Sydney
Description
MINERVA-Australis at the University of Southern Queensland's Mount Kent
Observatory is the only southern hemisphere precise radial velocity
facility wholly dedicated to follow-up of TESS planets.
MINERVA-Australis is a partnership between MIT, UNSW Sydney, George
Mason University, University of Louisville, Nanjing University,
UC-Riverside, University of Texas, and the University of Florida.
Observing time is also available to the US community via NSF NOIRLab
proposal calls. Being fully robotic, we have been unaffected by
Covid-19 closures. We have contributed data to the validation of 23
TESS planets. I give an overview and update of operations, highlighting
our recent mass measurements for TOI-778 and TOI-1842. I also describe
our new photometric capabilities, aiming to validate small TESS planets
and to rescue planets from ephemeris erosion.
Files
TESS_2021.pdf
Files
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