We report on the status of The Tierras Observatory at the F.L. Whipple Observatory atop Mt. Hopkins, Arizona, a refurbished 1.3-m ultra-precise fully-automated photometer. Tierras is designed to regularly achieve photometric precisions below 700 ppm from the ground, which will enable the characterization of terrestrial planet transits orbiting < 0.3R stars with 3σ significance, as well as the potential discovery of exo-moons and exo-rings. The design choices that will enable our science goals include: a four-lens focal reducer and field-flattener to increase the field-of-view of the telescope from a 11.94' to a 0.48‡ side; a custom narrow bandpass (40.2 nm FWHM) filter centered around 863.5 nm to minimize precipitable water vapor (PWV) errors known to limit ground-based photometry of red dwarfs; and a deep-depletion 4K x 4K CCD with a 300ke- full well and QE< 85% in our bandpass, operating in frame transfer mode. We are also pursuing the design⊚ of a set of baffes to minimize the significant amount of scattered light currently reaching the image plane. Tierras will begin science operations in early 2021.
Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks.
You are receiving this notice because your organization may not have SPIE eBooks access.*
*Shibboleth/Open Athens users─please
sign in
to access your institution's subscriptions.
To obtain this item, you may purchase the complete book in print or electronic format on
SPIE.org.
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.