Abstract
The exoplanet search is one of the most exciting research fields in astrophysics. The Antarctic Bright Star Survey Telescope (BSST), capable of continuous exoplanet observation on polar nights, is a Ritchey–Chretien telescope with a three-lens field corrector, and has a 300 mm aperture, 2.76 focal ratio, and a wavelength coverage ranging from 0.36 to 1.014 μm. Equipped with a 4 k×4 k and 12 μm/pixel CCD camera, the BSST can gain a field of view of 4.8°. This Letter presents the optical design, tolerance analysis, and the alignment plan for the BSST, and the test observation results.
© 2015 Chinese Laser Press
PDF Article
More Like This
Active optics system of the VLT Survey Telescope
Pietro Schipani, Lothar Noethe, Demetrio Magrin, Konrad Kuijken, Carmelo Arcidiacono, Javier Argomedo, Massimo Capaccioli, Massimo Dall’Ora, Sergio D’Orsi, Jacopo Farinato, Davide Fierro, Ronald Holzlöhner, Laurent Marty, Cesare Molfese, Francesco Perrotta, Roberto Ragazzoni, Salvatore Savarese, Andrew Rakich, and Gabriele Umbriaco
Appl. Opt. 55(7) 1573-1583 (2016)
Cited By
You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Login to access Optica Member Subscription