Poster + Presentation + Paper
13 December 2020 Deployment of beam alignment hardware at the Magdalena Ridge Observatory Interferometer
Author Affiliations +
Conference Poster
Abstract
The first unit telescope of Ridge Observatory Interferometer is integrated on the array and starlight has been observed in the Beam Combining Area for the first time. From the telescope, the beam travels in vacuum over a path of >50m, including a beam relay system and delay line. This feat was made possible by a prototype version of the Automated Alignment System that we are developing for minimising fringe visibility loss due to misalignment. We present results of on-site validation of UTLIS, a reference light source at the unit telescope acting as a proxy for starlight, and BEASST, a Shack-Hartmann sensor that simultaneously detects beam angle and position.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
James J. D. Luis, David F. Buscher, Chuck Dahl, Jonathan F. Dooley, Allen Farris, Christopher A. Haniff, E. Robert Ligon, Siavash Norouzi, Xiaowei Sun, and John S. Young "Deployment of beam alignment hardware at the Magdalena Ridge Observatory Interferometer", Proc. SPIE 11446, Optical and Infrared Interferometry and Imaging VII, 1144628 (13 December 2020); https://doi.org/10.1117/12.2562863
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Active optics

Interferometers

Magdalena Ridge Observatory

Optical alignment

Heart

Long baseline optical interferometry

Optical tracking

Back to Top