2014/10/31 by Reinhold Schaaf, R. Schaaf, Schaaf, Reinhold +9
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy and Astrophysical Research #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Stellar, planetary, and galactic studies #astro-ph.IM
paper · pdf · doi:10.48550/arxiv.1410.8788
Submitted to Proceedings of ADASS XXIV
arxiv created 2014/10/31 · openalex publication_date 2014/10/31 · arxiv updated 2014/11/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01
CCAT will be a large sub-millimeter telescope to be built near the ALMA site in northern Chile. The telescope must support a varied set of instrumentation including large format KID cameras, a large heterodyne array and a KID-based direct detection multi-object spectrometer. We are developing a new raw data model based on HDF5 that can cope with the expected data rates of order Gbit/s and is flexible enough to hold raw data from all planned instruments.