pith. sign in

arxiv: 1410.8788 · v1 · pith:ANBOBVHUnew · submitted 2014-10-31 · 🌌 astro-ph.IM

A new HDF5 based raw data model for CCAT

classification 🌌 astro-ph.IM
keywords datalargeccathdf5modeltelescopealmaarray
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.