The CCAT Software System

Tim Jenness; Adam Brazier; Kevin Edwards; Gaelen Marsden; Thomas Nikola; Volker Ossenkopf; Steve Padin; Jack Sayers; Reinhold Schaaf; Martin Shepherd

arXiv · 1401.8280

The CCAT Software System

Tim Jenness·Adam Brazier·Kevin Edwards·Gaelen Marsden·Thomas Nikola·Volker Ossenkopf·Steve Padin·Jack Sayers·Reinhold Schaaf·Martin Shepherd

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Abstract

CCAT will be a 25-meter telescope for sub millimeter astronomy located at 5600m altitude on Cerro Chajnantor in northern Chile. CCAT will combine high sensitivity, a wide field of view, and a broad wavelength range (0.35 to 2.1mm) to provide an unprecedented capability for deep, large-area multicolor submillimeter surveys. It is planned to have a suite of instruments including large format KID cameras, a large heterodyne array and a KID-based direct detection multi-object spectrometer. The remote location drives a desire for fully autonomous observing coupled with data reduction pipelines and fast feedback to principal investigators.

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Tim Jenness, Adam Brazier, Kevin Edwards, Gaelen Marsden, Thomas Nikola, Volker Ossenkopf, Steve Padin, Jack Sayers, Reinhold Schaaf, Martin Shepherd. 2014-01-31. The CCAT Software System. https://arxiv.org/abs/1401.8280

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