Paper
23 June 2006 Cerro Tololo Inter-American Observatory, Victor M. Blanco 4-m Telescope, and the Dark Energy Survey
Timothy M. C. Abbott, Rolando Catarutti, Eduardo Mondaca, Andres Montane, German Schumacher, Roberto Tighe, Alistair Walker, Del Allspach, Herman Cease, Brenna Flaugher, John Peoples, Andrew Stefanik, Jon Thaler, Vaidotas J. Simatis
Author Affiliations +
Abstract
The CTIO V. M. Blanco 4-m telescope is to be the host facility for the Dark Energy Survey (DES), a large area optical survey intended to measure the dark energy equation of state parameter, w, to a precision of ˜ 5%. The survey is expected to take 5 years and use a new 520 megapixel CCD prime focus imaging system: the Dark Energy Camera (DECam). In preparation for the arrival of DECam, we plan numerous upgrades to the telescope, including a new telescope control system optimized for programmed and queued survey observations, modifications to the telescope itself to improve reliability and performance, extended real-time telemetry of site and facility characteristics, and a distributed observer interface allowing for on- and off-site observations and real time quality control. These upgrades are specifically motivated by the scientific goals of the DES but will also improve community use of the telescope.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Timothy M. C. Abbott, Rolando Catarutti, Eduardo Mondaca, Andres Montane, German Schumacher, Roberto Tighe, Alistair Walker, Del Allspach, Herman Cease, Brenna Flaugher, John Peoples, Andrew Stefanik, Jon Thaler, and Vaidotas J. Simatis "Cerro Tololo Inter-American Observatory, Victor M. Blanco 4-m Telescope, and the Dark Energy Survey", Proc. SPIE 6267, Ground-based and Airborne Telescopes, 62673M (23 June 2006); https://doi.org/10.1117/12.672527
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Cited by 7 scholarly publications.
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KEYWORDS
Telescopes

Mirrors

Control systems

Observatories

Imaging systems

Active optics

Cameras

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