SCUBA-2: a 10,000 pixel submillimeter camera for the James Clerk Maxwell Telescope
arXiv:astro-ph/0606338 · doi:10.1117/12.671186
Abstract
SCUBA-2 is an innovative 10,000 pixel submillimeter camera due to be delivered to the James Clerk Maxwell Telescope in late 2006. The camera is expected to revolutionize submillimeter astronomy in terms of the ability to carry out wide-field surveys to unprecedented depths addressing key questions relating to the origins of galaxies, stars and planets. This paper presents an update on the project with particular emphasis on the laboratory commissioning of the instrument. The assembly and integration will be described as well as the measured thermal performance of the instrument. A summary of the performance results will be presented from the TES bolometer arrays, which come complete with in-focal plane SQUID amplifiers and multiplexed readouts, and are cooled to 100mK by a liquid cryogen-free dilution refrigerator. Considerable emphasis has also been placed on the operating modes of the instrument and the common-user aspect of the user interface and data reduction pipeline. These areas will also be described in the paper.
15 pages; in Proceedings of Millimeter and Submillimeter Detectors and Instrumentation, SPIE, in press
Cited by in corpus (31)
- Measurements of Secondary Cosmic Microwave Background Anisotropies with the South Pole Telescope
- Frequency Multiplexed SQUID Readout of Large Bolometer Arrays for Cosmic Microwave Background Measurements
- First results from BISTRO -- a SCUBA-2 polarimeter survey of the Gould Belt
- The JCMT Legacy Survey of the Gould Belt: a first look at Orion B with HARP
- Interferometric imaging of the high-redshift radio galaxy, 4C60.07: An SMA, Spitzer and VLA study reveals a binary AGN/starburst
- The evolution of submillimetre galaxies: two populations and a redshift cut-off
- The JCMT Legacy Survey of the Gould Belt: mapping 13CO and C18O in Orion A
- Faint Submillimter Galaxy Counts at 450 micron
- Digital Frequency Domain Multiplexer for mm-Wavelength Telescopes
- Scanning strategies for imaging arrays
- The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP
- CRUSH: fast and scalable data reduction for imaging arrays
- Observing Extended Sources with the \Herschel SPIRE Fourier Transform Spectrometer
- The dark GRB080207 in an extremely red host and the implications for GRBs in highly obscured environments
- SPIDER: a balloon-borne CMB polarimeter for large angular scales
- Spider Optimization: Probing the Systematics of a Large Scale B-Mode Experiment
- Empirical modelling of the BLASTPol achromatic half-wave plate for precision submillimetre polarimetry
- The Infrared Properties of Submillimeter Galaxies: Clues From Ultra-Deep 70 Micron Imaging
- Contribution of Lensed SCUBA Galaxies to the Cosmic Infrared Background
- The JCMT Gould Belt Survey: A First Look at IC 5146
- Predicting the incidence of planets and debris discs as a function of stellar mass
- The JCMT Gould Belt Survey: Evidence for radiative heating in Serpens MWC 297 and its influence on local star formation
- The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X
- Submillimetre surveys: The prospects for Herschel
- 143 GHz brightness measurements of Uranus, Neptune, and other secondary calibrators with Bolocam between 2003 and 2010
- Outbursting Young Stellar Object PGIR 20dci in the Perseus Arm
- Diffraction Considerations for Planar Detectors in the Few-Mode Limit
- Device modeling of superconductor transition edge sensors based on the two-fluid theory
- Biasing and Demodulation Firmware for Kilopixel TES Bolometer Arrays
- Simulations of partially coherent focal plane imaging arrays: Fisher matrix approach to performance evaluation
- Demonstration of wideband metal mesh filters for submillimeter astrophysics using flexible printed circuits