Invited article: millimeter-wave bolometer array receiver for the Atacama pathfinder experiment Sunyaev-Zel'dovich (APEX-SZ) instrument.

@article{Schwan2011InvitedAM,
  title={Invited article: millimeter-wave bolometer array receiver for the Atacama pathfinder experiment Sunyaev-Zel'dovich (APEX-SZ) instrument.},
  author={Dan Schwan and P. A. R. Ade and Kaustuv Basu and A. N. Bender and Frank Bertoldi and H-M. Cho and G. Chon and John Clarke and M. A. Dobbs and Daniel Ferrusca and Robert G{\"u}sten and N. W. Halverson and W. L. Holzapfel and C. Horellou and Daniel Johansson and B R Johnson and Joseph Kennedy and Zigmund D. Kermish and R{\"u}diger Kneissl and Trevor Lanting and A. T. Lee and M. Lueker and Jared Mehl and Karl M. Menten and Dirk Muders and F. Pacaud and Thomas J. Plagge and C. L. Reichardt and Paul L. Richards and R. Schaaf and Peter Schilke and M Sommer and H. Spieler and C E Tucker and Axel Weiss and B Westbrook and Oliver Zahn},
  journal={The Review of scientific instruments},
  year={2011},
  volume={82 9},
  pages={
          091301
        }
}
  • D. Schwan, P. Ade, +34 authors O. Zahn
  • Published 2 August 2010
  • Physics, Medicine
  • The Review of scientific instruments
The Atacama pathfinder experiment Sunyaev-Zel'dovich (APEX-SZ) instrument is a millimeter-wave cryogenic receiver designed to observe galaxy clusters via the Sunyaev-Zel'dovich effect from the 12 m APEX telescope on the Atacama plateau in Chile. The receiver contains a focal plane of 280 superconducting transition-edge sensor (TES) bolometers instrumented with a frequency-domain multiplexed readout system. The bolometers are cooled to 280 mK via a three-stage helium sorption refrigerator and a… 
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The apex-sz instrument is designed for the discovery and study of galaxy clusters at mm-wavelengths using the Sunyaev Zel’dovich effect. The receiver consists of 320 superconducting transition edge
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The Atacama Cosmology Telescope was designed to measure small-scale anisotropies in the cosmic microwave background and detect galaxy clusters through the Sunyaev-Zel'dovich effect. The instrument is
The Atacama Cosmology Telescope: The Receiver and Instrumentation
The Atacama Cosmology Telescope was designed to measure small-scale anisotropies in the Cosmic Microwave Background and detect galaxy clusters through the Sunyaev-Zel’dovich effect. The instrument is
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We describe BOOMERANG, a balloon-borne microwave telescope designed to map the cosmic microwave background at a resolution of 10' from the Long Duration Balloon (LDB) platform. The millimeter-wave
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Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich effect
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Q/U Imaging Experiment (QUIET): a ground-based probe of cosmic microwave background polarization
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  • Physics, Engineering
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QUIET is an experimental program to measure the polarization of the Cosmic Microwave Background (CMB) radiation from the ground. Previous CMB polarization data have been used to constrain the
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