Proceedings Paper
MUSTANG2: a large focal plan array for the 100 meter Green Bank Telescope| Format | Member Price | Non-Member Price |
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Paper Abstract
MUSTANG 2 is a 223 element focal plane that operates between 75 and 105 GHz on the 100 meter Green Bank Telescope. It shares many of the science goals of its predecessor, MUSTANG, but will have fifteen times the sensitivity and five times the field-of-view. Angular scales from 900 to 60 will be recovered with high fidelity providing a unique overlap between high resolution instruments such as ALMA and lower resolution single dish telescopes such as ACT or SPT. Individual TES bolometers are placed behind feedhorns spaced by 1.9λ f and are read out using a microwave SQUID multiplexing system.
Paper Details
Date Published: 23 July 2014
PDF: 8 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 91530J (23 July 2014); doi: 10.1117/12.2056455
Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)
PDF: 8 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 91530J (23 July 2014); doi: 10.1117/12.2056455
Show Author Affiliations
S. R. Dicker, Univ. of Pennsylvania (United States)
P. A. R. Ade, Cardiff Univ. (United Kingdom)
J. Aguirre, Univ. of Pennsylvania (United States)
J. A. Brevik, National Institute of Standards and Technology (United States)
H. M. Cho, National Institute of Standards and Technology (United States)
R. Datta, Univ. of Michigan (United States)
M. J. Devlin, Univ. of Pennsylvania (United States)
B. Dober, Univ. of Pennsylvania (United States)
D. Egan, National Radio Astronomy Observatory (United States)
J. Ford, National Radio Astronomy Observatory (United States)
P. Ford, National Radio Astronomy Observatory (United States)
G. Hilton, National Institute of Standards and Technology (United States)
J. Hubmayr, National Institute of Standards and Technology (United States)
P. A. R. Ade, Cardiff Univ. (United Kingdom)
J. Aguirre, Univ. of Pennsylvania (United States)
J. A. Brevik, National Institute of Standards and Technology (United States)
H. M. Cho, National Institute of Standards and Technology (United States)
R. Datta, Univ. of Michigan (United States)
M. J. Devlin, Univ. of Pennsylvania (United States)
B. Dober, Univ. of Pennsylvania (United States)
D. Egan, National Radio Astronomy Observatory (United States)
J. Ford, National Radio Astronomy Observatory (United States)
P. Ford, National Radio Astronomy Observatory (United States)
G. Hilton, National Institute of Standards and Technology (United States)
J. Hubmayr, National Institute of Standards and Technology (United States)
K. D. Irwin, Stanford Univ. (United States)
B. S. Mason, National Radio Astronomy Observatory (United States)
P. Marganian, National Radio Astronomy Observatory (United States)
M. Mello, National Radio Astronomy Observatory (United States)
J. J. McMahon, Univ. of Michigan (United States)
T. Mroczkowski, U.S. Naval Research Lab. (United States)
C. Romero, Stanford Univ. (United States)
Univ. of Virginia (United States)
S. Stanchfield, Univ. of Pennsylvania (United States)
C. Tucker, Cardiff Univ. (United Kingdom)
L. Vale, National Institute of Standards and Technology (United States)
S. White, National Radio Astronomy Observatory (United States)
M. Whitehead, National Radio Astronomy Observatory (United States)
A. H. Young, Univ. of Pennsylvania (United States)
B. S. Mason, National Radio Astronomy Observatory (United States)
P. Marganian, National Radio Astronomy Observatory (United States)
M. Mello, National Radio Astronomy Observatory (United States)
J. J. McMahon, Univ. of Michigan (United States)
T. Mroczkowski, U.S. Naval Research Lab. (United States)
C. Romero, Stanford Univ. (United States)
Univ. of Virginia (United States)
S. Stanchfield, Univ. of Pennsylvania (United States)
C. Tucker, Cardiff Univ. (United Kingdom)
L. Vale, National Institute of Standards and Technology (United States)
S. White, National Radio Astronomy Observatory (United States)
M. Whitehead, National Radio Astronomy Observatory (United States)
A. H. Young, Univ. of Pennsylvania (United States)
Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)
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