GISMO, a 2 mm Bolometer Camera Optimized for the Study of High Redshift Galaxies View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2008-05

AUTHORS

Johannes Staguhn, Christine Allen, Dominic Benford, Elmer Sharp, Troy Ames, Rick Arendt, David Chuss, Eli Dwek, Attila Kovacs, Stephen Maher, Catherine Marx, Tim Miller, S. Harvey Moseley, Santiago Navarro, Albrecht Sievers, George Voellmer, Edward Wollack

ABSTRACT

The 2 mm spectral range provides a unique terrestrial window enabling ground based observations of the earliest active dusty galaxies in the universe and thereby allowing a better constraint on the star formation rate in these objects. We have built GISMO (the Goddard-IRAM Superconducting 2-Millimeter Observer), a 2 mm, 128 element superconducting Transition Edge Sensor (TES) based bolometer camera for the IRAM 30 m telescope in Spain. The camera uses an 8×16 planar array of multiplexed TES bolometers, which incorporates our recently designed Backshort Under Grid (BUG) architecture, described elsewhere. The optical design incorporates a 100 mm (4 inches) diameter silicon lens cooled to 4 K, which provides the required fast beam of 0.9 λ/D. With this spatial sampling, GISMO will be very efficient at detecting sources serendipitously in large sky surveys, while the capability for diffraction-limited observations is preserved. With the background limited performance of the detectors, the camera provides significantly greater imaging sensitivity and mapping speed at this wavelength than has previously been possible. The major scientific driver for the instrument is to provide the IRAM 30 m telescope with the capability to rapidly observe galactic and extragalactic dust emission, in particular from high-z Ultra Luminous Infrared Galaxies (ULIRGs) and quasars, even in the summer season. The instrument will fill in the SEDs of high redshift galaxies at the Rayleigh-Jeans part of the dust emission spectrum, even at the highest redshifts. Our source count models predict that GISMO will serendipitously detect one galaxy every four hours on the blank sky, and that one quarter of these galaxies will be at a redshift of z 6.5. We expect to install GISMO at the 30 m telescope in the second half of 2007. More... »

PAGES

709-714

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10909-008-9733-6

DOI

http://dx.doi.org/10.1007/s10909-008-9733-6

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1051345605


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