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2 edition of A monolithic Si bolometer array for the Caltech Submillimeter Observatory found in the catalog.

A monolithic Si bolometer array for the Caltech Submillimeter Observatory

A monolithic Si bolometer array for the Caltech Submillimeter Observatory

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  • 24 Currently reading

Published by California Institute of Technology, National Aeronautics and Space Administration, National Technical Information Service, distributor in [Pasadena, Calif.], [Washington, DC, Springfield, Va .
Written in English

    Subjects:
  • Astronomy.

  • Edition Notes

    StatementWang, Ning ... [et al.].
    SeriesNASA technical memorandum -- NASA TM-109402., NASA technical memorandum -- 109402.
    ContributionsWang, Ning., United States. National Aeronautics and Space Administration.
    The Physical Object
    FormatMicroform
    Pagination1 v.
    ID Numbers
    Open LibraryOL15400413M

    Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V Editor(s): Wayne S. Holland ; Jonas Zmuidzinas For the purchase of this volume in printed format, please visit SCUBA The older continuum single pixel UKT14 bolometer receiver was replaced in the s by the Submillimeter Common-User Bolometer Array (SCUBA). The SCUBA project was green-lighted in by the JCMT board and was in development for nearly a decade before it saw first light on the telescope.

    Bolocam [1] will be used at the Caltech Submillimeter Observatory (CSO), located near the summit of Mauna Kea, Hawaii, to address important astrophysical problems which require mapping continuum emission from large re-gions of the sky. Over the past years several bolometer arrays with increasing number of detetors have been Size: KB. The Caltech Submillimeter Observatory (CSO) Phillips, T. G. AAS , ADS Theses Millimeter/submillimeter Fourier Transform Spectroscopy of Jovian Planet Atmospheres Weisstein, E. W. PhD Thesis, California Institute of Technology ADS Caltech Library.

    SHARC ll is a _m facility camera for the Caltech Submillimeter Observatory (CSO) expected to come on-line in The key component of SHARC II is a 12x32 array of doped silicon "pop-up" bolometers developed at NASA/Goddard and delivered to Caltech in March Each pixel is 1 mm × 1 ram, coated. 11)\Monolithic Microwave Integrated Circuits for Cosmology and Astrophysics." Special Cosmology Seminar at KICP, University of Chicago, Chicago, IL Ma 12)\Antenna-coupled TES bolometers in BICEP-2, Keck Array, Spider, and Polar-1" SPIE: Millimeter and Submillimeter Detectors and Instrumentation.


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A monolithic Si bolometer array for the Caltech Submillimeter Observatory Download PDF EPUB FB2

A Monolithic Si Bolometer Array for the Caltech Submillimeter Observatory Ning Wang, T. Hunter, D. Benford, E. Serabyn, T. Phillips California Institute of Technology, M/SPasadena, CA S. Moseley Laboratory for Extra Terrestrial Physics, Goddard Space Flight Center, NASA, Code Greenbelt, MD ABSTRACT.

We are developing a submillimeter continuum camera for the Caltech Submillimeter Observatory (CSO) located on Mauna Kea. The camera will employ a monolithic Si bolometer array which was developed by Mosley et al.

at the NASA Goddard Space Flight Center (GSFC). The camera will be cooled to a temperature of about mK in a ^3He cryostat, and will Cited by: 3. A Monolithic Si Bolometer Array for the Caltech Submillimeter Observatory Ning Wang, T. Hunter, D. Benford, E. Serabyn, T.

Phillips California Institute of Technology, M/SPasadena, CA S. Moseley Laboratory for Extra TerreslJ_l Physics, Goddard Space Fright Center NASA, Code Greenbelt, MD We are developing a submillimeter continuum camera for the Caltech Submillimeter Observatory (CSO) located on Mauna Kea.

The camera will employ a monolithic Si bolometer array which was developed by Mosley et al. at the NASA Goddard Space Flight Center (GSFC). The camera will be cooled to a temperature of about mK in a (superscript 3)He cryostat. We are developing a submillimeter continuum camera for the Caltech Submillimeter Observatory (CSO) located on Mauna Kea.

The camera will employ a monolithic Si bolometer array which was developed by Mosley et al. at the NASA Goddard Space Flight Center (GSFC).Cited by: 3. We are developing a submillimeter continuum camera for the Caltech Submillimeter Observatory (CSO) located on Mauna Kea. The camera will employ a monolithic Si bolometer array which was developed by Moseley et al.

at the NASA Goddard Space Flight Center (GSFC). The camera will be cooled to a temperature of about mK in a He-3 cryostat, and. We have constructed a continuum camera for the Caltech Submillimeter Observatory (CSO), operating in the pm and gm atmospheric window'.

It employs a monolithic linear Silicon bolometer. Wang N, Hunter TR, Benford DJ, Serabyn E, Lis DC, Phillips TG et al () Characterization of a submillimeter high-angular resolution camera with a monolithic silicon bolometer array for the Caltech Submillimeter Observatory.

Appl Opt ADS CrossRef Google ScholarAuthor: Vincent Minier, Roger-Maurice Bonnet, Vincent Bontems, Thijs de Graauw, Matt Griffin, Frank Helmich.

The Caltech Submillimeter Observatory (CSO) was formerly one of the world's premier facilities for astronomical research and instrumentation development at submillimeter wavelengths. The m diameter telescope is housed in a compact dome at m altitude near the summit of Maunakea, Hawai'i.

The Caltech Submillimeter Observatory (CSO) was a meter (34 ft) diameter submillimeter wavelength telescope situated alongside the meter (49 ft) James Clerk Maxwell Telescope (JCMT) at Mauna Kea was engaged in submillimetre astronomy, of the terahertz radiation band.

The telescope closed on Septem As of Aprilthe telescope Location(s): Mauna Kea, Hawaii County, US. We describe the development, construction, and testing of two element arrays of ion-implanted semiconducting cryogenic bolometers designed for use in far-infrared and submillimeter cameras.

These two dimensional arrays are assembled from a number of 32 element linear arrays of monolithic Pop-Up bolometer Detectors (PUD) developed at NASA Cited by: 2. Get this from a library. A monolithic Si bolometer array for the Caltech Submillimeter Observatory. [Ning Wang; United States. National Aeronautics and Space Administration.;].

The authors are building a bolometer array for use as a submillimeter continuum camera for the Caltech Submillimeter Observatory (CSO) located on Mauna Kea. who have developed the technique for fabricating monolithic bolometer arrays on Si wafers, as well as a sophisticated data taking system to use with these arrays (Moseley et al., ).

Characterization of a submillimeter high-angular-resolution camera with a monolithic silicon bolometer array for the Caltech Submillimeter Observatory. We present the design and performance of a feedhorn-coupled bolometer array intended for a sensitive µm photometer camera.

Silicon nitride micromesh absorbers minimize the suspended mass and heat capacity of the bolometers. The temperature transducers, neutron-transmutation-doped Ge thermistors, are attached to the absorber with In bump bonds.

The Herschel Space Observatory will carry onboard a new kind of bolometric architecture for the PACS (Photodetector Array Camera and Spectrometer) submillimeter photometer.

These new generation CCD-like multiplexed bolometer arrays are buttable and enable the conception of large fully sampled focal planes either for space or for ground-based Cited by: 7. We have constructed a continuum camera for the Caltech Submillimeter Observatory (CSO), operating in the pm and gm atmospheric window'.

It employs a monolithic linear Silicon bolometer array fabricated by the microelectronics laboratory at the Goddard Space Flight Center (GSFC). The array has 24 bolometer pixels. The Cosmological Evolution Survey (COSMOS) is an astronomical survey designed to probe the formation and evolution of galaxies as a function of both cosmic time (redshift) and the local galaxy environment.

The survey covers a 2 square degree equatorial field with imaging by most of the major space-based telescopes (Hubble, Spitzer, GALEX, XMM, Chandra, Herschel.

We describe a technique that enables bolometer arrays that use quarter-wave cavities to have a high spectral response over most of the submillimeter band. This technique is based on the addition on the front of the array of an antireflecting dielectric layer.

Keywords: bolometer, far-infrared, submillimeter, superconducting, SQUID, detector array, multiplexer, transition edge sensor Introduction Advances in bolometer fabrication have made possible the construction of submillimeter-wavelength cameras with several tens of detectors (e.g., CSO - SHARC (Wang et al.

The Lick Observatory Two Micron Camera.- Infrared Arrays at the European Southern Observatory.- The Impact of Infrared Array Technology on Astronomy.- Monolithic Si Bolometer Arrays: Detectors for far Infrared and Submillimeter Detection.- Observational Concerns and Techniques for High-Background Mid-Infrared ( Micron) Array Imagingthe Millimeter and Submillimeter Astronomy group of the MPIfR.

If the area to be mapped is much larger than the array itself, then the time for mapping to the same depth depends as 1/n, if n is the number of array elements.

As a compromise between technical risk and speed of development the number of array elements was set to around New Developments in Array Technology and Applications Monolithic Si Bolometer Arrays: Detectors for Far Infrared and Submillimeter Detection.

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