1 edition of Millimeter and submillimeter detectors and instrumentation for astronomy IV found in the catalog.
Millimeter and submillimeter detectors and instrumentation for astronomy IV
William D. Duncan
Published
2008
by SPIE in Bellingham, Wash
.
Written in English
Edition Notes
| Other titles | Millimeter and submillimeter detectors for astronomy II. |
| Statement | William D. Duncan ... [et al.], editors ; sponsored by SPIE [and] SPIE Europe ; cooperating organizations, AAS--American Astronomical Society (USA) ... [et al.]. |
| Series | Proceedings of SPIE -- 7020, Proceedings of SPIE--the International Society for Optical Engineering -- v. 7020. |
| Contributions | SPIE (Society), SPIE Europe, American Astronomical Society |
| Classifications | |
|---|---|
| LC Classifications | QB479.4 .M565 2008 |
| The Physical Object | |
| Pagination | 1 v. (various pagings) : |
| ID Numbers | |
| Open Library | OL24443104M |
| ISBN 10 | 0819472301 |
| ISBN 10 | 9780819472304 |
| LC Control Number | 2010459216 |
| OCLC/WorldCa | 263413691 |
Low-loss lenses are required for submillimeter astronomical applications, such as instrumentation for CCAT, a 25 m diameter telescope to be built at an elevation of 18, ft in Chile. Silicon is a leading candidate for dielectric lenses due to its low transmission loss and high index of refraction; however, the latter can lead to large reflection losses. In Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV [] BLAST-pol. in Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV., , Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV. (Proceedings of SPIE - The International Society for Optical.
Instrumentation Optical, Infrared, and Millimeter Wave Sunday-Friday 27 June-2 July • Part of Proceedings of SPIE Vol. Space Telescopes and Instrumentation Optical, Infrared, and Millimeter . Proceedings of SPIE—The International Society for Optical Engineering conference on Millimeter and Submillimeter Detectors for Astronomy II, Eds. J. Zmuidzinas, W.S. Holland, & S. Withington, Vol. , pp. ().
Jerry Shiao, YS & Looney, LW , Temperature-regulated 22 GHz water vapor radiometers for CARMA. in Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV., F, Proceedings of SPIE - The International Society for Optical Engineering, vol. , Millimeter and Submillimeter Detectors and Instrumentation for Astronomy. In Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV. O (Proceedings of SPIE - The International Society for Optical Engineering; Vol. ). M , Sensitive far-IR survey spectroscopy: BLISS for SPICA. in Millimeter and.
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Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Editor(s): William D. Duncan ; Wayne S. Holland ; Stafford Withington ; Jonas Zmuidzinas For the purchase of this volume in printed format, please visit Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Duncan, William D.; Holland, Wayne S.; Withington, Stafford; Zmuidzinas, Jonas; Abstract.
Publication: Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Cited by: Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III. Editor(s): Jonas Zmuidzinas; Kinetic inductance detectors for μm astronomy Author(s): Development of a GaAs-based BIB detector for sub-mm wavelengths.
The majority of the textbooks on this site are PDF, some of them are EPUB. Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III latest uploaded books, you can search book title name or ISBN in the search box.
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III PDF search engine helps you find free books in pdf format. The pointing Further author information: (Send correspondence to G.
Marsden) G. Marsden: E-mail: [email protected], Telephone: Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV edited by William D. Duncan, Wayne S. Holland, Stafford Withington, Jonas Zmuidzinas Proc. of SPIE Vol., ( Morozov, D, Mauskopf, P, Dunscombe, C & Henini, MAntenna coupled direct detector for millimetre and submillimetre astronomy based on 2D electron gas in semiconducting heterostructure.
in Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV.,Proceedings of SPIE - The International Society for Optical. Walker, CK, Kulesa, C, Groppi, C & Golish, DFuture prospects for THz spectroscopy. in Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV.,Proceedings of SPIE - The International Society for Optical Engineering, vol.
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV. Would be good for courses based primarily on describing detectors for astronomy or scientific instrumentation.
However, does not give much coverage to HgCdTe, a workhorse in the and micron ranges, and does not cover some fairly standard descriptions (e.g.
RoA product) of noise for such s: 2. Proc. SPIE.Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII. KEYWORDS: Staring arrays, Bolometers, Astronomy, Switches, Sensors, Superconductors, Detector arrays, Multiplexers, Semiconducting wafers, Cryogenics Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV.
Submillimetre astronomy or submillimeter astronomy (see spelling differences) is the branch of observational astronomy that is conducted at submillimetre wavelengths (i.e., terahertz radiation) of the electromagnetic omers place the submillimetre waveband between the far-infrared and microwave wavebands, typically taken to be between a few hundred micrometres and a millimetre.
Get this from a library. Millimeter and submillimeter detectors and instrumentation for astronomy IV: JuneMarseille, France. [W D Duncan; SPIE (Society); SPIE Europe.; American Astronomical Society.;].
Galitzki, N. [] “, Instrumental performance and results from testing of the BLAST-TNG receiver, submillimeter optics, and MKID detector arrays, ” Proc. SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, Vol.p.
PROCEEDINGSOFSPIE Millimeter, Submillimeter, and Far-Infrared Detectorsand InstrumentationforAstronomyV WayneS.
Holland JonasZmuidzinas Editors 29June-2July San Diego, California, United States Sponsored by SPIE CooperatingOrganizations AmericanAstronomical Society (United States) • Association of Universities for Researchin Astronomy, Inc.
(United States) •. spectrometer for submillimeter wave astronomy (Conference Presentation)," Proc. SPIEMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX, N (10 July ).
[12] Kirit S. Karkare, Peter S. Barry, C. Matt Bradford, Scott Chapman. Millimeter, Submillimeter, and Far-infrared Detectors and Instrumentation for Astronomy: Volume V: 29 June-2 JulySan Diego, California, United States on *FREE* shipping on qualifying offers.
Proceedings of SPIE present the original research papers presented at SPIE conferences and other high-quality conferences in the broad-ranging fields of optics and photonics. MUSIC (the Multiwavelength Submillimeter kinetic Inductance Camera) is an instrument being developed for the Caltech Submillimeter Observatory by Caltech, JPL, the University of Colorado, and UCSB.
MUSIC uses microwave kinetic inductance detectors (MKIDs) - superconducting micro-resonators - as photon detectors. The readout is almost entirely at room temperature and is highly.
Karwan Rostem, Dorota M. Glowacka, David J. Goldie, and Stafford Withington "Thermal conductance measurements for the development of ultra low-noise transition-edge sensors with a new method for measuring the noise equivalent power", Proc. SPIEMillimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, L (18 July.
Browse our growing collection of more thanconference proceedings papers. The MKID Camera is a millimeter/submillimeter instrument being built for astronomical observations from the Caltech Submillimeter Observatory.
It utilizes microwave kinetic inductance detectors, which are rapidly achieving near-BLIP sensitivity for ground-based observations, and a software-defined radio readout technique for elegant multiplexing of a large number of detectors.
Home; Profiles; Departments and Centers; Scholarly Works; Activities; Equipment; Grants; Prizes. Millimeter and submillimeter-wave observations provide important information for the studies of atmospheric chemistry and astrochemistry (molecular clouds, stars formation, galactic study, comets and cosmology).
But, these observations depend strongly on instrumentation .and Far-Infrared Detectors and Instrumentation for Astronomy VIII],T, International Society for Optics and Photonics ().
[15]Soliman, A., Ade, P., et al., \Design and performance of single/wide band corrugated walls for the bi-cep array detector modules at 30/40 ghz," in [Millimeter, Submillimeter, and Far-Infrared Detectors and.
Previous conference titled: Millimeter and submillimeter detectors and instrumentation for astronomy IV. Title from PDF title screen (SPIE digital library, viewed Aug. 12, ). Description: 1 online resource: illustrations (some color). Series Title: Proceedings of SPIE--the International Society for Optical Engineering, v.
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