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A hot-electron direct detector for radioastronomy

Author
KARASIK, B. S1 ; MCGRATH, W. R1 ; LEDUC, H. G1 ; GERSHENSON, M. E2
[1] Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, United States
[2] Department of Physics and Astronomy, Rutgers University, Piscataway, NJ 08854, United States
Conference title
Papers presented at the International Superconductive Electronics Conference, Berkeley, California, 21-25 June 1999
Conference name
International Superconductive Electronics Conference (Berkeley, California 1999-06-21)
Source

Superconductor science & technology (Print). 1999, Vol 12, Num 11, pp 745-747 ; ref : 13 ref

ISSN
0953-2048
Scientific domain
Electronics; Condensed state physics
Publisher
Institute of Physics, Bristol
Publication country
United Kingdom
Document type
Conference Paper
Language
English
Keyword (fr)
Bolomètre Conception Dispositif supraconducteur Instrument astronomique Interaction électron phonon Performance Radioastronomie Relaxation thermique
Keyword (en)
Bolometers Design Superconducting devices Astronomical instruments Electron-phonon interactions Performance Radioastronomy Thermal relaxation
Keyword (es)
Relajación térmica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A55 Astronomical and space-research instrumentation / 001E03A55J Radio telescopes and instrumentation ; heterodyne receivers

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
1217599

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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