Integrated heterodyne array receivers for submillimeter astronomy

C. K. Walker; C. E. Groppi; C. Drouet D'Aubigny; C. Kulesa; A. Hedden; D. Prober; I. Siddiqi; J. Kooi; G. Chen; A. W. Lichtenberger

doi:10.1117/12.459375

Integrated heterodyne array receivers for submillimeter astronomy

C. K. Walker, C. E. Groppi, C. Drouet D'Aubigny, C. Kulesa, A. Hedden, D. Prober, I. Siddiqi, J. Kooi, G. Chen, A. W. Lichtenberger

Research output: Contribution to journal › Conference article › peer-review

7 Scopus citations

Abstract

The advent of large format (∼100 pixels) spectroscopic imaging cameras at submillimeter wavelength would fundamentally change the way in which astronomy is performed in this important wavelength regime. While the possibility of such instruments has been discussed for more than two decades, only recently have advances in mixer technology, device fabrication, micromachining, digital signal processing, and telescope design made the construction of such an instrument possible and economical. In our paper, we will present the design concept for a 10×10 heterodyne camera.

Original language	English (US)
Pages (from-to)	349-354
Number of pages	6
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	4855
DOIs	https://doi.org/10.1117/12.459375
State	Published - 2002
Event	Millimeter and Submillimeter Detectors for Astronomy - Waikaloa, HI, United States Duration: Aug 25 2002 → Aug 28 2002

Keywords

SIS heterodyne array receiver submillimeter molecular spectroscopy

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.459375

Cite this

@article{d87e439268c747ee9a9e2c62da6f3439,

title = "Integrated heterodyne array receivers for submillimeter astronomy",

abstract = "The advent of large format (∼100 pixels) spectroscopic imaging cameras at submillimeter wavelength would fundamentally change the way in which astronomy is performed in this important wavelength regime. While the possibility of such instruments has been discussed for more than two decades, only recently have advances in mixer technology, device fabrication, micromachining, digital signal processing, and telescope design made the construction of such an instrument possible and economical. In our paper, we will present the design concept for a 10×10 heterodyne camera.",

keywords = "SIS heterodyne array receiver submillimeter molecular spectroscopy",

author = "Walker, {C. K.} and Groppi, {C. E.} and D'Aubigny, {C. Drouet} and C. Kulesa and A. Hedden and D. Prober and I. Siddiqi and J. Kooi and G. Chen and Lichtenberger, {A. W.}",

year = "2002",

doi = "10.1117/12.459375",

language = "English (US)",

volume = "4855",

pages = "349--354",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

issn = "0277-786X",

publisher = "SPIE",

note = "Millimeter and Submillimeter Detectors for Astronomy ; Conference date: 25-08-2002 Through 28-08-2002",

}

TY - JOUR

T1 - Integrated heterodyne array receivers for submillimeter astronomy

AU - Walker, C. K.

AU - Groppi, C. E.

AU - D'Aubigny, C. Drouet

AU - Kulesa, C.

AU - Hedden, A.

AU - Prober, D.

AU - Siddiqi, I.

AU - Kooi, J.

AU - Chen, G.

AU - Lichtenberger, A. W.

PY - 2002

Y1 - 2002

N2 - The advent of large format (∼100 pixels) spectroscopic imaging cameras at submillimeter wavelength would fundamentally change the way in which astronomy is performed in this important wavelength regime. While the possibility of such instruments has been discussed for more than two decades, only recently have advances in mixer technology, device fabrication, micromachining, digital signal processing, and telescope design made the construction of such an instrument possible and economical. In our paper, we will present the design concept for a 10×10 heterodyne camera.

AB - The advent of large format (∼100 pixels) spectroscopic imaging cameras at submillimeter wavelength would fundamentally change the way in which astronomy is performed in this important wavelength regime. While the possibility of such instruments has been discussed for more than two decades, only recently have advances in mixer technology, device fabrication, micromachining, digital signal processing, and telescope design made the construction of such an instrument possible and economical. In our paper, we will present the design concept for a 10×10 heterodyne camera.

KW - SIS heterodyne array receiver submillimeter molecular spectroscopy

UR - http://www.scopus.com/inward/record.url?scp=0038470009&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0038470009&partnerID=8YFLogxK

U2 - 10.1117/12.459375

DO - 10.1117/12.459375

M3 - Conference article

AN - SCOPUS:0038470009

SN - 0277-786X

VL - 4855

SP - 349

EP - 354

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

T2 - Millimeter and Submillimeter Detectors for Astronomy

Y2 - 25 August 2002 through 28 August 2002

ER -

Integrated heterodyne array receivers for submillimeter astronomy

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this