Far-infrared Array Receiver (FAR) for SOFIA

Christopher K Walker, C. E. Groppi, C. Y Drouet d'Aubigny, G. Chen, R. Schieder, G. Narayanan, A. Lichtenberger, P. Siegel

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

In this paper, we present the design for a 16-channel heterodyne array receiver for use on SOFIA. The array will be capable of using either hot-electron bolometers or membrane mounted Schottky diodes in efficient, low-cost waveguide mounts. Focal plane arrays will be constructed to target astrophysically important lines between approximately 1.9 and 3 THz. Due to the prevailing physical conditions in the interstellar medium, this frequency range is one of the richest in the FIR portion of the spectrum. An array receiver designed for this wavelength range will make excellent use of the telescope and the available atmospheric transmission, and will provide a new perspective on stellar, chemical, and galaxy evolution in the present as well as past epochs. The proposed system uses the most sensitive detectors available in an efficient optical system. The local oscillator will be a compact CO2 pumped far-infrared laser specifically developed for SOFIA. The backend spectrometer will be a 4×4 array of acousto-optic spectrometers (AOS). The spectrometer utilizes proven hardware and technologies to provide broadband performance (≥1 GHz per AOS channel) and high spectral resolution (1 MHz). The proposed instrument will be the fastest and most sensitive heterodyne receiver ever to operate in its wavelength regime.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
PublisherSociety of Photo-Optical Instrumentation Engineers
Pages125-136
Number of pages12
Volume4014
StatePublished - 2000
EventAirborne Telescope Systems - Munich, Ger
Duration: Mar 27 2000Mar 28 2000

Other

OtherAirborne Telescope Systems
CityMunich, Ger
Period3/27/003/28/00

Fingerprint

SOFIA (airborne observatory)
Spectrometers
receivers
spectrometers
Infrared radiation
acousto-optics
Optics
Wavelength
Bolometers
Galaxies
Focal plane arrays
Hot electrons
Infrared lasers
Spectral resolution
stellar evolution
chemical evolution
bolometers
focal plane devices
Schottky diodes
hot electrons

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Condensed Matter Physics

Cite this

Walker, C. K., Groppi, C. E., d'Aubigny, C. Y. D., Chen, G., Schieder, R., Narayanan, G., ... Siegel, P. (2000). Far-infrared Array Receiver (FAR) for SOFIA. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 4014, pp. 125-136). Society of Photo-Optical Instrumentation Engineers.

Far-infrared Array Receiver (FAR) for SOFIA. / Walker, Christopher K; Groppi, C. E.; d'Aubigny, C. Y Drouet; Chen, G.; Schieder, R.; Narayanan, G.; Lichtenberger, A.; Siegel, P.

Proceedings of SPIE - The International Society for Optical Engineering. Vol. 4014 Society of Photo-Optical Instrumentation Engineers, 2000. p. 125-136.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Walker, CK, Groppi, CE, d'Aubigny, CYD, Chen, G, Schieder, R, Narayanan, G, Lichtenberger, A & Siegel, P 2000, Far-infrared Array Receiver (FAR) for SOFIA. in Proceedings of SPIE - The International Society for Optical Engineering. vol. 4014, Society of Photo-Optical Instrumentation Engineers, pp. 125-136, Airborne Telescope Systems, Munich, Ger, 3/27/00.
Walker CK, Groppi CE, d'Aubigny CYD, Chen G, Schieder R, Narayanan G et al. Far-infrared Array Receiver (FAR) for SOFIA. In Proceedings of SPIE - The International Society for Optical Engineering. Vol. 4014. Society of Photo-Optical Instrumentation Engineers. 2000. p. 125-136
Walker, Christopher K ; Groppi, C. E. ; d'Aubigny, C. Y Drouet ; Chen, G. ; Schieder, R. ; Narayanan, G. ; Lichtenberger, A. ; Siegel, P. / Far-infrared Array Receiver (FAR) for SOFIA. Proceedings of SPIE - The International Society for Optical Engineering. Vol. 4014 Society of Photo-Optical Instrumentation Engineers, 2000. pp. 125-136
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