1997
DOI: 10.1063/1.1147970
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A fast scan submillimeter spectroscopic technique

Abstract: A new fast scan submillimeter spectroscopic technique ͑FASSST͒ has been developed which uses a voltage tunable backward wave oscillator ͑BWO͒ as a primary source of radiation, but which uses fast scan (ϳ10 5 Doppler limited resolution elements/s͒ and optical calibration methods rather than the more traditional phase or frequency lock techniques. Among its attributes are ͑1͒ absolute frequency calibration to ϳ1/10 of a Doppler limited gaseous absorption linewidth (Ͻ0.1 MHz, 0.000 003 cm Ϫ1 ), ͑2͒ high sensitivi… Show more

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Cited by 149 publications
(80 citation statements)
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“…The spectra were recorded using the Fast Scan Submillimeter Spectroscopic Technique (FASSST; Medvedev et al 2004;Petkie et al 1997). In the implementation used here a times 48 solid state multiplier chain (Virginia Diodes) was driven by a rapidly sweeping (Agilent E8256D) synthesizer.…”
Section: Methodsmentioning
confidence: 99%
“…The spectra were recorded using the Fast Scan Submillimeter Spectroscopic Technique (FASSST; Medvedev et al 2004;Petkie et al 1997). In the implementation used here a times 48 solid state multiplier chain (Virginia Diodes) was driven by a rapidly sweeping (Agilent E8256D) synthesizer.…”
Section: Methodsmentioning
confidence: 99%
“…The millimeter-and submillimeter-wave spectrum of 13 C 1 -methyl formate in the 110Y377 GHz region was measured with the FASSST system ( Petkie et al 1997;Albert et al 1998;Medvedev et al 2004) using three different backward-wave oscillators as sources of radiation. The spectrum of sulfur dioxide was used as reference to calibrate the frequencies.…”
Section: Experimental Considerationsmentioning
confidence: 99%
“…Particularly desired would be narrowband tunable sources to study low-frequency vibrations of polyatomic molecules and molecular clusters, and the rotational motion of small molecules (see, for instance, Refs. [6][7][8][9][10][11] and references therein), and in the identification of possible molecular carriers of astrophysical spectra, for which there is considerable current interest in the context of the new observational facilities ALMA [12] and Herschel [13].…”
Section: Introductionmentioning
confidence: 99%