1956
DOI: 10.1021/ac60116a002
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Catalog of Infrared Spectra for Qualitative Analysis of Gases

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Cited by 296 publications
(70 citation statements)
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References 14 publications
(3 reference statements)
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“…Purification, ~vhen required, was therefore done by orthodox means. The spectrum of fresh azomethane mas generally identical with the published datum (6); impurities, when present, turned out to be an assortment of the various chlorinated n~ethanes. * Azomethane containing any absorption a t or above 13 p (methyl chloride, n~ethylene chloride, chloroform) was discarded; azoinethane with traces of carbon tetrachloride (absorption a t 12.6 ,u) was purified b y distillation a t dry ice temperature.…”
Section: Azometha?zesupporting
confidence: 65%
“…Purification, ~vhen required, was therefore done by orthodox means. The spectrum of fresh azomethane mas generally identical with the published datum (6); impurities, when present, turned out to be an assortment of the various chlorinated n~ethanes. * Azomethane containing any absorption a t or above 13 p (methyl chloride, n~ethylene chloride, chloroform) was discarded; azoinethane with traces of carbon tetrachloride (absorption a t 12.6 ,u) was purified b y distillation a t dry ice temperature.…”
Section: Azometha?zesupporting
confidence: 65%
“…[61] Chollet observed that the FVT of this material at 4008C/10 À3 hPa afforded a 15-20 % yield of 2-cyanopyrrole 31 as well as NO 2 as the only low molecular weight products (Scheme 10). [62] NO 2 was identified by its IR spectrum [63] in the gas-phase. Loss of NO 2 is not expected at such a low temperature under FVT conditions.…”
mentioning
confidence: 99%
“…In this paper, we used a low resolution spectrum of Arvesen et al (1969) for the infrared solar radiation density for convenience, because according to the high resolution spectra obtained by the ATMOS (Atmospheric Trace Molecule Spectroscopy) instrument on the Spacelab 3 mission, the solar infrared spectrum between 2800 and 3200 cm −1 does not contain significant absorption features (Farmer and Norton, 1989). For the combination bands, we present only very rough band intensities (Table 1), which were derived by looking at a lab C 2 H 6 spectrum of Pierson et al (1956), since the quantitative values are not available in the literature.…”
Section: Band Modelsmentioning
confidence: 99%