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dc.creatorFortman, Sarah M.en_US
dc.creatorMedvedev, Ivan R.en_US
dc.creatorNeese, Christopher F.en_US
dc.creatorDe Lucia, Frank C.en_US
dc.date.accessioned2009-07-29T12:46:48Z
dc.date.available2009-07-29T12:46:48Z
dc.date.issued2009en_US
dc.identifier2009-WH-05en_US
dc.identifier.urihttp://hdl.handle.net/1811/38126
dc.description"An experimental approach to the prediction of complete millimeter and submillimeter spectra at astrophysical temperatures: Applications to confusion-limited astrophysical observations," I. R. Medvedev and F. C. De Lucia, Ap. J. 656, 621-628 (2007).en_US
dc.descriptionAuthor Institution: Department of Physics, 191 W. Woodruff Ave., Ohio State University, Columbus, OH 43210 USAen_US
dc.description.abstractWe have previously reported on the experimental spectroscopic approach that makes possible the calculation of lower state energy levels and transition strengths without the need for spectral assignment . Analysis of the temperature dependent measurements significantly improves the estimate of the lower state energy, recovered by division of temperature dependent spectral intensities. Also, this approach provides results both in the standard astronomical catalog form (frequency, line strength, lower state energy) and as experimental temperature dependent spectra. We are reporting on temperature resolved \mbox{3-D} spectroscopy of ethyl cyanide --- a well known astronomical `weed'.en_US
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleTEMPERATURE RESOLVED 3-D SUBMILLIMETER SPECTROSCOPY OF ASTRONOMICAL `WEEDs'.en_US
dc.typeArticleen_US


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