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dc.creatorPearson, John C.en_US
dc.creatorYu, Shanshanen_US
dc.creatorGupta, Harshalen_US
dc.creatorDrouin, Brian J.en_US
dc.date.accessioned2011-07-12T17:30:55Z
dc.date.available2011-07-12T17:30:55Z
dc.date.issued2011en_US
dc.identifier2011-TC-05en_US
dc.identifier.urihttp://hdl.handle.net/1811/49434
dc.descriptionAuthor Institution: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109en_US
dc.description.abstractThe recent detection of HD$^{18}$O in Orion KL nderline{\textbf{521}}, (L20), 2010.} by the \emph{Herschel Space Observatory} provided a strong motivation to revisit the rotational spectrum in order to obtain more accurate calculations of transition frequencies. Rotational ransitions were recorded in the $300-2700$~GHz frequency range. Analysis of the combined microwave and infrared data sets with an Euler series Hamiltonian nderline{\textbf{233}} (174), 2005.} has facilitated determination of a set of precise rotational constants to support precision velocity measurements. The new rotational data also provides a means of evaluating the performance of the MARVEL algorithm used in the recent review of all available HDO data nderline{\textbf{111}}(2160), 2010.}.en_US
dc.language.isoenen_US
dc.publisherOhio State Universityen_US
dc.titleROTATIONAL SPECTROSCOPY OF HD$^{18}$Oen_US
dc.typeArticleen_US
dc.typeImageen_US
dc.typePresentationen_US


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