A computer accessible catalogue of submillimeter, millimeter, and microwave spectral lines in the frequency range between O and 3000 GHz (such as; wavelengths longer than 100 m) is discussed. The catalogue was used as a planning guide and as an aid in the identification and analysis of observed spectral lines. The information listed for each spectral line includes the frequency and its estimated error, the intensity, lower state energy, and quantum number assignment. The catalogue was constructed by using theoretical least squares fits of published spectral lines to accepted molecular models. The associated predictions and their estimated errors are based upon the resultant fitted parameters and their covariances
Context. A discharge of nitrogen gas, as created in a microwave-induced plasma, exhibits a very dens...
The advent of large instantaneous bandwidth receivers and high spectral resolution spectro...
We have made accurate calculations of recombination lines of H, He, C, and S from 100 GHz to 10 ?m (...
A computer accessible catalogue of submillimeter, millimeter and microwave spectral lines in the fre...
A computer-accessible catalog of submillimeter, millimeter, and microwave spectral lines in the freq...
AbstractÐThis paper describes a computer-accessible catalog of submillimeter, millimeter, and microw...
Author Institution: Jet Propulsion Laboratory, California Institute of TechnologyThe Jet Propulsion ...
The spectrum of most known astrophysical molecules is derived from transitions between a few hundred...
Author Institution: Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 9110...
none3Unambiguous identification of observed molecular spectral lines is critical for the scientific ...
[[abstract]]The length of wave of radiations, which was released by the transition of gas-phase mole...
A molecular line survey is a study of the spectrum of an astronomical source over a wide, approximat...
none3Unambiguous identification of observed molecular spectral lines is critical for the scientific ...
A spectral line survey of the OMC1 cloud core has been obtained, over the frequency range 257.04-273...
Author Institution: National Bureau of StandardsA program for the critical evaluation of microwave s...
Context. A discharge of nitrogen gas, as created in a microwave-induced plasma, exhibits a very dens...
The advent of large instantaneous bandwidth receivers and high spectral resolution spectro...
We have made accurate calculations of recombination lines of H, He, C, and S from 100 GHz to 10 ?m (...
A computer accessible catalogue of submillimeter, millimeter and microwave spectral lines in the fre...
A computer-accessible catalog of submillimeter, millimeter, and microwave spectral lines in the freq...
AbstractÐThis paper describes a computer-accessible catalog of submillimeter, millimeter, and microw...
Author Institution: Jet Propulsion Laboratory, California Institute of TechnologyThe Jet Propulsion ...
The spectrum of most known astrophysical molecules is derived from transitions between a few hundred...
Author Institution: Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 9110...
none3Unambiguous identification of observed molecular spectral lines is critical for the scientific ...
[[abstract]]The length of wave of radiations, which was released by the transition of gas-phase mole...
A molecular line survey is a study of the spectrum of an astronomical source over a wide, approximat...
none3Unambiguous identification of observed molecular spectral lines is critical for the scientific ...
A spectral line survey of the OMC1 cloud core has been obtained, over the frequency range 257.04-273...
Author Institution: National Bureau of StandardsA program for the critical evaluation of microwave s...
Context. A discharge of nitrogen gas, as created in a microwave-induced plasma, exhibits a very dens...
The advent of large instantaneous bandwidth receivers and high spectral resolution spectro...
We have made accurate calculations of recombination lines of H, He, C, and S from 100 GHz to 10 ?m (...