The measurement of lifetimes using laser-induced fluorescence at the University of Wisconsin-Madison has been one of the most productive experiments in the measurement of atomic spectroscopic data. The NIST bibliographic database on Atomic Transition Probabilities lists over 60 papers with Jim Lawler as an author or coauthor on lifetimes of neutral and singly-ionized elements ranging from carbon to mercury. The applications of these measurements range from astrophysics to lighting research. However, it is necessary to combine these lifetimes with branching fractions in order to obtain the atomic transition probabilities, and these branching fractions are now frequently the limiting factor in the accuracy of the measurements. I shall describ...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
Much progress has been made in the measurement of oscillator strengths in neutral and singly-ionized...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...
In this talk I will describe the laboratory astrophysics program of the Jim Lawler group at the Univ...
The focus of this work is on the experimental techniques and data analysis in atomic spectroscopy. I...
A widely used method for determination of transition probabilities and oscillator strengths is based...
We propose a laser induced sensitized fluorescence spectrometry for measuring the spontaneous emissi...
Abstract. The use of lifetime measurements for the specification of transition probabilities along i...
We present an overview of current needs for accurate laboratory atomic transition probabilities (log...
Fourier transform spectroscopy has proven to be a useful tool when measuring wavelengths and branchi...
The critical data compilation work as well as the bibliographical efforts of two data centers on ato...
We have started a systematic investigation of the radiative properties of the elements of the sixth ...
Accurate atomic parameters, such as transition probabilities, wavelengths, and energy levels, are in...
Fourier transform spectroscopy has proven to be a useful toot when measuring wavelengths and branchi...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
Much progress has been made in the measurement of oscillator strengths in neutral and singly-ionized...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...
In this talk I will describe the laboratory astrophysics program of the Jim Lawler group at the Univ...
The focus of this work is on the experimental techniques and data analysis in atomic spectroscopy. I...
A widely used method for determination of transition probabilities and oscillator strengths is based...
We propose a laser induced sensitized fluorescence spectrometry for measuring the spontaneous emissi...
Abstract. The use of lifetime measurements for the specification of transition probabilities along i...
We present an overview of current needs for accurate laboratory atomic transition probabilities (log...
Fourier transform spectroscopy has proven to be a useful tool when measuring wavelengths and branchi...
The critical data compilation work as well as the bibliographical efforts of two data centers on ato...
We have started a systematic investigation of the radiative properties of the elements of the sixth ...
Accurate atomic parameters, such as transition probabilities, wavelengths, and energy levels, are in...
Fourier transform spectroscopy has proven to be a useful toot when measuring wavelengths and branchi...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
Much progress has been made in the measurement of oscillator strengths in neutral and singly-ionized...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...