What is he best known for?
The fields of study he is best known for:
His scientific interests lie mostly in Radiative transfer, Spectral line, Atomic physics, Astrophysics and Stars.
His work deals with themes such as Wavelength and Fourier transform spectrometers, which intersect with Radiative transfer.
His Spectral line research integrates issues from Hyperfine structure, Solar observatory and Observatory.
His research integrates issues of Plasma parameters, Spectrometer, Plasma-enhanced chemical vapor deposition, Fluorescence and Emission intensity in his study of Atomic physics.
Within one scientific family, J. E. Lawler focuses on topics pertaining to Branching fraction under Fluorescence, and may sometimes address concerns connected to Laser-induced fluorescence.
In general Astrophysics study, his work on Stellar classification and Abundance of the chemical elements often relates to the realm of Point and Range, thereby connecting several areas of interest.
His most cited work include:
- Improved Laboratory Transition Probabilities for Ce II, Application to the Cerium Abundances of the Sun and Five r-process Rich, Metal-Poor Stars, and Rare Earth Lab Data (140 citations)
- the SDSS-III APOGEE Spectral Line List for H-Band Spectroscopy (129 citations)
- Atomic transition probabilities for Dy I and Dy II (112 citations)
What are the main themes of his work throughout his whole career to date?
His main research concerns Atomic physics, Radiative transfer, Astrophysics, Spectral line and Analytical chemistry.
J. E. Lawler has included themes like Ionization, Fluorescence and Absorption spectroscopy in his Atomic physics study.
In his study, Wavelength is inextricably linked to Ultraviolet, which falls within the broad field of Fluorescence.
His Radiative transfer study combines topics from a wide range of disciplines, such as Spectroscopy, Fourier transform spectrometers and Laser-induced fluorescence.
His Spectral line research is multidisciplinary, incorporating perspectives in Dysprosium, Solar observatory, Line, Spectrometer and H band.
His work in Analytical chemistry addresses issues such as Emission spectrum, which are connected to fields such as Plasma.
He most often published in these fields:
- Atomic physics (49.69%)
- Radiative transfer (28.83%)
- Astrophysics (19.02%)
What were the highlights of his more recent work (between 2011-2021)?
- Astrophysics (19.02%)
- Atomic physics (49.69%)
- Stars (11.66%)
In recent papers he was focusing on the following fields of study:
Astrophysics, Atomic physics, Stars, Radiative transfer and Analytical chemistry are his primary areas of study.
His work on Star, Arcturus, Galaxy and Nucleosynthesis as part of his general Astrophysics study is frequently connected to Vanadium, thereby bridging the divide between different branches of science.
J. E. Lawler works in the field of Atomic physics, namely Hyperfine structure.
The study incorporates disciplines such as Ionization equilibrium and Sigma in addition to Stars.
He combines subjects such as Spectroscopy, Fourier transform spectrometers and Branching fraction with his study of Radiative transfer.
His research investigates the link between Analytical chemistry and topics such as Neodymium that cross with problems in Spectral line.
Between 2011 and 2021, his most popular works were:
- the SDSS-III APOGEE Spectral Line List for H-Band Spectroscopy (129 citations)
- Improved Ti II log(gf) Values and Abundance Determinations in the Photospheres of the Metal-Poor Star HD 84937 (85 citations)
- Fe I OSCILLATOR STRENGTHS FOR TRANSITIONS FROM HIGH-LYING EVEN-PARITY LEVELS (69 citations)
In his most recent research, the most cited papers focused on:
His primary areas of investigation include Astrophysics, Radiative transfer, Nucleosynthesis, Spectral line and Branching fraction.
His study in the fields of Arcturus and Star under the domain of Astrophysics overlaps with other disciplines such as Scandium, Iron group and Sequence.
His work on Radiative transfer is being expanded to include thematically relevant topics such as Fourier transform spectrometers.
His work deals with themes such as Accretion and Galaxy, which intersect with Nucleosynthesis.
His Spectral line study incorporates themes from H band, Neodymium and Analytical chemistry.
His Branching fraction study is associated with Atomic physics.
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