What is he best known for?
The fields of study he is best known for:
- Astronomy
- Astrophysics
- Galaxy
Jason W. T. Hessels focuses on Astrophysics, Pulsar, Astronomy, Neutron star and Millisecond pulsar.
His study involves Fast radio burst, Galaxy, Telescope, Redshift and Green Bank Telescope, a branch of Astrophysics.
His Telescope research incorporates themes from LOFAR and Precision Array for Probing the Epoch of Reionization.
The study incorporates disciplines such as Gravitational wave, Radio telescope and X-ray binary in addition to Pulsar.
The concepts of his Millisecond pulsar study are interwoven with issues in Accretion, Millisecond, Binary star, Fermi Gamma-ray Space Telescope and Luminosity.
His Pulsar planet study in the realm of Binary pulsar connects with subjects such as Electromagnetic field.
His most cited work include:
- A two-solar-mass neutron star measured using Shapiro delay (2595 citations)
- A two-solar-mass neutron star measured using Shapiro delay (2595 citations)
- A massive pulsar in a compact relativistic binary (2268 citations)
What are the main themes of his work throughout his whole career to date?
His primary areas of investigation include Astrophysics, Pulsar, Astronomy, Millisecond pulsar and Neutron star.
His Astrophysics study focuses mostly on LOFAR, Radio telescope, Fast radio burst, Telescope and Galaxy.
The Canadian Hydrogen Intensity Mapping Experiment research Jason W. T. Hessels does as part of his general Fast radio burst study is frequently linked to other disciplines of science, such as Arecibo Observatory, therefore creating a link between diverse domains of science.
His Pulsar research incorporates elements of Fermi Gamma-ray Space Telescope, Gravitational wave and White dwarf.
His Millisecond pulsar research is multidisciplinary, incorporating elements of Globular cluster, X-ray binary, Galactic plane and Millisecond.
His research integrates issues of Accretion, Accretion, Roche lobe, Luminosity and Low Mass in his study of Neutron star.
He most often published in these fields:
- Astrophysics (142.80%)
- Pulsar (115.49%)
- Astronomy (74.32%)
What were the highlights of his more recent work (between 2018-2021)?
- Astrophysics (142.80%)
- Pulsar (115.49%)
- Fast radio burst (25.54%)
In recent papers he was focusing on the following fields of study:
Astrophysics, Pulsar, Fast radio burst, Neutron star and Radio telescope are his primary areas of study.
His Pulsar study is related to the wider topic of Astronomy.
His work in the fields of Astronomy, such as Milky Way and Interstellar medium, intersects with other areas such as Lightning, Spatiotemporal resolution and Natural phenomenon.
His Fast radio burst research incorporates themes from Supernova remnant, Afterglow and Circular polarization.
The Neutron star study combines topics in areas such as Ejecta, Kilonova, Solar mass, Mass ratio and Luminosity.
His work deals with themes such as Radio frequency, Radio astronomy and Observatory, which intersect with Radio telescope.
Between 2018 and 2021, his most popular works were:
- Fast radio bursts (231 citations)
- Fast radio bursts (231 citations)
- A repeating fast radio burst source localized to a nearby spiral galaxy (177 citations)
In his most recent research, the most cited papers focused on:
- Astronomy
- Astrophysics
- Milky Way
Jason W. T. Hessels focuses on Astrophysics, Fast radio burst, Pulsar, Canadian Hydrogen Intensity Mapping Experiment and Neutron star.
His work investigates the relationship between Astrophysics and topics such as Scattering that intersect with problems in Dispersion.
His Fast radio burst research includes elements of Magnetar, Telescope, Circular polarization and Nebula.
His study on Millisecond pulsar is often connected to Lorentz covariance as part of broader study in Pulsar.
Black hole, X-ray pulsar, Fermi Gamma-ray Space Telescope and Observatory is closely connected to Luminosity in his research, which is encompassed under the umbrella topic of Neutron star.
His Radio telescope study is concerned with the field of Astronomy as a whole.
This overview was generated by a machine learning system which analysed the scientist’s
body of work. If you have any feedback, you can
contact us
here.
