World's Best Scientists 2026 revealed!
Michael J. Hudson

Michael J. Hudson

D-Index & Metrics

Physics

D-Index
73
Citations
22205
World Ranking
3514
National Ranking
85

Overview

What is he best known for?

The fields of study he is best known for:

  • Galaxy
  • Astronomy
  • Milky Way

The scientist’s investigation covers issues in Astrophysics, Astronomy, Galaxy, Weak gravitational lensing and Redshift. His study in Dark energy, Dark matter, Cosmology, Supernova and Telescope falls under the purview of Astrophysics. His work focuses on many connections between Cosmology and other disciplines, such as COSMIC cancer database, that overlap with his field of interest in Pixel.

When carried out as part of a general Astronomy research project, his work on Wide Field Infrared Survey Telescope, Primary mirror, Planet and Angular resolution is frequently linked to work in Remote sensing, therefore connecting diverse disciplines of study. Hubble's law, Redshift survey and Galaxy cluster are among the areas of Galaxy where Michael J. Hudson concentrates his study. His study in Weak gravitational lensing is interdisciplinary in nature, drawing from both Dark matter halo, Photometric redshift and Galactic halo.

His most cited work include:

  • SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY (676 citations)
  • Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report (663 citations)
  • Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey (627 citations)

What are the main themes of his work throughout his whole career to date?

Michael J. Hudson focuses on Astrophysics, Galaxy, Astronomy, Redshift and Weak gravitational lensing. His work is connected to Dark matter, Galaxy cluster, Peculiar velocity, Star formation and Cosmology, as a part of Astrophysics. His work carried out in the field of Dark matter brings together such families of science as Halo and Gravitational lens.

His research in Cosmology intersects with topics in COSMIC cancer database and Cosmic microwave background. In his study, which falls under the umbrella issue of Redshift, Supernova is strongly linked to Universe. His research integrates issues of Cold dark matter and Galaxy group in his study of Weak gravitational lensing.

He most often published in these fields:

  • Astrophysics (150.69%)
  • Galaxy (125.86%)
  • Astronomy (76.55%)

What were the highlights of his more recent work (between 2016-2021)?

  • Galaxy (125.86%)
  • Astrophysics (150.69%)
  • Redshift (54.48%)

In recent papers he was focusing on the following fields of study:

His main research concerns Galaxy, Astrophysics, Redshift, Dark matter and Astronomy. Much of his study explores Galaxy relationship to Cosmology. Michael J. Hudson merges Astrophysics with Population in his study.

The Redshift study combines topics in areas such as Fundamental plane, Universe and Cosmic microwave background. In his study, Inference, Statistical physics, Bayesian probability and Mass distribution is strongly linked to Halo, which falls under the umbrella field of Dark matter. His study in the field of Telescope and Large Synoptic Survey Telescope is also linked to topics like Engineering.

Between 2016 and 2021, his most popular works were:

  • The Canada–France Imaging Survey: First Results from the u-Band Component (47 citations)
  • The Canada-France Imaging Survey: First results from the u-band component (47 citations)
  • The Weak Lensing Masses of Filaments between Luminous Red Galaxies (43 citations)

In his most recent research, the most cited papers focused on:

  • Galaxy
  • Milky Way
  • Astronomy

Michael J. Hudson mostly deals with Galaxy, Astrophysics, Astronomy, Milky Way and Redshift. His Halo, Reverberation mapping, Cold dark matter, Intergalactic travel and Dark energy investigations are all subjects of Astrophysics research. His Milky Way research focuses on Metallicity and how it connects with Blue straggler, Galactic anticenter, Dwarf galaxy, Galactic halo and Local Group.

His work on Redshift survey and Hubble's law as part of his general Redshift study is frequently connected to Amplitude, thereby bridging the divide between different branches of science. His Redshift survey research integrates issues from Star formation, Galaxy formation and evolution, Cosmic microwave background, Universe and Large Synoptic Survey Telescope. Michael J. Hudson interconnects Telescope, COSMIC cancer database, Cosmology, Metric expansion of space and Dark matter in the investigation of issues within Weak gravitational lensing.

Best Publications

  • Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

    D. Spergel;N. Gehrels;C. Baltay;D. Bennett

  • SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY

    A. Conley;A. Conley;J. Guy;M. Sullivan;N. Regnault

  • Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey

    A. Conley;J. Guy;M. Sullivan;N. Regnault

  • CFHTLenS: the Canada-France-Hawaii Telescope Lensing Survey

    Catherine Heymans;Ludovic Van Waerbeke;Lance Miller;Thomas Erben

  • CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments

    Catherine Heymans;Emma Grocutt;Alan Heavens;Martin Kilbinger

  • SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes

    M. Sullivan;J. Guy;A. Conley;N. Regnault

  • SNLS3: Constraints on dark energy combining the supernova legacy survey three-year data with other probes

    M. Sullivan;J. Guy;A. Conley;A. Conley;N. Regnault

  • Very weak lensing in the CFHTLS Wide: Cosmology from cosmic shear in the linear regime

    L. Fu;L. Fu;E. Semboloni;E. Semboloni;H. Hoekstra;M. Kilbinger;M. Kilbinger

  • CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products

    T. Erben;H. Hildebrandt;H. Hildebrandt;L. Miller;L. van Waerbeke

  • Bayesian galaxy shape measurement for weak lensing surveys – III. Application to the Canada–France–Hawaii Telescope Lensing Survey

    L. Miller;C. Heymans;T. D. Kitching;L. van Waerbeke

  • Consistently Large Cosmic Flows on Scales of 100 Mpc/h: a Challenge for the Standard LCDM Cosmology

    Richard Watkins;Hume A. Feldman;Michael J. Hudson

  • Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey

    A. Rest;D. Scolnic;R. J. Foley;M. E. Huber

  • CFHTLenS: combined probe cosmological model comparison using 2D weak gravitational lensing

    Martin Kilbinger;Liping Fu;Catherine Heymans;Fergus Simpson

  • NOAO Fundamental Plane Survey -- II. Age and Metallicity along the Red Sequence

    Jenica E. Nelan;Russell J. Smith;Michael J. Hudson;Gary A. Wegner

  • First Cosmic Shear Results from the Canada-France-Hawaii Telescope Wide Synoptic Legacy Survey

    H. Hoekstra;Y. Mellier;L. van Waerbeke;E. Semboloni

  • Consistently large cosmic flows on scales of 100 h−1 Mpc: a challenge for the standard ΛCDM cosmology

    Richard Watkins;Hume A. Feldman;Michael J. Hudson

  • CFHTLenS: Improving the quality of photometric redshifts with precision photometry

    H. Hildebrandt;T. Erben;K.H. Kuijken;L. van Waerbeke

  • Cosmological Constraints from Measurements of Type Ia Supernovae Discovered During the First 1.5 Yr of the Pan-STARRS1 Survey

    Armin Wolfgang Rest;D. Scolnic;R. J. Foley;R. J. Foley;M. E. Huber

  • NOAO fundamental plane survey II : age and metallicity along the red sequence from line-strength data.

    Jenica E. Nelan;Russell J. Smith;Michael J. Hudson;Gary A. Wegner

  • Cosmic flows in the nearby universe from Type Ia supernovae

    Stephen J. Turnbull;Michael J. Hudson;Michael J. Hudson;Hume A. Feldman;Malcolm Hicken

Frequent Co-Authors

Henk Hoekstra
Henk Hoekstra Leiden University
Catherine Heymans
Catherine Heymans University of Edinburgh
Lance Miller
Lance Miller University of Oxford
Konrad Kuijken
Konrad Kuijken Leiden University
Yannick Mellier
Yannick Mellier Institut d'Astrophysique de Paris
Terry J. Bridges
Terry J. Bridges Queen's University
Roger L. Davies
Roger L. Davies University of Oxford
H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
David J. Schlegel
David J. Schlegel Lawrence Berkeley National Laboratory
Raymond G. Carlberg
Raymond G. Carlberg University of Toronto

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