World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
107
Citations
74156
World Ranking
1272
National Ranking
666

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Galaxy
  • Milky Way

Huan Lin mainly focuses on Astrophysics, Galaxy, Astronomy, Sky and Redshift. His study in Stars, Quasar, Photometry, Dark energy and Gravitational wave is carried out as part of his Astrophysics studies. His research in Dark energy intersects with topics in Redshift-space distortions and Cosmic microwave background.

Huan Lin studied Astronomy and Library science that intersect with Gemini Observatory. His work on Celestial equator and Data release is typically connected to Imaging data and Spectral density as part of general Sky study, connecting several disciplines of science. Huan Lin interconnects Luminosity and Supernova in the investigation of issues within Redshift.

His most cited work include:

  • The Seventh Data Release of the Sloan Digital Sky Survey (4732 citations)
  • Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies (3620 citations)
  • Cosmological parameters from SDSS and WMAP (3312 citations)

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

The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Astronomy and Dark energy. His Sky, Quasar, Weak gravitational lensing, Galaxy cluster and Photometric redshift investigations are all subjects of Astrophysics research. Many of his research projects under Sky are closely connected to Imaging data with Imaging data, tying the diverse disciplines of science together.

His Galaxy research is multidisciplinary, relying on both Stars and Photometry. His work on Hubble's law as part of his general Redshift study is frequently connected to Population, thereby bridging the divide between different branches of science. His Dark energy research includes elements of Telescope, Cosmic microwave background, Dark matter and Supernova.

He most often published in these fields:

  • Astrophysics (88.59%)
  • Galaxy (59.73%)
  • Redshift (50.00%)

What were the highlights of his more recent work (between 2015-2021)?

  • Astrophysics (88.59%)
  • Dark energy (37.92%)
  • Redshift (50.00%)

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

His primary areas of investigation include Astrophysics, Dark energy, Redshift, Galaxy and Astronomy. The various areas that Huan Lin examines in his Dark energy study include Telescope, Sky, Weak gravitational lensing, Cosmic microwave background and Dark matter. His research integrates issues of Magnitude and Remote sensing in his study of Sky.

The Redshift study combines topics in areas such as Planck, Stellar mass, Galaxy cluster and Photometry. He combines subjects such as Lens and Data set with his study of Galaxy. His study in the field of Einstein radius, Strong gravitational lensing and Radius also crosses realms of European research.

Between 2015 and 2021, his most popular works were:

  • Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing (670 citations)
  • The DESI Experiment Part I: Science,Targeting, and Survey Design (545 citations)
  • The Dark Energy Survey: more than dark energy - an overview (513 citations)

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

  • Astronomy
  • Galaxy
  • Milky Way

Huan Lin spends much of his time researching Astrophysics, Dark energy, Galaxy, Redshift and Astronomy. His work in Astrophysics covers topics such as Cosmic microwave background which are related to areas like Universe. The study incorporates disciplines such as Weak gravitational lensing and Photometric redshift in addition to Dark energy.

Huan Lin works in the field of Galaxy, namely Redshift survey. His work carried out in the field of Redshift brings together such families of science as Luminosity and Quasar. The Photometry research he does as part of his general Astronomy study is frequently linked to other disciplines of science, such as European research, Fundamental physics and European union, therefore creating a link between diverse domains of science.

Best Publications

  • The Seventh Data Release of the Sloan Digital Sky Survey

    Kevork N. Abazajian;Jennifer K. Adelman-Mccarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam

  • Cosmological parameters from SDSS and WMAP

    Max Tegmark;Max Tegmark;Michael Abram Strauss;Michael R. Blanton;Kevork Abazajian

  • Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies

    Daniel J. Eisenstein;Daniel J. Eisenstein;Idit Zehavi;David W. Hogg;Roman Scoccimarro

  • The Sixth Data Release of the Sloan Digital Sky Survey

    Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam;Carlos Allende Prieto

  • The fourth data release of the Sloan Digital Sky Survey

    Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam;Kurt S.J. Anderson

  • The Fifth Data Release of the Sloan Digital Sky Survey

    Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam;Kurt S.J. Anderson

  • THE THREE-DIMENSIONAL POWER SPECTRUM OF GALAXIES FROM THE SLOAN DIGITAL SKY SURVEY

    Max Tegmark;Michael R. Blanton;Michael A. Strauss;Fiona Hoyle

  • The 3D power spectrum of galaxies from the SDSS

    M Tegmark;M Blanton;M Strauss;F Hoyle

  • Cosmological constraints from the SDSS luminous red galaxies

    Max Tegmark;Daniel J. Eisenstein;Michael A. Strauss;David H. Weinberg

  • The Second Data Release of the Sloan Digital Sky Survey

    Kevork Abazajian;Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam

  • Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

    J. Abadie;B. P. Abbott

  • Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing

    T. M. C. Abbott;F. B. Abdalla;A. Alarcon;J. Aleksić

  • The first data release of the sloan digital sky survey

    Kevork Abazajian;Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam

  • SEGUE: A SPECTROSCOPIC SURVEY OF 240,000 STARS WITH g = 14-20

    Brian Yanny;Constance Rockosi;Heidi Jo Newberg;Gillian R. Knapp

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

    P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger

  • The Third Data Release of the Sloan Digital Sky Survey

    Kevork Abazajian;Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam

  • The Dark Energy Survey: more than dark energy - an overview

    T. Abbott;F. B. Abdalla;J. Aleksić

  • An efficient targeting strategy for multiobject spectrograph surveys: The Sloan digital sky survey "tiling" algorithm

    Michael R. Blanton;Michael R. Blanton;Huan Lin;Robert H. Lupton;F. Miller Maley

  • An Efficient Algorithm for Positioning Tiles in the Sloan Digital Sky Survey

    M. R. Blanton;R. H. Lupton;F. Miller Maley;N. Young

  • The DESI Experiment Part I: Science,Targeting, and Survey Design

    Amir Aghamousa;Jessica Aguilar;Steve Ahlen

Frequent Co-Authors

Joshua A. Frieman
Joshua A. Frieman University of Chicago
Robert A. Gruendl
Robert A. Gruendl University of Illinois at Urbana-Champaign
B. Flaugher
B. Flaugher Fermilab
Marcelle Soares-Santos
Marcelle Soares-Santos Brandeis University
D. L. Burke
D. L. Burke Stanford University
K. Honscheid
K. Honscheid The Ohio State University
A. Roodman
A. Roodman Stanford University

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