World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
101
Citations
49778
World Ranking
1569
National Ranking
831

Michael Endl publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Michael Endl sits on this spectrum.

103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103 publications 1,469+

This scientist: 492 publications — 55th percentile

55% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

Michael Endl D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Michael Endl sits on this spectrum.

70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70 D-Index 185+

This scientist: 101 D-Index — 58th percentile

58% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Overview

Michael Endl is affiliated with The University of Texas at Austin in the United States. Their research primarily focuses on physics and astronomy, contributing substantially to the field with 156 publications. Within this broad domain, their work is particularly concentrated in several subfields including astronomy and astrophysics, instrumentation, aerospace engineering, atomic and molecular physics and optics, as well as nuclear and high energy physics.

The scientist's research interests cover a range of topics related to stellar, planetary, and galactic studies, with an emphasis on astro and planetary science, astronomy and astrophysical research, and astrophysics and star formation studies. Other areas of investigation include gamma-ray bursts and supernovae, space exploration and technology, and adaptive optics and wavefront sensing.

Michael Endl has published research in several leading scientific venues. Frequent publication venues include:

  • The Astronomical Journal
  • arXiv (Cornell University)
  • The Astrophysical Journal Letters
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society

Their recent papers demonstrate a focus on planetary and stellar phenomena, featuring work such as:

  • Evidence for He i 10830 Å Absorption during the Transit of a Warm Neptune around the M-dwarf GJ 3470 with the Habitable-zone Planet Finder, 2020, The Astrophysical Journal
  • The Warm Neptune GJ 3470b Has a Polar Orbit, 2022, The Astrophysical Journal Letters
  • ARCES Observations of the TESS Circumbinary Planet TIC 172900988b, 2021, UA Campus Repository (The University of Arizona)
  • Kepler-1661 b: A Neptune-sized Kepler Transiting Circumbinary Planet around a Grazing Eclipsing Binary, 2020, The Astronomical Journal
  • A Warm Jupiter Transiting an M Dwarf: A TESS Single-transit Event Confirmed with the Habitable-zone Planet Finder, 2020, The Astronomical Journal

Michael Endl frequently collaborates with several co-authors who contribute extensively to their joint research efforts. Notable frequent co-authors include:

  • William D. Cochran (54 publications)
  • Joe P. Ninan (25 publications)
  • Suvrath Mahadevan (23 publications)
  • Guðmundur Stefánsson (22 publications)
  • Paul Robertson (22 publications)

Best Publications

  • Kepler Planet-Detection Mission: Introduction and First Results

    William J. Borucki;David Koch;Gibor Basri;Natalie Batalha

  • The Transiting Exoplanet Survey Satellite

    George R. Ricker;Joshua N. Winn;Roland Vanderspek;David W. Latham

  • Transiting Exoplanet Survey Satellite

    George R. Ricker;Joshua N. Winn;Roland Vanderspek;David Winslow Latham

  • Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data

    William J. Borucki;David G. Koch;Gibor Basri;Natalie Batalha

  • Transiting Exoplanet Survey Satellite (TESS)

    George R. Ricker;Joshua N. Winn;Roland Vanderspek;David W. Latham

  • Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data

    William J. Borucki;David G. Koch;Gibor Basri;Natalie Batalha

  • A terrestrial planet candidate in a temperate orbit around Proxima Centauri

    Guillem Anglada-Escudé;Pedro J. Amado;John Barnes;Zaira M. Berdiñas

  • Planet Occurrence within 0.25 AU of Solar-Type Stars from Kepler

    Andrew W. Howard;Geoffrey W. Marcy;Stephen T. Bryson;Jon M. Jenkins

  • Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets

    Geoffrey W. Marcy;Howard Isaacson;Andrew W. Howard;Jason F. Rowe

  • An abundance of small exoplanets around stars with a wide range of metallicities

    Lars A. Buchhave;David W. Latham;Anders Johansen;Martin Bizzarro

  • Masses, Radii, and Orbits of Small Kepler Planets: The Transition From Gaseous to Rocky Planets

    Geoffrey W. Marcy;Howard Isaacson;Andrew W. Howard;Jason F. Rowe

  • Sodium Absorption From the Exoplanetary Atmosphere of HD189733b Detected in the Optical Transmission Spectrum

    Seth Redfield;Michael Endl;William D. Cochran;Lars Koesterke

  • Emergence and frustration of magnetism with variable-range interactions in a quantum simulator.

    R. Islam;C. Senko;W. C. Campbell;S. Korenblit

  • Transiting circumbinary planets Kepler-34 b and Kepler-35 b

    William F. Welsh;Jerome A. Orosz;Joshua A. Carter;Daniel C. Fabrycky

  • Detection of a NEPTUNE-mass planet in the $ ho^{1}$ Cancri system using the Hobby-Eberly Telescope

    Barbara E. McArthur;Michael Endl;William D. Cochran;G. Fritz Benedict

  • Kepler-9: a system of multiple planets transiting a Sun-like star, confirmed by timing variations.

    Matthew J. Holman;Daniel C. Fabrycky;Darin Ragozzine;Eric B. Ford

  • Sodium Absorption from the Exoplanetary Atmosphere of HD 189733b Detected in the Optical Transmission Spectrum

    Seth Redfield;Michael Endl;William D. Cochran;Lars Koesterke

  • Detection of a NEPTUNE-mass planet in the $ρ^{1}$ Cancri system using the Hobby-Eberly Telescope

    Barbara E. McArthur;Michael Endl;William D. Cochran;G. Fritz Benedict

  • Characteristics of Kepler Planetary Candidates Based on the First Data Set

    William J. Borucki;David G. Koch;Gibor Basri;Natalie Batalha

  • Planet occurrence within 0.25AU of solar-type stars from Kepler

    Andrew W. Howard;Geoffrey W. Marcy;Stephen T. Bryson;Jon M. Jenkins

Frequent Co-Authors

William D. Cochran
William D. Cochran The University of Texas at Austin
Heike Rauer
Heike Rauer Freie Universität Berlin
Lars A. Buchhave
Lars A. Buchhave Technical University of Denmark
Jon M. Jenkins
Jon M. Jenkins Ames Research Center
Eric B. Ford
Eric B. Ford Pennsylvania State University
David W. Latham
David W. Latham Harvard University
Howard Isaacson
Howard Isaacson University of California, Berkeley
Geoffrey W. Marcy
Geoffrey W. Marcy University of California, Berkeley
Natalie M. Batalha
Natalie M. Batalha University of California, Santa Cruz
Jason F. Rowe
Jason F. Rowe Bishop's University

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