World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
81
Citations
20485
World Ranking
2963
National Ranking
18

Karin Lind 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 Karin Lind 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: 207 publications — 4th percentile

4% of scientists in this discipline score the same or lower.

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

Karin Lind 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 Karin Lind 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: 81 D-Index — 22nd percentile

22% of scientists in this discipline score the same or lower.

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

Overview

What is she best known for?

The fields of study she is best known for:

  • Astronomy
  • Astrophysics
  • Stars

Her primary areas of study are Astrophysics, Stars, Astronomy, Milky Way and Spectral line. Particularly relevant to Metallicity is her body of work in Astrophysics. Her Metallicity research includes themes of Disc and Galactic plane.

She has included themes like Ionization and Lithium in her Stars study. Her research in Abundance of the chemical elements and Galaxy are components of Astronomy. Her study in Milky Way is interdisciplinary in nature, drawing from both Star formation, Galaxy formation and evolution, Magnitude and Spectrograph.

Her most cited work include:

  • The Gaia-ESO Public Spectroscopic Survey (516 citations)
  • The GALAH survey: scientific motivation (426 citations)
  • Non-LTE calculations for neutral Na in late-type stars using improved atomic data (316 citations)

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

Karin Lind mainly investigates Astrophysics, Stars, Astronomy, Metallicity and Spectral line. Her research in the fields of Milky Way, Galaxy and Globular cluster overlaps with other disciplines such as Context and Population. Her Milky Way study incorporates themes from Data release and Radial velocity.

Her research investigates the connection between Stars and topics such as Spectroscopy that intersect with issues in Parallax. Karin Lind usually deals with Metallicity and limits it to topics linked to Disc and Thin disk. Karin Lind studied Spectral line and Line that intersect with Atomic physics.

She most often published in these fields:

  • Astrophysics (118.04%)
  • Stars (111.34%)
  • Astronomy (50.00%)

What were the highlights of her more recent work (between 2019-2021)?

  • Stars (111.34%)
  • Astrophysics (118.04%)
  • Galaxy (29.38%)

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

Her primary areas of investigation include Stars, Astrophysics, Galaxy, Metallicity and Milky Way. Her Stars research includes elements of Radius, Spectrograph, Telescope and Supernova. Astrophysics connects with themes related to Spectral line in her study.

In general Spectral line study, her work on Arcturus often relates to the realm of Wavelength, thereby connecting several areas of interest. Her Milky Way study combines topics from a wide range of disciplines, such as Spectroscopy and Halo. Her Halo research incorporates themes from Globular cluster and Big Bang nucleosynthesis.

Between 2019 and 2021, her most popular works were:

  • The GALAH+ Survey: Third Data Release (16 citations)
  • The GALAH survey: Temporal chemical enrichment of the galactic disc (14 citations)
  • The GALAH survey: Temporal chemical enrichment of the galactic disc (14 citations)

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

  • Astronomy
  • Milky Way
  • Galaxy

Her main research concerns Stars, Astrophysics, Milky Way, Data release and Halo. Her Stars study frequently links to related topics such as Spectral line. Her studies deal with areas such as Line and Hyperfine structure, Atomic physics as well as Spectral line.

Her Halo study combines topics in areas such as Chemical element, Spectroscopy and Bulge. Her Metallicity research is multidisciplinary, incorporating elements of Radius, Sigma and Velocity dispersion. Her studies in Star formation integrate themes in fields like Supernova, Hydrostatic equilibrium and Neutron star.

Best Publications

  • The Gaia-ESO Public Spectroscopic Survey

    G. Gilmore;S. Randich;M. Asplund;J. Binney

  • The GALAH survey: scientific motivation

    G.M. De Silva;G.M. De Silva;K.C. Freeman;J. Bland-Hawthorn;S. Martell

  • Non‐LTE line formation of Fe in late‐type stars – I. Standard stars with 1D and 〈3D〉 model atmospheres

    Maria Bergemann;Karin Lind;R Collet;Zazralt Magic

  • Non-LTE line formation of Fe in late-type stars - II. 1D spectroscopic stellar parameters

    Karin Lind;Maria Bergemann;Martin Asplund

  • NLTE line formation of Fe in late-type stars II: 1D spectroscopic stellar parameters

    Karin Lind;Maria Bergemann;Martin Asplund

  • NLTE line formation of Fe for late-type stars. I. Standard stars with 1D and model atmospheres

    Maria Bergemann;Karin Lind;Remo Collet;Zazralt Magic

  • The GALAH+ survey: Third data release

    Sven Buder;Sven Buder;Sanjib Sharma;Janez Kos;Anish M. Amarsi

  • Non-LTE calculations for neutral Na in late-type stars using improved atomic data

    Karin Lind;Martin Asplund;Paul S Barklem;A. Belyaev

  • A single low-energy, iron-poor supernova as the source of metals in the star SMSS J031300.36−670839.3

    Stefan C. Keller;M. S. Bessell;Anna L. Frebel;Andrew R. Casey

  • Gaia FGK Benchmark Stars - Metallicity

    Paula Jofre;U. Heiter;C. Soubiran;S. Blanco-Cuaresma

  • The GALAH Survey: Second Data Release

    Sven Buder;Sven Buder;Martin Asplund;Ly Duong;Janez Kos

  • Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC 6397 ,

    K Lind;Francesca Primas;C Charbonnel;Frank Grundahl

  • Departures from LTE for neutral Li in late-type stars

    K Lind;Martin Asplund;Paul S Barklem

  • Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

    R. Smiljanic;A. J. Korn;M. Bergemann;A. Frasca

  • The Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

    A. Recio-Blanco;P. de Laverny;G. Kordopatis;A. Helmi

  • The Gaia-ESO Survey: radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk

    M. Bergemann;G. Ruchti;A. Serenelli;S. Feltzing

  • Gaia FGK benchmark stars: Metallicity

    P. Jofre;P. Jofre;Ulrike Heiter;C. Soubiran;S. Blanco-Cuaresma

  • The Gaia-ESO Survey: the analysis of high-resolution UVES spectra of FGK-type stars

    R. Smiljanic;A. J. Korn;M. Bergemann;A. Frasca

  • The Gaia-ESO Survey: the Galactic thick to thin disc transition

    A. Recio-Blanco;P. de Laverny;G. Kordopatis;Amina Helmi

  • The Gaia-ESO Survey : radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk

    M. Bergemann;G.R. Ruchti;A.M. Serenelli;S. Feltzing

Frequent Co-Authors

Martin Asplund
Martin Asplund Australian National University
Joss Bland-Hawthorn
Joss Bland-Hawthorn University of Sydney
Daniel B. Zucker
Daniel B. Zucker Macquarie University
Laura Magrini
Laura Magrini National Institute for Astrophysics
Dennis Stello
Dennis Stello University of New South Wales
Sofia Randich
Sofia Randich National Institute for Astrophysics
Sergey E. Koposov
Sergey E. Koposov University of Edinburgh
Kenneth C. Freeman
Kenneth C. Freeman Australian National University
Geraint F. Lewis
Geraint F. Lewis University of Sydney
Gerard Gilmore
Gerard Gilmore University of Cambridge

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