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Karin Lind

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 81 2963 2813 17 17 207 20485

Karin Lind publications per year

The chart shows the history of publications by Karin Lind between 1983 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Karin Lind published across 39 years, from 1983 to 2021, averaging 4.9 papers a year. Output peaked at 23 publications in 2015. 38 of the 192 publications appeared in the last two years.

No. of publications
5 10 15 20
Bar chart. Horizontal axis: year, 1983 to 2021. Vertical axis: number of publications, 0 to 23. Peak 23 publications in 2015. 1983: 1 publication 1984: 0 publications 1985: 0 publications 1986: 0 publications 1987: 0 publications 1988: 0 publications 1989: 0 publications 1990: 0 publications 1991: 0 publications 1992: 0 publications 1993: 0 publications 1994: 0 publications 1995: 0 publications 1996: 0 publications 1997: 1 publication 1998: 1 publication 1999: 1 publication 2000: 1 publication 2001: 0 publications 2002: 0 publications 2003: 0 publications 2004: 0 publications 2005: 0 publications 2006: 0 publications 2007: 0 publications 2008: 2 publications 2009: 5 publications 2010: 1 publication 2011: 9 publications 2012: 17 publications 2013: 9 publications 2014: 22 publications 2015: 23 publications 2016: 13 publications 2017: 10 publications 2018: 20 publications 2019: 18 publications 2020: 15 publications 2021: 23 publications
1983 2021

192 publications in total across all disciplines

View publications per year as a table
Karin Lind: publications per year, 1983 to 2021
Year Publications
1983 1
1984 0
1985 0
1986 0
1987 0
1988 0
1989 0
1990 0
1991 0
1992 0
1993 0
1994 0
1995 0
1996 0
1997 1
1998 1
1999 1
2000 1
2001 0
2002 0
2003 0
2004 0
2005 0
2006 0
2007 0
2008 2
2009 5
2010 1
2011 9
2012 17
2013 9
2014 22
2015 23
2016 13
2017 10
2018 20
2019 18
2020 15
2021 23
Total 192
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Karin Lind publications per year - data summary

  • Karin Lind, a Physics scholar from Stockholm University, has 192 publications recorded across 39 years, from 1983 to 2021.
  • The oldest publication on record dates to 1983 and the most recent to 2021.
  • The most productive years are 2015 and 2021, with 23 publications each.
  • The least productive years with any output are 1983, 1997, 1998, 1999 and others, with 1 publication each.
  • 20 of the 39 years in the span carry no publications at all (1984, 1985, 1986, 1987 and others).
  • The rate of publication averages 4.9 papers per year over the whole span, or 10.1 per year counting only the 19 years with at least one publication.
  • The last 5 years on the chart (2017-2021) hold 86 publications, 45% of the career total.
  • Split into equal eras - 1983-1995: 1 publication (0.1 per year); 1996-2008: 6 publications (0.5 per year); 2009-2021: 185 publications (14.2 per year).
  • Comparing the opening and closing eras, the overall trend of publication is rising.

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.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 203–222 publications, is where this scientist sits. 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
103–122 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.

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31
163–182 35
183–202 53
203–222 81 207
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
Download as CSV

Karin Lind publication distribution in Physics in 2026 - data summary

  • The chart plots the publication count of all 3,678 Physics scientists ranked by Research.com in 2026, grouped into 70 ranges running from 103–122 to 1,469+ publications.
  • Karin Lind, a Physics scholar from Stockholm University, records 207 publications - the 4th percentile of the discipline.
  • 4% of ranked Physics scientists score the same or lower than Karin Lind, and about 96% score higher.
  • The median of the discipline falls in the 463–482 publications range, and Karin Lind ranks below the median.
  • The most crowded range is 323–342 publications, holding 162 scientists (4% of the field).
  • 49% of the field sits in the lowest quarter of the value range (up to 443–462 publications), so the distribution leans towards the lower end of the scale.
  • The final bar has no upper bound: it groups every scientist with 1,469 publications or more, 100 scientists in all (3% of the field).

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.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 80–81 D-Index, is where this scientist sits. 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
70–71 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.

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153
78–79 144
80–81 167 81
82–83 167
84–85 166
86–87 132
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60
122–123 59
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
Download as CSV

Karin Lind D-index placement in Physics in 2026 - data summary

  • The chart plots the discipline H-index (D-index) of all 3,678 Physics scientists ranked by Research.com in 2026, grouped into 59 ranges running from 70–71 to 185+ D-Index.
  • Karin Lind, a Physics scholar from Stockholm University, records 81 D-Index - the 22nd percentile of the discipline.
  • 22% of ranked Physics scientists score the same or lower than Karin Lind, and about 78% score higher.
  • The median of the discipline falls in the 96–97 D-Index range, and Karin Lind ranks below the median.
  • The most crowded range is 80–81 D-Index, holding 167 scientists (5% of the field).
  • 55% of the field sits in the lowest quarter of the value range (up to 98–99 D-Index), so the distribution is heavily right-skewed and high scores are rare.
  • The final bar has no upper bound: it groups every scientist with 185 D-Index or more, 99 scientists in all (3% of the field).

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

External Links

Personal website of Karin Lind

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Best Scientists Citing Karin Lind

Timothy C. Beers

Timothy C. Beers

University of Notre Dame

Publications: 159

A. Bragaglia

A. Bragaglia

National Institute for Astrophysics

Publications: 141

Martin Asplund

Martin Asplund

Australian National University

Publications: 131

Sofia Randich

Sofia Randich

National Institute for Astrophysics

Publications: 123

Anna Frebel

Anna Frebel

MIT

Publications: 114

Jorge Melendez

Jorge Melendez

Universidade de São Paulo

Publications: 113

Antonino Milone

Antonino Milone

University of Padua

Publications: 102

Carlos Allende Prieto

Carlos Allende Prieto

University of La Laguna

Publications: 100

Laura Magrini

Laura Magrini

National Institute for Astrophysics

Publications: 95

Piercarlo Bonifacio

Piercarlo Bonifacio

Université Paris Cité

Publications: 91

Matthew Shetrone

Matthew Shetrone

The University of Texas at Austin

Publications: 85

Santi Cassisi

Santi Cassisi

National Institute for Astrophysics

Publications: 84

Giovanni Carraro

Giovanni Carraro

University of Padua

Publications: 82

Joss Bland-Hawthorn

Joss Bland-Hawthorn

University of Sydney

Publications: 80

Gerard Gilmore

Gerard Gilmore

University of Cambridge

Publications: 80

Sergey E. Koposov

Sergey E. Koposov

University of Edinburgh

Publications: 78

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