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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 91 2142 2036 1092 1020 209 44610

Shy Genel publications per year

The chart shows the history of publications by Shy Genel between 2008 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Shy Genel published across 19 years, from 2008 to 2026, averaging 13.7 papers a year. Output peaked at 28 publications in 2021. 23 of the 260 publications appeared in the last two years.

No. of publications
5 10 15 20 25
Bar chart. Horizontal axis: year, 2008 to 2026. Vertical axis: number of publications, 0 to 28. Peak 28 publications in 2021. 2008: 7 publications 2009: 8 publications 2010: 6 publications 2011: 5 publications 2012: 7 publications 2013: 10 publications 2014: 10 publications 2015: 22 publications 2016: 10 publications 2017: 8 publications 2018: 22 publications 2019: 23 publications 2020: 16 publications 2021: 28 publications 2022: 19 publications 2023: 19 publications 2024: 17 publications 2025: 20 publications 2026: 3 publications
2008 2026

260 publications in total across all disciplines

View publications per year as a table
Shy Genel: publications per year, 2008 to 2026
Year Publications
2008 7
2009 8
2010 6
2011 5
2012 7
2013 10
2014 10
2015 22
2016 10
2017 8
2018 22
2019 23
2020 16
2021 28
2022 19
2023 19
2024 17
2025 20
2026 3
Total 260
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Shy Genel 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 Shy Genel 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: 209 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 81 209
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
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Shy Genel 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 Shy Genel 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, 90–91 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: 91 D-Index — 42nd percentile

42% 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
82–83 167
84–85 166
86–87 132
88–89 155
90–91 134 91
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
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Overview

Shy Genel is affiliated with Columbia University in the United States and has a significant body of research in physics and astronomy, particularly focusing on galaxy formation, evolution, and astrophysical phenomena. Their scholarly output includes over two hundred publications primarily in the fields of astronomy and astrophysics.

The scientist's research encompasses various subfields including astronomy and astrophysics, instrumentation, artificial intelligence, nuclear and high energy physics, and computer vision and pattern recognition. Their work often intersects with topics involving galaxies' formation, evolution, and phenomena, as well as broader aspects of cosmology and gravitation theories. Other thematic areas include stellar, planetary, and galactic studies, computational physics with Python applications, and star formation studies.

Frequent publication venues for Genel's work are diverse but largely concentrated in well-regarded journals such as arXiv (Cornell University) with 41 publications, The Astrophysical Journal (34 publications), and the Monthly Notices of the Royal Astronomical Society (16 publications). Additional research appears in The Astrophysical Journal Supplement Series and Astronomy and Astrophysics.

Recent papers authored or co-authored by Genel demonstrate a focus on black hole astrophysics and galactic evolution. Notable articles include:

  • The relationship between black hole mass and galaxy properties: examining the black hole feedback model in IllustrisTNG, 2020, Monthly Notices of the Royal Astronomical Society
  • Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing, 2020, Monthly Notices of the Royal Astronomical Society
  • Supermassive black holes in cosmological simulations I: MBH − M⋆ relation and black hole mass function, 2021, Monthly Notices of the Royal Astronomical Society
  • The diversity and variability of star formation histories in models of galaxy evolution, 2020, Monthly Notices of the Royal Astronomical Society
  • Supermassive black holes in cosmological simulations - II: the AGN population and predictions for upcoming X-ray missions, 2021, Monthly Notices of the Royal Astronomical Society

General collaborates extensively, with frequent co-authors including Francisco Villaescusa-Navarro, Daniel Anglés-Alcázar, Lars Hernquist, Mark Vogelsberger, and Rachel S. Somerville. These collaborations reflect a network deeply engaged in computational and theoretical astrophysics.

Best Publications

  • Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe

    Mark Vogelsberger;Shy Genel;Volker Springel;Volker Springel;Paul Torrey

  • Simulating galaxy formation with the IllustrisTNG model

    Annalisa Pillepich;Annalisa Pillepich;Volker Springel;Volker Springel;Dylan Nelson;Shy Genel;Shy Genel

  • First results from the IllustrisTNG simulations: matter and galaxy clustering

    Volker Springel;Volker Springel;Rüdiger Pakmor;Annalisa Pillepich;Rainer Weinberger

  • First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

    Annalisa Pillepich;Annalisa Pillepich;Dylan Nelson;Lars Hernquist;Volker Springel;Volker Springel

  • Properties of galaxies reproduced by a hydrodynamic simulation

    Mark Vogelsberger;Shy Genel;Volker Springel;Volker Springel;Paul Torrey

  • First results from the IllustrisTNG simulations: the galaxy colour bimodality

    Dylan Nelson;Annalisa Pillepich;Volker Springel;Volker Springel;Rainer Weinberger

  • THE SINS SURVEY: SINFONI INTEGRAL FIELD SPECTROSCOPY OF z ∼ 2 STAR-FORMING GALAXIES*

    N. M. Förster Schreiber;R. Genzel;N. Bouché;G. Cresci

  • Submillimeter Galaxies at z~2: Evidence for Major Mergers & Constraints on Lifetimes, IMF and CO-H2 Conversion Factor

    L.J. Tacconi;R. Genzel;I. Smail;R. Neri

  • Introducing the Illustris Project: the evolution of galaxy populations across cosmic time

    Shy Genel;Mark Vogelsberger;Volker Springel;Volker Springel;Debora Sijacki

  • The IllustrisTNG simulations: public data release

    Dylan Nelson;Volker Springel;Volker Springel;Volker Springel;Annalisa Pillepich;Vicente Rodriguez-Gomez

  • First results from the IllustrisTNG simulations: a tale of two elements - chemical evolution of magnesium and europium

    Jill P. Naiman;Annalisa Pillepich;Volker Springel;Enrico Ramirez-Ruiz

  • Simulating galaxy formation with black hole driven thermal and kinetic feedback

    Rainer Weinberger;Volker Springel;Volker Springel;Lars Hernquist;Annalisa Pillepich;Annalisa Pillepich

  • First results from the IllustrisTNG simulations: radio haloes and magnetic fields

    Federico Marinacci;Mark Vogelsberger;Rüdiger Pakmor;Paul Torrey

  • A model for cosmological simulations of galaxy formation physics

    Mark Vogelsberger;Shy Genel;Debora Sijacki;Paul Torrey

  • Submillimeter Galaxies at z ~ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO-H2 Conversion Factor*

    L. J. Tacconi;R. Genzel;I. Smail;R. Neri

  • From Rings to Bulges: Evidence for Rapid Secular Galaxy Evolution at z ~ 2 from Integral Field Spectroscopy in the SINS Survey

    R. Genzel;A. Burkert;N. Bouché;G. Cresci

  • First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback

    Dylan Nelson;Annalisa Pillepich;Volker Springel;Volker Springel;Volker Springel;Rüdiger Pakmor;Rüdiger Pakmor

  • THE IMPACT OF COLD GAS ACCRETION ABOVE A MASS FLOOR ON GALAXY SCALING RELATIONS

    N. Bouché;A. Dekel;R. Genzel;S. Genel

  • The merger rate of galaxies in the Illustris simulation: a comparison with observations and semi-empirical models

    Vicente Rodríguez-Gómez;Shy Genel;Shy Genel;Mark Vogelsberger;Debora Sijacki

  • A model for cosmological simulations of galaxy formation physics: multi-epoch validation

    Paul Torrey;Mark Vogelsberger;Shy Genel;Debora Sijacki

Frequent Co-Authors

Volker Springel
Volker Springel Max Planck Institute for Astrophysics
Lars Hernquist
Lars Hernquist Harvard University
Reinhard Genzel
Reinhard Genzel Max Planck Institute for Extraterrestrial Physics
Dieter Lutz
Dieter Lutz Max Planck Society
Giovanni Cresci
Giovanni Cresci National Institute for Astrophysics
Linda J. Tacconi
Linda J. Tacconi Max Planck Institute for Extraterrestrial Physics
Andreas Burkert
Andreas Burkert Ludwig-Maximilians-Universität München
Ric Davies
Ric Davies Max Planck Society
Alvio Renzini
Alvio Renzini National Institute for Astrophysics

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