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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 81 2917 2770 1420 1322 288 27001

Steven R. Furlanetto publications per year

The chart shows the history of publications by Steven R. Furlanetto between 2001 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Steven R. Furlanetto published across 25 years, from 2001 to 2025, averaging 13.3 papers a year. Output peaked at 36 publications in 2019. 38 of the 332 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 2001 to 2025. Vertical axis: number of publications, 0 to 36. Peak 36 publications in 2019. 2001: 1 publication 2002: 5 publications 2003: 4 publications 2004: 16 publications 2005: 10 publications 2006: 23 publications 2007: 12 publications 2008: 8 publications 2009: 27 publications 2010: 4 publications 2011: 9 publications 2012: 4 publications 2013: 25 publications 2014: 7 publications 2015: 6 publications 2016: 8 publications 2017: 7 publications 2018: 12 publications 2019: 36 publications 2020: 12 publications 2021: 27 publications 2022: 21 publications 2023: 10 publications 2024: 24 publications 2025: 14 publications
2001 2025

332 publications in total across all disciplines

View publications per year as a table
Steven R. Furlanetto: publications per year, 2001 to 2025
Year Publications
2001 1
2002 5
2003 4
2004 16
2005 10
2006 23
2007 12
2008 8
2009 27
2010 4
2011 9
2012 4
2013 25
2014 7
2015 6
2016 8
2017 7
2018 12
2019 36
2020 12
2021 27
2022 21
2023 10
2024 24
2025 14
Total 332
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Steven R. Furlanetto 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 Steven R. Furlanetto 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, 283–302 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: 288 publications — 15th percentile

15% 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
223–242 85
243–262 112
263–282 114
283–302 126 288
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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Steven R. Furlanetto 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 Steven R. Furlanetto 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
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Research.com Recognitions

  • 2010 - Fellow of Alfred P. Sloan Foundation

Overview

Steven R. Furlanetto is affiliated with the University of California, Los Angeles in the United States. Their research activity primarily focuses on the fields of Physics and Astronomy, complemented by work in Engineering.

The main subfields of study encompass Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Electrical and Electronic Engineering, and Aerospace Engineering.

Key research topics addressed in their publications include:

  • Galaxies: Formation, Evolution, Phenomena
  • Radio Astronomy Observations and Technology
  • Astronomy and Astrophysical Research
  • Astrophysics and Cosmic Phenomena
  • Stellar, planetary, and galactic studies
  • Antenna Design and Optimization
  • Astrophysical Phenomena and Observations

Frequent co-authors in their work are:

  • Andrei Mesinger
  • G. Bernardi
  • Tashalee S. Billings
  • Judd D. Bowman
  • Jacob Burba

Steven R. Furlanetto has published extensively in venues such as:

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

Recent publications include:

  • First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum (2022, The Astrophysical Journal)
  • HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization (2022, The Astrophysical Journal)
  • Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations (2023, The Astrophysical Journal)
  • Balancing the efficiency and stochasticity of star formation with dust extinction in z ≳ 10 galaxies observed by JWST (2022, Monthly Notices of the Royal Astronomical Society)
  • The effects of population III radiation backgrounds on the cosmological 21-cm signal (2020, Monthly Notices of the Royal Astronomical Society)

Steven R. Furlanetto received the Fellow of Alfred P. Sloan Foundation award in 2010.

Best Publications

  • Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe

    Steven R. Furlanetto;S. Peng Oh;Frank H. Briggs

  • Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and Hubble Space Telescope

    Brant E. Robertson;Richard S. Ellis;Steven R. Furlanetto;James S. Dunlop

  • Cosmic Reionization and Early Star-forming Galaxies: a Joint Analysis of new Constraints From Planck and the Hubble Space Telescope

    Brant E. Robertson;Richard S. Ellis;Steven R. Furlanetto;James S. Dunlop

  • The Growth of HII Regions During Reionization

    Steven Furlanetto;Matias Zaldarriaga;Lars Hernquist

  • 21cmfast: a fast, seminumerical simulation of the high‐redshift 21‐cm signal

    Andrei Mesinger;Steven Furlanetto;Renyue Cen

  • The Abundance of Star-Forming Galaxies in the Redshift Range 8.5 to 12: New Results from the 2012 Hubble Ultra Deep Field Campaign

    Richard S Ellis;Ross J McLure;James S Dunlop;Brant E Robertson

  • Hydrogen epoch of reionization array (HERA)

    David R. DeBoer;Aaron R. Parsons;James E. Aguirre;Paul Alexander

  • The Growth of H II Regions During Reionization

    Steven R. Furlanetto;Matias Zaldarriaga;Lars Hernquist

  • 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal

    Andrei Mesinger;Steven Furlanetto;Renyue Cen

  • New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign

    Brant E. Robertson;Steven R. Furlanetto;Evan Schneider;Stephane Charlot

  • The Abundance of Star-forming Galaxies in the Redshift Range 8.5-12: New Results from the 2012 Hubble Ultra Deep Field Campaign

    Richard S. Ellis;Ross J. McLure;James S. Dunlop;Brant E. Robertson

  • 21 Centimeter Fluctuations from Cosmic Gas at High Redshifts

    Matias Zaldarriaga;Steven R. Furlanetto;Lars Hernquist

  • Hydrogen Epoch of Reionization Array (HERA)

    David R. DeBoer;Aaron R. Parsons;James E. Aguirre;Paul Alexander

  • Efficient Simulations of Early Structure Formation and Reionization

    Andrei Mesinger;Steven Furlanetto

  • Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization

    Matthew McQuinn;Oliver Zahn;Matias Zaldarriaga;Lars Hernquist

  • A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble Ultra-Deep Field imaging

    R. J. McLure;J. S. Dunlop;R. A. A. Bowler;E. Curtis-Lake

  • Simulations and Analytic Calculations of Bubble Growth during Hydrogen Reionization

    Oliver Zahn;Adam Lidz;Matthew McQuinn;Suvendra Dutta

  • The global 21-centimeter background from high redshifts

    Steven R. Furlanetto

  • 21-cm fluctuations from inhomogeneous X-ray heating before reionization

    Jonathan R. Pritchard;Steven R. Furlanetto

  • Intergalactic Magnetic Fields from Quasar Outflows

    Steven R. Furlanetto;Abraham Loeb

Frequent Co-Authors

Abraham Loeb
Abraham Loeb Harvard University
Matias Zaldarriaga
Matias Zaldarriaga Princeton University
Brant Robertson
Brant Robertson University of California, Santa Cruz
Olivier Doré
Olivier Doré California Institute of Technology
Michele Cirasuolo
Michele Cirasuolo European Southern Observatory
Volker Bromm
Volker Bromm The University of Texas at Austin
Richard S. Ellis
Richard S. Ellis University College London
Anton M. Koekemoer
Anton M. Koekemoer Space Telescope Science Institute
Lars Hernquist
Lars Hernquist Harvard University
Gianni Bernardi
Gianni Bernardi National Institute for Astrophysics

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