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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 106 1324 1254 693 645 344 47846

Charlie Conroy publications per year

The chart shows the history of publications by Charlie Conroy between 2004 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Charlie Conroy published across 22 years, from 2004 to 2025, averaging 20.2 papers a year. Output peaked at 53 publications in 2019. 60 of the 445 publications appeared in the last two years.

No. of publications
10 20 30 40 50
Bar chart. Horizontal axis: year, 2004 to 2025. Vertical axis: number of publications, 0 to 53. Peak 53 publications in 2019. 2004: 1 publication 2005: 5 publications 2006: 2 publications 2007: 4 publications 2008: 4 publications 2009: 5 publications 2010: 9 publications 2011: 9 publications 2012: 12 publications 2013: 17 publications 2014: 15 publications 2015: 26 publications 2016: 17 publications 2017: 21 publications 2018: 46 publications 2019: 53 publications 2020: 24 publications 2021: 37 publications 2022: 49 publications 2023: 29 publications 2024: 42 publications 2025: 18 publications
2004 2025

445 publications in total across all disciplines

View publications per year as a table
Charlie Conroy: publications per year, 2004 to 2025
Year Publications
2004 1
2005 5
2006 2
2007 4
2008 4
2009 5
2010 9
2011 9
2012 12
2013 17
2014 15
2015 26
2016 17
2017 21
2018 46
2019 53
2020 24
2021 37
2022 49
2023 29
2024 42
2025 18
Total 445
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Charlie Conroy 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 Charlie Conroy 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, 343–362 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: 344 publications — 26th percentile

26% 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
303–322 136
323–342 162
343–362 155 344
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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Charlie Conroy 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 Charlie Conroy 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, 106–107 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: 106 D-Index — 65th percentile

65% 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
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
106–107 87 106
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

  • 2013 - Fellow of Alfred P. Sloan Foundation

Overview

Charlie Conroy is affiliated with Harvard University in the United States and specializes in the field of Physics and Astronomy. Their research primarily focuses on areas within Astronomy and Astrophysics, with significant contributions to subfields such as Instrumentation, Atomic and Molecular Physics and Optics, General Health Professions, and Statistical and Nonlinear Physics.

The main topics of Conroy's work include stellar, planetary, and galactic studies; astronomy and astrophysical research; galaxies related to formation, evolution, and phenomena; astrophysics and star formation studies; gamma-ray bursts and supernovae; astrophysical phenomena and observations; and pulsars and gravitational waves research.

They have published extensively in several academic venues. The most frequent publication outlets include:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal Letters
  • Zenodo (CERN European Organization for Nuclear Research)

Recent scientific papers authored or co-authored by Conroy include:

  • "Two Remarkably Luminous Galaxy Candidates at z ≈ 10-12 Revealed by JWST" (2022), The Astrophysical Journal Letters
  • "The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V" (2023), The Astrophysical Journal Supplement Series
  • "A Sun-like star orbiting a black hole" (2022), Monthly Notices of the Royal Astronomical Society
  • "Reconstructing the Last Major Merger of the Milky Way with the H3 Survey" (2021), The Astrophysical Journal
  • "Fast, Slow, Early, Late: Quenching Massive Galaxies at z ∼ 0.8" (2022), The Astrophysical Journal

Conroy frequently collaborates with several researchers in their field. Notable co-authors include:

  • Rohan P. Naidu
  • Benjamin D. Johnson
  • Vedant Chandra
  • Pieter van Dokkum
  • Ana Bonaca

Among the recognitions awarded to Charlie Conroy is the Fellowship from the Alfred P. Sloan Foundation, received in 2013.

Best Publications

  • The Average Star Formation Histories of Galaxies in Dark Matter Halos from z = 0-8

    Peter S. Behroozi;Peter S. Behroozi;Risa H. Wechsler;Risa H. Wechsler;Charlie Conroy

  • The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies

    Charlie Conroy;James E. Gunn;Martin White

  • Galaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation

    S. M. Faber;C. N. A. Willmer;C. Wolf;D. C. Koo

  • Galaxy luminosity functions to z∼ 1 from DEEP2 and COMBO-17: Implications for red galaxy formation

    S. M. Faber;C. N. A. Willmer;C. Wolf;D. C. Koo

  • MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS

    Jieun Choi;Aaron Dotter;Charlie Conroy;Matteo Cantiello

  • Overview of the SDSS-IV MaNGA Survey: Mapping nearby Galaxies at Apache Point Observatory

    Kevin Bundy;Matthew A. Bershady;David R. Law;Renbin Yan

  • THE PROPAGATION OF UNCERTAINTIES IN STELLAR POPULATION SYNTHESIS MODELING. III. MODEL CALIBRATION, COMPARISON, AND EVALUATION

    Charlie Conroy;James E. Gunn

  • A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4

    Peter S. Behroozi;Peter S. Behroozi;Charlie Conroy;Risa H. Wechsler;Risa H. Wechsler

  • UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10

    Peter Behroozi;Risa H Wechsler;Risa H Wechsler;Andrew P Hearin;Charlie Conroy

  • Modeling the Panchromatic Spectral Energy Distributions of Galaxies

    Charlie Conroy

  • The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts

    Jeffrey A. Newman;Michael C. Cooper;Marc Davis;S. M. Faber

  • Modeling luminosity-dependent galaxy clustering through cosmic time

    Charlie Conroy;Risa H. Wechsler;Andrey V. Kravtsov

  • A Substantial Population of Low-Mass Stars in Luminous Elliptical Galaxies

    Pieter G. van Dokkum;Charlie Conroy;Charlie Conroy

  • THE STELLAR INITIAL MASS FUNCTION IN EARLY-TYPE GALAXIES FROM ABSORPTION LINE SPECTROSCOPY. II. RESULTS

    Charlie Conroy;Charlie Conroy;Pieter G. van Dokkum

  • Galaxy evolution in groups and clusters: satellite star formation histories and quenching time-scales in a hierarchical Universe

    Andrew R. Wetzel;Jeremy L. Tinker;Charlie Conroy;Frank C. van den Bosch

  • The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-frame Optical Spectroscopy for ~1500 H-selected Galaxies at 1.37 ? z ? 3.8

    Mariska Kriek;Alice E. Shapley;Naveen A. Reddy;Brian Siana

  • The DEEP2 Galaxy Redshift Survey: The Galaxy Luminosity Function to z ~ 1

    C. N. A. Willmer;S. M. Faber;D. C. Koo;B. J. Weiner

  • Connecting Galaxies, Halos, and Star Formation Rates Across Cosmic Time

    Charlie Conroy;Risa H. Wechsler

  • FORTY-SEVEN MILKY WAY-SIZED, EXTREMELY DIFFUSE GALAXIES IN THE COMA CLUSTER

    Pieter G. van Dokkum;Roberto Abraham;Allison Merritt;Jielai Zhang

  • THE DUST ATTENUATION LAW IN DISTANT GALAXIES: EVIDENCE FOR VARIATION WITH SPECTRAL TYPE

    Mariska Kriek;Charlie Conroy

Frequent Co-Authors

Aaron J. Romanowsky
Aaron J. Romanowsky San Jose State University
Pieter G. van Dokkum
Pieter G. van Dokkum Yale University
Roberto Abraham
Roberto Abraham University of Toronto
Jean P. Brodie
Jean P. Brodie University of California, Santa Cruz
Dennis Zaritsky
Dennis Zaritsky University of Arizona
Mariska Kriek
Mariska Kriek University of California, Berkeley
Jeremy L. Tinker
Jeremy L. Tinker New York University
Risa H. Wechsler
Risa H. Wechsler Stanford University
Gabriel B. Brammer
Gabriel B. Brammer University of Copenhagen
Renbin Yan
Renbin Yan University of Kentucky

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