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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 130 563 542 312 298 474 66677

Casey Papovich publications per year

The chart shows the history of publications by Casey Papovich between 1998 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Casey Papovich published across 28 years, from 1998 to 2025, averaging 24 papers a year. Output peaked at 79 publications in 2023. 80 of the 673 publications appeared in the last two years.

No. of publications
25 50 75
Bar chart. Horizontal axis: year, 1998 to 2025. Vertical axis: number of publications, 0 to 79. Peak 79 publications in 2023. 1998: 1 publication 1999: 1 publication 2000: 2 publications 2001: 3 publications 2002: 5 publications 2003: 7 publications 2004: 32 publications 2005: 27 publications 2006: 28 publications 2007: 27 publications 2008: 20 publications 2009: 24 publications 2010: 16 publications 2011: 26 publications 2012: 20 publications 2013: 17 publications 2014: 19 publications 2015: 25 publications 2016: 25 publications 2017: 22 publications 2018: 25 publications 2019: 24 publications 2020: 31 publications 2021: 27 publications 2022: 60 publications 2023: 79 publications 2024: 47 publications 2025: 33 publications
1998 2025

673 publications in total across all disciplines

View publications per year as a table
Casey Papovich: publications per year, 1998 to 2025
Year Publications
1998 1
1999 1
2000 2
2001 3
2002 5
2003 7
2004 32
2005 27
2006 28
2007 27
2008 20
2009 24
2010 16
2011 26
2012 20
2013 17
2014 19
2015 25
2016 25
2017 22
2018 25
2019 24
2020 31
2021 27
2022 60
2023 79
2024 47
2025 33
Total 673
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Casey Papovich 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 Casey Papovich 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, 463–482 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: 474 publications — 52nd percentile

52% 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
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131 474
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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Casey Papovich 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 Casey Papovich 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, 130–131 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: 130 D-Index — 85th percentile

85% 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
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 33 130
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

Casey Papovich is affiliated with Texas A&M University in the United States and works primarily in the field of Physics and Astronomy. Their research spans several subfields including Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics and Optics, Nuclear and High Energy Physics, and Electrical and Electronic Engineering.

Their scientific contributions focus on main topics such as Galaxies: Formation, Evolution, and Phenomena, Astronomy and Astrophysical Research, Gamma-ray bursts and supernovae, Stellar, planetary, and galactic studies, Astrophysics and Star Formation Studies, Astrophysical Phenomena and Observations, and Adaptive optics and wavefront sensing.

Casey Papovich has published extensively in several venues. The most frequent publication outlets include:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astrophysical Journal Letters
  • Astronomy and Astrophysics
  • Monthly Notices of the Royal Astronomical Society

Recent papers authored or coauthored by Papovich demonstrate engagement with high-profile astrophysical phenomena observed with cutting-edge telescopes and instruments. Selected recent publications include:

  • CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST, 2023, The Astrophysical Journal Letters
  • Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS, 2023, The Astrophysical Journal Letters
  • A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging, 2022, The Astrophysical Journal Letters
  • A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars, 2023, The Astrophysical Journal Letters
  • UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z > 5, 2024, The Astrophysical Journal

The scientist has collaborated frequently with several colleagues, reflecting interdisciplinary and collaborative research efforts across astronomy and astrophysics. Frequent coauthors include:

  • Steven L. Finkelstein
  • L. Y. Aaron Yung
  • Anton M. Koekemoer
  • Mark Dickinson
  • Jeyhan S. Kartaltepe

Casey Papovich's profile is indicative of ongoing research that integrates observational astronomy with instrumentation development to explore cosmic origins, galaxy formation, and high-redshift phenomena, contributing to the broader understanding of the universe through rigorous astrophysical inquiry.

Best Publications

  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics

    Anton M. Koekemoer;S. M. Faber;Henry C. Ferguson;Norman A. Grogin

  • The Multiband Imaging Photometer for Spitzer (MIPS)

    G. H. Rieke;E. T. Young;C. W. Engelbracht;D. M. Kelly

  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

    Norman A. Grogin;Dale D. Kocevski;S. M. Faber;Henry C. Ferguson

  • Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies

    K. G. Noeske;B. J. Weiner;S. M. Faber;Casey J. Papovich

  • The Great Observatories Origins Deep Survey: Initial results from optical and near-infrared imaging

    M. Giavalisco;H. C. Ferguson;H. C. Ferguson;A. M. Koekemoer;M. Dickinson;M. Dickinson

  • Candels: The cosmic assembly near-infrared deep extragalactic legacy survey - The hubble space telescope observations, imaging data products, and mosaics

    Anton M. Koekemoer;S. M. Faber;Henry C. Ferguson;Norman A. Grogin

  • GOODS-Herschel: an infrared main sequence for star-forming galaxies

    D.Elbaz;M.Dickinson;H.S.Hwang;T.Diaz-Santos

  • GOODS–Herschel: an infrared main sequence for star-forming galaxies

    D. Elbaz;M. Dickinson;H. S. Hwang;T. Díaz-Santos

  • Infrared luminosity functions from the Chandra Deep Field South : the Spitzer view on the history of dusty star formation at 0<z<1

    E. Le Floc'h;C. Papovich;H. Dole;E. Bell

  • SPECTRAL ENERGY DISTRIBUTIONS AND MULTIWAVELENGTH SELECTION OF TYPE 1 QUASARS

    Gordon T. Richards;Gordon T. Richards;Mark Lacy;Lisa J. Storrie-Lombardi;Patrick B. Hall

  • Infrared Luminosity Functions from the Chandra Deep Field-South: The Spitzer View on the History of Dusty Star Formation at 0 ≲ z ≲ 1*

    Emeric Le Floc'h;Emeric Le Floc'h;Casey Papovich;Hervé Dole;Eric F. Bell

  • The Stellar Populations and Evolution of Lyman Break Galaxies

    Casey Papovich;Casey Papovich;Mark Dickinson;Mark Dickinson;Henry C. Ferguson

  • The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years

    Steven Lyle Finkelstein;Russell E. Ryan;Casey Papovich;Mark Dickinson

  • Towards an understanding of the rapid decline of the cosmic star formation rate

    Eric F. Bell;Casey Papovich;Christian Wolf;Emeric Le Floc'h

  • The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background.

    H Dole;G Lagache;JL Puget;KI Caputi

  • Toward an Understanding of the Rapid Decline of the Cosmic Star Formation Rate

    Eric F. Bell;Casey Papovich;Christian Wolf;Emeric Le Floc'h

  • The All-Wavelength Extended Groth Strip International Survey(AEGIS) Data Sets

    M. Davis;P. Guhathakurta;N. P. Konidaris;J. A. Newman

  • Spitzer view on the evolution of star-forming galaxies from z = 0 to z ∼ 3

    Pablo G. Pérez-González;George H. Rieke;Eiichi Egami;Almudena Alonso-Herrero;Almudena Alonso-Herrero

  • The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background

    Herve Dole;Guilaine Lagache;Jean-Loup Puget;Karina I. Caputi

  • The Evolution of the global stellar mass density at 0 < z < 3

    Mark Dickinson;Mark Dickinson;Casey Papovich;Casey Papovich;Henry C. Ferguson;Tamas Budavari

Frequent Co-Authors

Mark Dickinson
Mark Dickinson National Optical Astronomy Observatory
Anton M. Koekemoer
Anton M. Koekemoer Space Telescope Science Institute
Henry C. Ferguson
Henry C. Ferguson Space Telescope Science Institute
Steven L. Finkelstein
Steven L. Finkelstein The University of Texas at Austin
Mauro Giavalisco
Mauro Giavalisco University of Massachusetts Amherst
Christopher J. Conselice
Christopher J. Conselice University of Manchester
George H. Rieke
George H. Rieke University of Arizona
Jennifer M. Lotz
Jennifer M. Lotz Space Telescope Science Institute
Karl Glazebrook
Karl Glazebrook Swinburne University of Technology
Eric F. Bell
Eric F. Bell University of Michigan–Ann Arbor

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