| Discipline name | D-Index | World Ranking | Current World Ranking | National Ranking | Current National Ranking | Publications | Citations |
|---|---|---|---|---|---|---|---|
| Physics | 133 | 510 | 491 | 284 | 272 | 997 | 75004 |
The chart shows the history of publications by H. T. Diehl between 1987 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. H. T. Diehl published across 39 years, from 1987 to 2025, averaging 28.5 papers a year. Output peaked at 67 publications in 2020. 56 of the 1,112 publications appeared in the last two years.
1,112 publications in total across all disciplines
| Year | Publications |
|---|---|
| 1987 | 1 |
| 1988 | 0 |
| 1989 | 3 |
| 1990 | 2 |
| 1991 | 4 |
| 1992 | 2 |
| 1993 | 3 |
| 1994 | 4 |
| 1995 | 16 |
| 1996 | 10 |
| 1997 | 24 |
| 1998 | 33 |
| 1999 | 22 |
| 2000 | 22 |
| 2001 | 25 |
| 2002 | 15 |
| 2003 | 5 |
| 2004 | 10 |
| 2005 | 33 |
| 2006 | 33 |
| 2007 | 34 |
| 2008 | 64 |
| 2009 | 49 |
| 2010 | 40 |
| 2011 | 51 |
| 2012 | 60 |
| 2013 | 30 |
| 2014 | 28 |
| 2015 | 47 |
| 2016 | 51 |
| 2017 | 53 |
| 2018 | 44 |
| 2019 | 57 |
| 2020 | 67 |
| 2021 | 61 |
| 2022 | 32 |
| 2023 | 21 |
| 2024 | 31 |
| 2025 | 25 |
| Total | 1,112 |
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 H. T. Diehl sits on this spectrum.
This scientist: 997 publications — 91st percentile
91% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
| 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 | |
| 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 | 997 |
| 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 |
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where H. T. Diehl sits on this spectrum.
This scientist: 133 D-Index — 86th percentile
86% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
| 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 | |
| 132–133 | 32 | 133 |
| 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 |
H. T. Diehl is affiliated with Fermilab in the United States and has contributed extensively to the field of Physics and Astronomy, with a primary focus on Astronomy and Astrophysics, Nuclear and High Energy Physics, and Instrumentation. Their body of research also touches on Atomic and Molecular Physics, and Optics, as well as Electrical and Electronic Engineering.
Diehl's scholarly work predominantly covers topics related to:
Frequent collaborators include:
Key venues for Diehl's publications encompass:
Recent notable papers authored or co-authored by H. T. Diehl include:
The research contributions by H. T. Diehl span a significant range of studies related to dark energy, cosmic shear, galaxy clustering, weak lensing, and supernova cosmology. Their work on large-scale surveys contributes to constraining cosmological parameters, understanding dark matter properties, and expanding the knowledge base regarding the evolution of cosmic structures through observational astronomy.
S. Abachi;M. Abolins;B. S. Acharya;I. Adam
V. M. Abazov;B. Abbott;M. Abolins;B. S. Acharya
T. M. C. Abbott;F. B. Abdalla;A. Alarcon;J. Aleksić
B. Flaugher;H. T. Diehl;K. Honscheid;T. M. C. Abbott
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese;F. Acernese
P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger
B. Flaugher;H. T. Diehl;K. Honscheid;T. M. C. Abbott
T. Abbott;F. B. Abdalla;J. Aleksić
P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger
V. M. Abazov;B. Abbott;M. Abolins;B. S. Acharya
K. Bechtol;A. Drlica-Wagner;E. Balbinot
M. A. Troxel;N. MacCrann;N. MacCrann;J. Zuntz;T. F. Eifler
A. Drlica-Wagner;K. Bechtol;E. S. Rykoff
V. M. Abazov;B. Abbott;M. Abolins;B. S. Acharya
T. M. C. Abbott;F. B. Abdalla;F. B. Abdalla;S. Allam;A. Amara
V. M. Abazov;B. Abbott;B. S. Acharya;M. Adams
A. Drlica-Wagner;K. Bechtol;E. S. Rykoff;E. S. Rykoff;E. Luque
T. M. C. Abbott;F. B. Abdalla;S. Allam;A. Amara
K. Bechtol;A. Drlica-Wagner;E. Balbinot;A. Pieres
M. Soares-Santos;D. E. Holz;J. Annis;R. Chornock
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