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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 95 1923 1827 1000 934 246 36241

Daniel H. McIntosh publications per year

The chart shows the history of publications by Daniel H. McIntosh between 1951 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Daniel H. McIntosh published across 75 years, from 1951 to 2025, averaging 3.6 papers a year. Output peaked at 29 publications in 2009. 2 of the 267 publications appeared in the last two years.

No. of publications
5 10 15 20 25
Bar chart. Horizontal axis: year, 1951 to 2025. Vertical axis: number of publications, 0 to 29. Peak 29 publications in 2009. 1951: 2 publications 1952: 1 publication 1953: 5 publications 1954: 0 publications 1955: 3 publications 1956: 0 publications 1957: 1 publication 1958: 0 publications 1959: 1 publication 1960: 0 publications 1961: 3 publications 1962: 0 publications 1963: 4 publications 1964: 1 publication 1965: 1 publication 1966: 0 publications 1967: 0 publications 1968: 0 publications 1969: 0 publications 1970: 0 publications 1971: 0 publications 1972: 1 publication 1973: 0 publications 1974: 0 publications 1975: 0 publications 1976: 1 publication 1977: 1 publication 1978: 1 publication 1979: 0 publications 1980: 0 publications 1981: 0 publications 1982: 0 publications 1983: 1 publication 1984: 0 publications 1985: 0 publications 1986: 0 publications 1987: 0 publications 1988: 0 publications 1989: 0 publications 1990: 0 publications 1991: 1 publication 1992: 0 publications 1993: 0 publications 1994: 0 publications 1995: 0 publications 1996: 0 publications 1997: 0 publications 1998: 0 publications 1999: 2 publications 2000: 4 publications 2001: 2 publications 2002: 3 publications 2003: 10 publications 2004: 24 publications 2005: 15 publications 2006: 8 publications 2007: 14 publications 2008: 24 publications 2009: 29 publications 2010: 4 publications 2011: 11 publications 2012: 11 publications 2013: 7 publications 2014: 12 publications 2015: 13 publications 2016: 8 publications 2017: 11 publications 2018: 8 publications 2019: 7 publications 2020: 3 publications 2021: 1 publication 2022: 6 publications 2023: 0 publications 2024: 0 publications 2025: 2 publications
1951 2025

267 publications in total across all disciplines

View publications per year as a table
Daniel H. McIntosh: publications per year, 1951 to 2025
Year Publications
1951 2
1952 1
1953 5
1954 0
1955 3
1956 0
1957 1
1958 0
1959 1
1960 0
1961 3
1962 0
1963 4
1964 1
1965 1
1966 0
1967 0
1968 0
1969 0
1970 0
1971 0
1972 1
1973 0
1974 0
1975 0
1976 1
1977 1
1978 1
1979 0
1980 0
1981 0
1982 0
1983 1
1984 0
1985 0
1986 0
1987 0
1988 0
1989 0
1990 0
1991 1
1992 0
1993 0
1994 0
1995 0
1996 0
1997 0
1998 0
1999 2
2000 4
2001 2
2002 3
2003 10
2004 24
2005 15
2006 8
2007 14
2008 24
2009 29
2010 4
2011 11
2012 11
2013 7
2014 12
2015 13
2016 8
2017 11
2018 8
2019 7
2020 3
2021 1
2022 6
2023 0
2024 0
2025 2
Total 267
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Daniel H. McIntosh 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 Daniel H. McIntosh 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, 243–262 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: 246 publications — 9th percentile

9% 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
243–262 112 246
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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Daniel H. McIntosh 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 Daniel H. McIntosh 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, 94–95 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: 95 D-Index — 49th percentile

49% 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 95
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

Daniel H. McIntosh is affiliated with the University of Missouri-Kansas City in the United States. Their research primarily focuses on physics and astronomy, with a significant concentration on astronomy and astrophysics, instrumentation, and nuclear and high energy physics subfields.

The scientist's work covers a range of topics, including:

  • Gamma-ray bursts and supernovae
  • Astronomy and astrophysical research
  • Galaxies: formation, evolution, phenomena
  • Stellar, planetary, and galactic studies
  • Astrophysical phenomena and observations
  • Astrophysics and cosmic phenomena
  • Pulsars and gravitational waves research

Daniel H. McIntosh's publications have appeared in several venues, most notably:

  • arXiv (Cornell University)
  • The Astrophysical Journal Letters
  • UNC Libraries
  • The Astrophysical Journal

Some of the recent papers associated with their research include:

  • 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)
  • Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations (2023, The Astrophysical Journal Letters)
  • Optimized Photometric Redshifts for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) (2023, The Astrophysical Journal)
  • The Cosmic Evolution Early Release Science Survey (CEERS) (2025, 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, arXiv (Cornell University))

Frequent collaborators include:

  • Avishai Dekel
  • Steven L. Finkelstein
  • Mark Dickinson
  • Henry C. Ferguson
  • Kartheik G. Iyer

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 optical and near-infrared properties of galaxies. I. Luminosity and stellar mass functions

    Eric F. Bell;Daniel H. McIntosh;Neal Katz;Martin D. Weinberg

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

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

  • 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

  • Nearly 5000 Distant Early-Type Galaxies in COMBO-17: A Red Sequence and Its Evolution since z ~ 1

    Eric F. Bell;Christian Wolf;Klaus Meisenheimer;Hans Walter Rix

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

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

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

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

  • GEMS: Galaxy Evolution from Morphologies and SEDs

    Hans-Walter Rix;Marco Barden;Steven V. W. Beckwith;Eric F. Bell

  • The size evolution of galaxies since z~3: combining SDSS, GEMS, and FIRES

    Ignacio Trujillo;Ignacio Trujillo;Natascha M. Förster Schreiber;Gregory Rudnick;Marco Barden

  • CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA

    Malcolm Hicken;Peter Challis;Saurabh Jha;Robert P. Kirshner

  • STRUCTURAL PARAMETERS OF GALAXIES IN CANDELS

    A. van der Wel;E. F. Bell;B. Häussler;E. J. McGrath

  • GEMS: Galaxy Evolution from Morphologies and SEDs

    Hans Walter Rix;Marco Barden;Steven V.W. Beckwith;Eric F. Bell

  • CANDELS: constraining the AGN-merger connection with host morphologies at z ~ 2

    Dale D. Kocevski;S. M. Faber;Mark Mozena;Anton M. Koekemoer

  • The importance of satellite quenching for the build-up of the red sequence of present-day galaxies

    Frank C. Van Den Bosch;Daniel Aquino;Xiaohu Yang;H. J. Mo

  • Dry Mergers in GEMS: The Dynamical Evolution of Massive Early-Type Galaxies

    Eric F. Bell;Thorsten Naab;Daniel H. McIntosh;Rachel S. Somerville

  • GEMS: Galaxy fitting catalogues and testing parametric galaxy fitting codes

    Boris Häußler;Daniel H. McIntosh;Marco Barden;Eric F. Bell

  • Dry Mergers in GEMS: The Dynamical Evolution of Massive Early-Type Galaxies

    Eric F. Bell;Thorsten Naab;Daniel H. McIntosh;Rachel S. Somerville

  • What turns galaxies off? The different morphologies of star-forming and quiescent galaxies since z ~ 2 from CANDELS

    Eric F. Bell;Arjen Van Der Wel;Casey Papovich;Dale Kocevski

  • GEMS: The Size Evolution of Disk Galaxies

    Marco Barden;Hans-Walter Rix;Rachel S. Somerville;Eric F. Bell

  • Scaling Relations of Spiral Galaxies

    S. Courteau;A. A. Dutton;F. van den Bosch;L. A. MacArthur

Frequent Co-Authors

Eric F. Bell
Eric F. Bell University of Michigan–Ann Arbor
Knud Jahnke
Knud Jahnke Max Planck Society
Chien Y. Peng
Chien Y. Peng Herzberg Institute of Astrophysics
Klaus Meisenheimer
Klaus Meisenheimer Max Planck Society
Rachel S. Somerville
Rachel S. Somerville Flatiron Institute
Catherine Heymans
Catherine Heymans University of Edinburgh
Sebastián F. Sánchez
Sebastián F. Sánchez National Autonomous University of Mexico
Shardha Jogee
Shardha Jogee The University of Texas at Austin
Christian Wolf
Christian Wolf Australian National University
Steven V. W. Beckwith
Steven V. W. Beckwith University of California, Berkeley

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