World's Best Scientists 2026 revealed!
Julianne J. Dalcanton

Julianne J. Dalcanton

D-Index & Metrics

Physics

D-Index
102
Citations
52392
World Ranking
1526
National Ranking
802

Julianne J. Dalcanton 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 Julianne J. Dalcanton sits on this spectrum.

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 publications 1,469+

This scientist: 500 publications — 56th percentile

56% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

Julianne J. Dalcanton 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 Julianne J. Dalcanton sits on this spectrum.

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 D-Index 185+

This scientist: 102 D-Index — 59th percentile

59% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Research.com Recognitions

  • 2002 - Fellow of Alfred P. Sloan Foundation

Overview

Julianne J. Dalcanton is affiliated with the University of Washington in the United States. Their research focuses primarily on physics and astronomy, with a substantial emphasis on astronomy and astrophysics. This work spans subfields including instrumentation, computational mechanics, nuclear and high energy physics, and electrical and electronic engineering.

Their scientific contributions cover various main topics, including stellar, planetary, and galactic studies, astronomy and astrophysical research, and galaxies concerning formation, evolution, and phenomena. Additional areas of study include astrophysics and star formation studies, gamma-ray bursts and supernovae, astronomical observations and instrumentation, and CCD and CMOS imaging sensors.

Frequent publication venues for their work include:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • The Astronomical Journal
  • The Astrophysical Journal Supplement Series

Among notable recent papers are:

  • "Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud," 2020, Monthly Notices of the Royal Astronomical Society
  • "Stellar Feedback and Resolved Stellar IFU Spectroscopy in the Nearby Spiral Galaxy NGC 300," 2020, The Astrophysical Journal
  • "The JWST Resolved Stellar Populations Early Release Science Program. II. Survey Overview," 2023, The Astrophysical Journal Supplement Series
  • "The JWST Resolved Stellar Populations Early Release Science Program. V. DOLPHOT Stellar Photometry for NIRCam and NIRISS," 2024, The Astrophysical Journal Supplement Series
  • "The TREX Survey: Kinematical Complexity Throughout M33's Stellar Disk and Evidence for a Stellar Halo*," 2022, The Astrophysical Journal

Collaborations are a significant part of their research output. Frequent coauthors include Benjamin F. Williams, Andrew E. Dolphin, Daniel R. Weisz, Evan D. Skillman, and Puragra Guhathakurta, reflecting ongoing collaborative efforts across multiple projects and studies.

In recognition of contribution to the field, Julianne J. Dalcanton was named a Fellow of the Alfred P. Sloan Foundation in 2002.

Best Publications

  • Sloan Digital Sky Survey: Early data release

    C. Stoughton;R. H. Lupton;M. Bernardi;M. R. Blanton

  • Sloan digital sky survey: Early data release

    Chris Stoughton;Robert H. Lupton;Mariangela Bernardi;Michael R. Blanton;Michael R. Blanton

  • The fourth data release of the Sloan Digital Sky Survey

    Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam;Kurt S.J. Anderson

  • The Fifth Data Release of the Sloan Digital Sky Survey

    Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam;Kurt S.J. Anderson

  • Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample

    Michael A. Strauss;David H. Weinberg;Robert H. Lupton;Vijay K. Narayanan

  • The first data release of the sloan digital sky survey

    Kevork Abazajian;Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam

  • The Luminosity Function of Galaxies in SDSS Commissioning Data

    M. R. Blanton

  • The Third Data Release of the Sloan Digital Sky Survey

    Kevork Abazajian;Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam

  • A New Generation of PARSEC-COLIBRI Stellar Isochrones Including the TP-AGB Phase

    Paola Marigo;Léo Girardi;Alessandro Bressan;Philip Rosenfield

  • The Luminosity Function of Galaxies in SDSS Commissioning Data

    Michael R. Blanton;Julianne Dalcanton;Daniel Eisenstein;Jon Loveday

  • The Milky Way Tomography with SDSS: II. Stellar Metallicity

    Zeljko Ivezic;Branimir Sesar;Mario Juric;Nicholas Bond

  • Galaxy clustering in early sloan digital sky survey redshift data

    Idit Zehavi;Idit Zehavi;Michael R. Blanton;Michael R. Blanton;Joshua A. Frieman;Joshua A. Frieman;David H. Weinberg

  • Comparison of H-alpha and UV Star Formation Rates in the Local Volume: Systematic Discrepancies for Dwarf Galaxies

    Janice C. Lee;Armando Gil de Paz;Christy Tremonti;Robert C. Kennicutt

  • THE FORMATION OF DISK GALAXIES

    Julianne J. Dalcanton;David N. Spergel;F. J. Summers

  • The Milky Way Tomography with SDSS. II. Stellar Metallicity

    Željko Ivezić;Branimir Sesar;Mario Jurić;Nicholas Bond

  • COMPARISON OF Hα AND UV STAR FORMATION RATES IN THE LOCAL VOLUME: SYSTEMATIC DISCREPANCIES FOR DWARF GALAXIES

    Janice C. Lee;Armando Gil de Paz;Christy Tremonti;Christy Tremonti;Robert C. Kennicutt;Robert C. Kennicutt

  • The ACS Nearby Galaxy Survey Treasury

    Julianne J. Dalcanton;Benjamin F. Williams;Anil C. Seth;Andrew Dolphin

  • A New Milky Way Dwarf Galaxy in Ursa Major

    Beth Willman;Julianne J. Dalcanton;David Martinez-Delgado;David Martinez-Delgado;Andrew A. West

  • The Panchromatic Hubble Andromeda Treasury

    J. J. Dalcanton;B. F. Williams;D. Lang;T. R. Lauer

  • THE SPITZER LOCAL VOLUME LEGACY: SURVEY DESCRIPTION AND INFRARED PHOTOMETRY

    D. A. Dale;S. A. Cohen;L. C. Johnson;L. C. Johnson;M. D. Schuster

Frequent Co-Authors

Daniel R. Weisz
Daniel R. Weisz University of California, Berkeley
Anil C. Seth
Anil C. Seth University of Utah
Evan D. Skillman
Evan D. Skillman University of Minnesota
Eric F. Bell
Eric F. Bell University of Michigan–Ann Arbor
Léo Girardi
Léo Girardi National Institute for Astrophysics
Dennis Zaritsky
Dennis Zaritsky University of Arizona
Daniel A. Dale
Daniel A. Dale University of Wyoming
Puragra Guhathakurta
Puragra Guhathakurta University of California, Santa Cruz
Stephanie M. Gogarten
Stephanie M. Gogarten University of Washington
Jon A. Holtzman
Jon A. Holtzman New Mexico State University

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