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D-Index & Metrics

Physics

D-Index
86
Citations
32948
World Ranking
2511
National Ranking
1246

Christopher M. Hirata 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 Christopher M. Hirata 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: 308 publications — 19th percentile

19% of scientists in this discipline score the same or lower.

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

Christopher M. Hirata 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 Christopher M. Hirata 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: 86 D-Index — 32nd percentile

32% of scientists in this discipline score the same or lower.

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

Overview

Christopher M. Hirata is affiliated with The Ohio State University in the United States. Their research primarily spans the fields of physics and astronomy, with a focus on subfields including astronomy and astrophysics, atomic and molecular physics and optics, nuclear and high energy physics, instrumentation, and electrical and electronic engineering.

The main topics of their research encompass galaxies: formation, evolution, and phenomena, adaptive optics and wavefront sensing, astronomy and astrophysical research, cosmology and gravitation theories, astrophysics and cosmic phenomena, radio astronomy observations and technology, and stellar, planetary, and galactic studies.

Christopher M. Hirata has published extensively in various scientific venues. Frequent publication venues include arXiv (Cornell University), Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, Physical Review D, and Publications of the Astronomical Society of the Pacific.

Their recent papers cover a range of topics and journal publications such as:

  • "Cosmology with the Roman Space Telescope - multiprobe strategies", 2021, Monthly Notices of the Royal Astronomical Society
  • "The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope", 2022, The Astrophysical Journal
  • "Cosmology with the Roman Space Telescope: synergies with the Rubin Observatory Legacy Survey of Space and Time", 2021, Monthly Notices of the Royal Astronomical Society
  • "SPHEREx: NASA's near-infrared spectrophotometric all-sky survey", 2020, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave
  • "Toward Powerful Probes of Neutrino Self-Interactions in Supernovae", 2023, Physical Review Letters

Collaborations are an important aspect of their research. Frequent co-authors include:

  • Heyang Long
  • M. A. Troxel
  • A. Choi
  • Mike Jarvis
  • Rachel Mandelbaum

Best Publications

  • The Sixth Data Release of the Sloan Digital Sky Survey

    Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam;Carlos Allende Prieto

  • 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

  • Observational probes of cosmic acceleration

    David H. Weinberg;Michael J. Mortonson;Daniel J. Eisenstein;Daniel J. Eisenstein;Christopher Hirata

  • Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

    D. Spergel;N. Gehrels;C. Baltay;D. Bennett

  • Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the SDSS: stellar mass, luminosity, morphology, and environment dependencies

    Rachel Mandelbaum;Uros Seljak;Guinevere Kauffmann;Christopher M. Hirata

  • Galaxy halo masses and satellite fractions from galaxy–galaxy lensing in the Sloan Digital Sky Survey: stellar mass, luminosity, morphology and environment dependencies

    Rachel Mandelbaum;Uroš Seljak;Uroš Seljak;Guinevere Kauffmann;Christopher M. Hirata

  • Intrinsic alignment-lensing interference as a contaminant of cosmic shear

    Christopher M. Hirata;Uroš Seljak

  • Relative velocity of dark matter and baryonic fluids and the formation of the first structures

    Dmitriy Tseliakhovich;Christopher Hirata

  • Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)

    Masahiro Takada;Richard Ellis;Masashi Chiba;Jenny E. Greene

  • Shear calibration biases in weak-lensing surveys

    Christopher M. Hirata;Uros Seljak

  • Constraints on local primordial non-Gaussianity from large scale structure

    Anže Slosar;Anže Slosar;Christopher Hirata;Uroš Seljak;Uroš Seljak;Shirley Ho

  • Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph

    Masahiro Takada;Richard S. Ellis;Masashi Chiba;Jenny E. Greene

  • Correlation of CMB with large-scale structure. I. Integrated Sachs-Wolfe tomography and cosmological implications

    Shirley Ho;Christopher M. Hirata;Nikhil Padmanabhan;Uros Seljak;Uros Seljak

  • The Shear TEsting Programme 2: Factors affecting high precision weak lensing analyses

    Richard Massey;Catherine Heymans;Joel Bergé;Gary Bernstein

  • Reconstruction of lensing from the cosmic microwave background polarization

    Christopher M. Hirata;Uroš Seljak

  • Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7

    Rachel Mandelbaum;Rachel Mandelbaum;Anÿze Slosar;Tobias Baldauf;Uroÿs Seljak

  • A simulation-calibrated limit on the H i power spectrum from the GMRT Epoch of Reionization experiment

    Gregory Paciga;Joshua G. Albert;Kevin Bandura;Kevin Bandura;Tzu-Ching Chang;Tzu-Ching Chang

  • A halo mass—concentration relation from weak lensing

    Rachel Mandelbaum;Uroš Seljak;Uroš Seljak;Christopher M. Hirata

  • Wouthuysen-Field coupling strength and application to high-redshift 21-cm radiation

    Christopher M. Hirata

  • Density profiles of galaxy groups and clusters from SDSS galaxy–galaxy weak lensing

    Rachel Mandelbaum;Uroš Seljak;Uroš Seljak;Richard J. Cool;Michael Blanton

Frequent Co-Authors

Rachel Mandelbaum
Rachel Mandelbaum Carnegie Mellon University
Uroš Seljak
Uroš Seljak University of California, Berkeley
Olivier Doré
Olivier Doré California Institute of Technology
David N. Spergel
David N. Spergel Princeton University
David H. Weinberg
David H. Weinberg The Ohio State University
Anže Slosar
Anže Slosar Brookhaven National Laboratory
Marc Kamionkowski
Marc Kamionkowski Johns Hopkins University
Nikhil Padmanabhan
Nikhil Padmanabhan Yale University
Bhuvnesh Jain
Bhuvnesh Jain University of Pennsylvania
Daniel J. Eisenstein
Daniel J. Eisenstein Harvard University

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