World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
98
Citations
40996
World Ranking
1743
National Ranking
916

Harry I. Teplitz 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 Harry I. Teplitz 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: 511 publications — 58th percentile

58% of scientists in this discipline score the same or lower.

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

Harry I. Teplitz 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 Harry I. Teplitz 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: 98 D-Index — 53rd percentile

53% of scientists in this discipline score the same or lower.

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

Overview

Harry I. Teplitz is affiliated with the California Institute of Technology in the United States. Their research primarily spans the fields of Physics and Astronomy, with a focused specialization in Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics and Optics, Electrical and Electronic Engineering, and Nuclear and High Energy Physics.

The scientist's work covers a range of topics including Galaxies: Formation, Evolution, Phenomena; Astronomy and Astrophysical Research; Gamma-ray bursts and supernovae; Stellar, planetary, and galactic studies; Astrophysics and Star Formation Studies; Adaptive optics and wavefront sensing; and Astrophysics and Cosmic Phenomena.

Teplitz has published extensively in numerous venues, with notable frequency in:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astrophysical Journal Supplement Series
  • The Astrophysical Journal Letters
  • Astronomy and Astrophysics

Frequent co-authors include:

  • Marc Rafelski
  • Claudia Scarlata
  • Anahita Alavi
  • Anton M. Koekemoer
  • Xin Wang

Selected recent papers by Harry I. Teplitz include:

  • "COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs," 2022, The Astrophysical Journal Supplement Series
  • "The CatWISE2020 Catalog," 2021, The Astrophysical Journal Supplement Series
  • "The Low-redshift Lyman Continuum Survey. I. New, Diverse Local Lyman Continuum Emitters," 2022, The Astrophysical Journal Supplement Series
  • "The Low-redshift Lyman Continuum Survey. II. New Insights into LyC Diagnostics," 2022, The Astrophysical Journal
  • "The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope," 2022, The Astrophysical Journal

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

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

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

  • THE INFRARED SPECTROGRAPH (IRS) ON THE SPITZER SPACE TELESCOPE

    J. R. Houck;T. L. Roellig;J. van Cleve;W. J. Forrest

  • 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

  • Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

    B. T. Draine;D. A. Dale;G. Bendo;K. D. Gordon

  • Obscured and unobscured active galactic nuclei in the Spitzer Space Telescope First Look Survey

    M. Lacy;L. J. Storrie-Lombardi;A. Sajina;P. N. Appleton

  • Design and development of NIRSPEC: a near-infrared echelle spectrograph for the Keck II telescope

    Ian S. McLean;Eric E. Becklin;Oddvar Bendiksen;George Brims

  • The afterglow, redshift and extreme energetics of the γ-ray burst of 23 January 1999

    [No Value] Kulkarni;SG Djorgovski;SC Odewahn;JS Bloom

  • The afterglow, the redshift, and the extreme energetics of the gamma-ray burst 990123

    S. R. Kulkarni;S. G. Djorgovski;S. C. Odewahn;J. S. Bloom

  • Observations of Ultraluminous Infrared Galaxies with the Infrared Spectrograph on the Spitzer Space Telescope. II. The IRAS Bright Galaxy Sample

    L. Armus;V. Charmandaris;V. Charmandaris;J. Bernard-Salas;H. W. W. Spoon

  • Mid-Infrared Spectral Diagnosis of Submillimeter Galaxies

    Alexandra Pope;Ranga-Ram Chary;David M. Alexander;Lee Armus

  • The Far- and Mid-Infrared/Radio Correlations in the Spitzer Extragalactic First Look Survey

    P. N. Appleton;D. T. Fadda;F. R. Marleau;D. T. Frayer

  • The Far- and Mid-Infrared/Radio Correlations in the Spitzer Extragalactic First Look Survey

    P. N. Appleton;D. T. Fadda;F. R. Marleau;D. T. Frayer

  • The Massive Hosts of Radio Galaxies Across Cosmic Time

    Nick Seymour;Daniel Stern;Carlos De Breuck;Joel Vernet

  • Massive Stars in the Arches Cluster

    Donald F. Figer;Donald F. Figer;Francisco Najarro;Diane Gilmore;Mark Morris

  • SPECTROSCOPIC REDSHIFTS TO Z > 2 FOR OPTICALLY OBSCURED SOURCES DISCOVERED WITH THE SPITZER SPACE TELESCOPE

    J. R. Houck;B. T. Soifer;D. Weedman;Sarah J.U. Higdon

  • Very Strong Emission-Line Galaxies in the WISP Survey and Implications for High-Redshift Galaxies

    H. Atek;B. Siana;C. Scarlata;M. Malkan

  • Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z ~ 2. I. The Spectra

    Lin Yan;Anna Sajina;Dario Fadda;Phil Choi

Frequent Co-Authors

Claudia Scarlata
Claudia Scarlata University of Minnesota
Brian Siana
Brian Siana University of California, Riverside
Lee Armus
Lee Armus California Institute of Technology
Matthew A. Malkan
Matthew A. Malkan University of California, Los Angeles
James R. Graham
James R. Graham University of California, Berkeley
Nimish P. Hathi
Nimish P. Hathi Space Telescope Science Institute
Anton M. Koekemoer
Anton M. Koekemoer Space Telescope Science Institute
George Helou
George Helou California Institute of Technology
Vassilis Charmandaris
Vassilis Charmandaris University of Crete
Jason Surace
Jason Surace California Institute of Technology

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