World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
85
Citations
22581
World Ranking
2622
National Ranking
1295

Crystal L. Martin 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 Crystal L. Martin 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: 267 publications — 12th percentile

12% of scientists in this discipline score the same or lower.

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

Crystal L. Martin 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 Crystal L. Martin 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: 85 D-Index — 31st percentile

31% 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

  • 2003 - Fellow of Alfred P. Sloan Foundation

Overview

Crystal L. Martin is affiliated with the University of California, Santa Barbara in the United States. Their research primarily spans the fields of physics and astronomy, with a specific focus on astronomy and astrophysics, instrumentation, spectroscopy, nuclear and high energy physics, and general health professions.

Their work contributes to several core topics in the discipline, including:

  • Galaxies: Formation, Evolution, Phenomena
  • Astrophysics and Star Formation Studies
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Spectroscopy and Laser Applications

Among frequent co-authors with whom they have collaborated on multiple publications are Danielle A. Berg, Bethan L. James, Matthew Hayes, Karla Z. Arellano-Córdova, and Xinfeng Xu.

Their research has been published predominantly in the following venues:

  • The Astrophysical Journal
  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal Supplement Series
  • OPAL (Open@LaTrobe) (La Trobe University)

Several recent papers authored or co-authored by Crystal L. Martin include:

  • "COSMOS-Web: An Overview of the JWST Cosmic Origins Survey" (2023) published in The Astrophysical Journal
  • "The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas*" (2022) published in The Astrophysical Journal Supplement Series
  • "COSMOS-Web: Intrinsically Luminous z ≳ 10 Galaxy Candidates Test Early Stellar Mass Assembly" (2024) published in The Astrophysical Journal
  • "Possible signatures of a cold-flow disk from muse using a z ~ to 1 galaxy-quasar pair toward SDSS J1422-0001" (2024) published in OPAL (Open@LaTrobe) (La Trobe University)
  • "Kinematics of Circumgalactic Gas: Feeding Galaxies and Feedback" (2024) published in OPAL (Open@LaTrobe) (La Trobe University)

In recognition of contributions to their field, Crystal L. Martin was awarded the title of Fellow of the Alfred P. Sloan Foundation in 2003.

Best Publications

  • Mapping Large-Scale Gaseous Outflows in Ultraluminous Galaxies with Keck II ESI Spectra: Variations in Outflow Velocity with Galactic Mass

    Crystal L. Martin

  • Star Formation Thresholds in Galactic Disks

    Crystal L. Martin;Robert C. Kennicutt

  • Properties of Galactic Outflows: Measurements of the Feedback from Star Formation

    Crystal L. Martin

  • The Metal Content of Dwarf Starburst Winds: Results from Chandra Observations of NGC 1569*

    Crystal L. Martin;Crystal L. Martin;Crystal L. Martin;Henry A. Kobulnicky;Timothy M. Heckman

  • EVIDENCE FOR UBIQUITOUS COLLIMATED GALACTIC-SCALE OUTFLOWS ALONG THE STAR-FORMING SEQUENCE AT z ∼ 0.5

    Kate H. R. Rubin;Kate H. R. Rubin;J. Xavier Prochaska;J. Xavier Prochaska;David C. Koo;Andrew C. Phillips

  • Demographics and Physical Properties of Gas Out/Inflows at 0.4 < z < 1.4

    Crystal L. Martin;Alice E. Shapley;Alison L. Coil;Katherine A. Kornei

  • The Impact of Star Formation on the Interstellar Medium in Dwarf Galaxies. II. The Formation of Galactic Winds

    Crystal L. Martin

  • Recent Star Formation in the Extreme Outer Disk of M83

    D. A. Thilker;L. Bianchi;S. Boissier;A. Gil de Paz

  • DEMOGRAPHICS AND PHYSICAL PROPERTIES OF GAS OUTFLOWS/INFLOWS AT 0.4 < z < 1.4

    Crystal L. Martin;Alice E. Shapley;Alison L. Coil;Alison L. Coil;Katherine A. Kornei

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

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

  • THE PERSISTENCE OF COOL GALACTIC WINDS IN HIGH STELLAR MASS GALAXIES BETWEEN z ~ 1.4 AND ~ 1

    Kate H. R. Rubin;Benjamin J. Weiner;David C. Koo;Crystal L. Martin

  • Ly$lpha$ emission from Green Peas: the role of circumgalactic gas density, covering, and kinematics

    Alaina Henry;Claudia Scarlata;Crystal L. Martin;Dawn Erb

  • Lyα Emission from Green Peas: The Role of Circumgalactic Gas Density, Covering, and Kinematics

    Alaina Henry;Claudia M Scarlata;Crystal L. Martin;Dawn Erb

  • Physical properties of galactic winds using background quasars

    N. Bouché;N. Bouché;N. Bouché;W. Hohensee;R. Vargas;G. G. Kacprzak

  • The Impact of Star Formation on the Interstellar Medium. I. The Excitation of Diffuse, Warm Ionized Gas in Dwarf Galaxies*

    Crystal L. Martin;Crystal L. Martin

  • Discovery of a Giant Lya Emitter Near the Reionization Epoch

    Masami Ouchi;Yoshiaki Ono;Eiichi Egami;Tomoki Saito

  • Dust extinction from Balmer decrements of star-forming galaxies at 0.75<z<1.5 with HST/WFC3 spectroscopy from the WISP survey

    A. Domínguez;B. Siana;A. L. Henry;C. Scarlata

  • DUST EXTINCTION FROM BALMER DECREMENTS OF STAR-FORMING GALAXIES AT 0.75 z 1.5 WITH HUBBLE SPACE TELESCOPE/WIDE-FIELD-CAMERA 3 SPECTROSCOPY FROM THE WFC3 INFRARED SPECTROSCOPIC PARALLEL SURVEY

    A. Domínguez;B. Siana;A. L. Henry;C. Scarlata

  • Signatures of Cool Gas Fueling a Star-Forming Galaxy at Redshift 2.3

    N. Bouché;N. Bouché;M. T. Murphy;G. G. Kacprzak;C. Péroux

  • Very Strong Emission-line Galaxies in the WFC3 Infrared Spectroscopic Parallel Survey and Implications for High-redshift Galaxies

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

Frequent Co-Authors

Harry I. Teplitz
Harry I. Teplitz California Institute of Technology
Claudia Scarlata
Claudia Scarlata University of Minnesota
Alan Dressler
Alan Dressler Carnegie Institution for Science
Nimish P. Hathi
Nimish P. Hathi Space Telescope Science Institute
Brian Siana
Brian Siana University of California, Riverside
Jennifer M. Lotz
Jennifer M. Lotz Space Telescope Science Institute
Henry C. Ferguson
Henry C. Ferguson Space Telescope Science Institute
Timothy M. Heckman
Timothy M. Heckman Johns Hopkins University
Masami Ouchi
Masami Ouchi University of Tokyo
David Schiminovich
David Schiminovich Columbia University

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