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Daniel P. Stark

D-Index & Metrics

Physics

D-Index
103
Citations
30582
World Ranking
1512
National Ranking
794

Daniel P. Stark 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 P. Stark 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: 311 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.

Daniel P. Stark 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 P. Stark 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: 103 D-Index — 60th percentile

60% of scientists in this discipline score the same or lower.

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

Overview

Daniel P. Stark is affiliated with the University of Arizona in the United States. Their research primarily spans the broad field of Physics and Astronomy, with a focus on several subfields including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Electrical and Electronic Engineering, and Spectroscopy.

The main topics covered in Daniel P. Stark's body of work include:

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

Daniel P. Stark has collaborated frequently with several researchers, including:

  • Ryan Endsley
  • S. Charlot
  • Michael W. Topping
  • Renske Smit
  • Jacopo Chevallard

The scientist's research has been published predominantly in the following venues:

  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal
  • Astronomy and Astrophysics
  • Nature Astronomy

Representative recent papers authored by Daniel P. Stark include:

  • Spectroscopic confirmation of four metal-poor galaxies at z = 10.3-13.2, 2023, Nature Astronomy
  • JADES NIRSpec Spectroscopy of GN-z11: Lyman-α emission and possible enhanced nitrogen abundance in a z = 10.60 luminous galaxy, 2023, Astronomy and Astrophysics
  • Identification and properties of intense star-forming galaxies at redshifts z > 10, 2023, Nature Astronomy
  • Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe, 2022, The Astrophysical Journal
  • A JWST/NIRCam study of key contributors to reionization: the star-forming and ionizing properties of UV-faint z ∼ 7−8 galaxies, 2023, Monthly Notices of the Royal Astronomical Society

Best Publications

  • The Abundance of Star-Forming Galaxies in the Redshift Range 8.5 to 12: New Results from the 2012 Hubble Ultra Deep Field Campaign

    Richard S Ellis;Ross J McLure;James S Dunlop;Brant E Robertson

  • New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign

    Brant E. Robertson;Steven R. Furlanetto;Evan Schneider;Stephane Charlot

  • Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies: - I. New constraints on cosmic reionisation from the luminosity and redshift-dependent fraction of Lyman-alpha emission

    Daniel P. Stark;Richard S. Ellis;Kuenley Chiu;Masami Ouchi

  • Keck spectroscopy of faint 3 < z < 7 Lyman break galaxies – I. New constraints on cosmic reionization from the luminosity and redshift-dependent fraction of Lyman α emission

    Daniel P. Stark;Richard S. Ellis;Kuenley Chiu;Masami Ouchi

  • The Abundance of Star-forming Galaxies in the Redshift Range 8.5-12: New Results from the 2012 Hubble Ultra Deep Field Campaign

    Richard S. Ellis;Ross J. McLure;James S. Dunlop;Brant E. Robertson

  • A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble Ultra-Deep Field imaging

    R. J. McLure;J. S. Dunlop;R. A. A. Bowler;E. Curtis-Lake

  • THE EVOLUTIONARY HISTORY OF LYMAN BREAK GALAXIES BETWEEN REDSHIFT 4 AND 6: OBSERVING SUCCESSIVE GENERATIONS OF MASSIVE GALAXIES IN FORMATION

    Daniel P. Stark;Daniel P. Stark;Richard S. Ellis;Richard S. Ellis;Andrew Bunker;Kevin Bundy;Kevin Bundy

  • Line Emitting Galaxies Beyond a Redshift of 7: An Improved Method for Estimating the Evolving Neutrality of the Intergalactic Medium

    Matthew A. Schenker;Richard S. Ellis;Nick P. Konidaris;Daniel P. Stark

  • Keck Spectroscopy of Faint 3>z>7 Lyman Break Galaxies: A High Fraction of Line Emitters at Redshift Six

    Daniel P. Stark;Richard S. Ellis;Masami Ouchi

  • Intense star formation within resolved compact regions in a galaxy at z = 2.3

    A.M. Swinbank;I. Smail;S. Longmore;A.I. Harris

  • KECK SPECTROSCOPY OF 3 < z < 7 FAINT LYMAN BREAK GALAXIES: THE IMPORTANCE OF NEBULAR EMISSION IN UNDERSTANDING THE SPECIFIC STAR FORMATION RATE AND STELLAR MASS DENSITY

    Daniel P. Stark;Matthew A. Schenker;Richard Ellis;Brant Robertson

  • Early star-forming galaxies and the reionization of the Universe

    Brant E. Robertson;Richard S. Ellis;James S. Dunlop;Ross J. McLure

  • Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies:- II. A High Fraction of Line Emitters at Redshift Six

    Daniel P. Stark;Richard S. Ellis;Masami Ouchi

  • Galaxies at z = 6 - 9 from the WFC3/IR imaging of the HUDF

    R.J. McLure;J.S. Dunlop;M. Cirasuolo;A.M. Koekemoer

  • Galaxies at z= 6–9 from the WFC3/IR imaging of the Hubble Ultra Deep Field

    R. J. McLure;James Dunlop;M. Cirasuolo;M. Cirasuolo;A. M. Koekemoer

  • Lyα and C iii] emission in z = 7–9 Galaxies: accelerated reionization around luminous star-forming systems?

    Daniel P. Stark;Richard S. Ellis;Richard S. Ellis;Stéphane Charlot;Jacopo Chevallard

  • KECK SPECTROSCOPY OF FAINT 3 < z < 8 LYMAN BREAK GALAXIES: EVIDENCE FOR A DECLINING FRACTION OF EMISSION LINE SOURCES IN THE REDSHIFT RANGE 6 < z < 8

    Matthew A. Schenker;Daniel P Stark;Richard S. Ellis;Brant E Robertson

  • The intense starburst HDF 850.1 in a galaxy overdensity at z ≈ 5.2 in the Hubble Deep Field

    Fabian Walter;Roberto Decarli;Chris Carilli;Frank Bertoldi

  • Resolved spectroscopy of gravitationally lensed galaxies: recovering coherent velocity fields in subluminous z ~ 2-3 galaxies

    T. A. Jones;A. M. Swinbank;R. S. Ellis;J. Richard

  • Ultraviolet emission lines in young low-mass galaxies at z ≃ 2: physical properties and implications for studies at z > 7

    Daniel P. Stark;Johan Richard;Brian Siana;Stéphane Charlot

Frequent Co-Authors

Richard S. Ellis
Richard S. Ellis University College London
Johan Richard
Johan Richard Lyon Observatory
Brant Robertson
Brant Robertson University of California, Santa Cruz
Masami Ouchi
Masami Ouchi University of Tokyo
Michele Trenti
Michele Trenti University of Melbourne
Michele Cirasuolo
Michele Cirasuolo European Southern Observatory
Keiichi Umetsu
Keiichi Umetsu Institute of Astronomy and Astrophysics, Academia Sinica
Ross J. McLure
Ross J. McLure University of Edinburgh
James S. Dunlop
James S. Dunlop University of Edinburgh
Pascal Oesch
Pascal Oesch University of Geneva

External Links

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Best Scientists Citing Daniel P. Stark

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