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Peter H. Hauschildt

Peter H. Hauschildt

Universität Hamburg
Germany

D-Index & Metrics

Physics

D-Index
105
Citations
44790
World Ranking
1375
National Ranking
119

Peter H. Hauschildt 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 Peter H. Hauschildt 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: 606 publications — 69th percentile

69% of scientists in this discipline score the same or lower.

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

Peter H. Hauschildt 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 Peter H. Hauschildt 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: 105 D-Index — 63rd percentile

63% of scientists in this discipline score the same or lower.

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

Overview

Peter H. Hauschildt is affiliated with Universität Hamburg in Germany. Their research primarily focuses on Physics and Astronomy, with a detailed specialization in Astronomy and Astrophysics. Their work also extends into related subfields including Spectroscopy, Instrumentation, Atmospheric Science, and Aerospace Engineering.

Their research topics consistently revolve around areas such as:

  • Stellar, planetary, and galactic studies
  • Astrophysics and star formation studies
  • Spectroscopy and laser applications
  • Astronomy and astrophysical research
  • Gamma-ray bursts and supernovae
  • Astro and planetary science
  • Atmospheric ozone and climate

Hauschildt has contributed to various scientific publications with notable papers including:

  • "A comparison between X-shooter spectra and PHOENIX models across the HR-diagram," published in 2021 in Springer Link (Chiba Institute of Technology)
  • "EMISSA (Exploring Millimeter Indicators of Solar-Stellar Activity)," published in 2021 in Springer Link (Chiba Institute of Technology)
  • "EMISSA (Exploring millimetre indicators of solar-stellar activity)," published in 2022 in Astronomy and Astrophysics
  • "OPTAB: Public code for generating gas opacity tables for radiation hydrodynamics simulations," published in 2021 in Astronomy and Astrophysics
  • "The PEPSI Exoplanet Transit Survey (PETS) - V. New Naₐ transmission spectra indicate a quieter atmosphere on HD 189733b," published in 2024 in Monthly Notices of the Royal Astronomical Society

The venues where Hauschildt frequently publishes highlight the interdisciplinary nature of their work. These include:

  • Astronomy and Astrophysics
  • Springer Link (Chiba Institute of Technology)
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society

Collaboration is a significant component of Hauschildt's research. Frequent coauthors include:

  • Atul Mohan
  • Sven Wedemeyer
  • E. Baron
  • Sneha Pandit
  • Maryam Saberi

Their collaborative network and publication record illustrate a sustained engagement with contemporary astrophysics and related spectroscopic techniques, contributing to ongoing advancements in the understanding of stellar and planetary atmospheres, as well as radiation hydrodynamics simulations.

Best Publications

  • Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945

    I. Baraffe;G. Chabrier;T. Barman;F. Allard

  • The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$

    Peter H. Hauschildt;E. Baron

  • Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458

    I. Baraffe;G. Chabrier;T. S. Barman;F. Allard

  • A new extensive library of PHOENIX stellar atmospheres and synthetic spectra

    T.-O. Husser;S. Wende-von Berg;S. Dreizler;D. Homeier;D. Homeier

  • A new extensive library of PHOENIX stellar atmospheres and synthetic spectra

    Tim-Oliver Husser;Sebastian Wende von Berg;Stefan Dreizler;Derek Homeier

  • Evolutionary Models for Very Low-Mass Stars and Brown Dwarfs with Dusty Atmospheres

    G. Chabrier;G. Chabrier;I. Baraffe;I. Baraffe;F. Allard;P. Hauschildt

  • The NextGen Model Atmosphere Grid for 3000 ≤ Teff ≤ 10,000 K

    Peter H. Hauschildt;E. Baron

  • LOW-TEMPERATURE OPACITIES

    Jason W. Ferguson;David R. Alexander;Travis Barman

  • THE LIMITING EFFECTS OF DUST IN BROWN DWARF MODEL ATMOSPHERES

    Peter H. Hauschildt;David R. Alexander;Akemi Tamanai

  • Evolutionary models for low-mass stars and brown dwarfs: uncertainties and limits at very young ages

    I. Baraffe;G. Chabrier;F. Allard;P. H. Hauschildt

  • Model atmospheres for M (sub)dwarf stars. 1: The base model grid

    Peter H. Hauschildt

  • MODEL ATMOSPHERES OF VERY LOW MASS STARS AND BROWN DWARFS

    Peter H. Hauschildt;David R. Alexander;Sumner Starrfield

  • The NEXTGEN Model Atmosphere Grid. II. Spherically Symmetric Model Atmospheres for Giant Stars with Effective Temperatures between 3000 and 6800 K

    Peter H. Hauschildt;Jason Ferguson;E. Baron

  • Model Atmospheres for M (Sub)Dwarfs: I. The base model grid

    Peter H. Hauschildt

  • Evidence for a Spectroscopic Sequence among Type Ia Supernovae

    Peter Nugent;Mark Phillips;E. Baron;David Branch

  • Evidence for a Spectroscopic Sequence Among SNe Ia

    Peter Nugent;Mark Phillips;E. Baron;David Branch

  • Evolutionary Stellar Population Synthesis at High Spectral Resolution: Optical Wavelengths

    R. M. Gonzalez Delgado;Miguel Cervino;L. Pires Martins;Claus Leitherer

  • Evolutionary stellar population synthesis at high spectral resolution: optical wavelengths

    R. M. González Delgado;M. Cerviño;L. P. Martins;C. Leitherer

  • New limb-darkening coefficients for Phoenix/1d model atmospheres - II. Calculations for 5000 K ≤ Teff ≤ 10 000 K Kepler, CoRot, Spitzer, uvby, UBVRIJHK, Sloan, and 2MASS photometric systems

    A. Claret;P. H. Hauschildt;S. Witte

  • Infrared Spectra and Spectral Energy Distributions of Late M and L Dwarfs

    S. K. Leggett;F. Allard;T. R. Geballe;P. H. Hauschildt

Frequent Co-Authors

E. Baron
E. Baron University of Oklahoma
Sumner Starrfield
Sumner Starrfield Arizona State University
Isabelle Baraffe
Isabelle Baraffe École Normale Supérieure de Lyon
Gilles Chabrier
Gilles Chabrier École Normale Supérieure de Lyon
Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
D. Montes
D. Montes Complutense University of Madrid
Ansgar Reiners
Ansgar Reiners University of Göttingen
Ignasi Ribas
Ignasi Ribas Institute of Space Sciences
José A. Caballero
José A. Caballero Spanish National Research Council
M. R. Zapatero Osorio
M. R. Zapatero Osorio Spanish National Research Council

External Links

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