World's Best Scientists 2026 revealed!
Peter H. Hauschildt

Peter H. Hauschildt

D-Index & Metrics

Physics

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

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

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