Peter H. Hauschildt

发表

A Comparison of the Infrared Spectra of Two Very Late-type M Dwarfs with Different Gravities

Jonathan Tennyson, Hugh R. A. Jones, S. Viti, 1998 .

Multi-level non-LTE radiative transfer in expanding shells

Peter H. Hauschildt, P. Hauschildt, 1993 .

Testing spherical, expanding, line-blanketed model atmospheres of giant stars with interferometry

Peter H. Hauschildt, Jason Paul Aufdenberg, P. Hauschildt, 2003, SPIE Astronomical Telescopes + Instrumentation.

A 3D radiative transfer framework: XII. Many-core, vector and GPU methods

Peter H. Hauschildt, E. Baron, 2021, Astron. Comput..

Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program. II. Wavelength Parallelization

Peter H. Hauschildt, France Allard, E. Baron, 1996, astro-ph/9709238.

Detailed Spectroscopic Analysis of SN 1987A: The Distance to the Large Magellanic Cloud Using the Spectral-fitting Expanding Atmosphere Method

Peter Nugent, David Branch, Peter H. Hauschildt, 2002 .

Multiwavelength analyses of the extraordinary nova LMC 1991

Steven N. Shore, M. Della Valle, Sumner Starrfield, 2001 .

The Physics of Early Nova Spectra

Steven N. Shore, Sumner Starrfield, Peter H. Hauschildt, 1995 .

Parallel implementation of the PHOENIX generalized stellar atmosphere program. II. Wavelength parallelization

Peter H. Hauschildt, E. Baron, 1998 .

THE LIMITING EFFECTS OF DUST IN BROWN DWARF MODEL ATMOSPHERES

David R. Alexander, Peter H. Hauschildt, France Allard, 2001 .

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

David R. Alexander, Peter H. Hauschildt, France Allard, 1999, astro-ph/9907194.

Type IIP Supernovae as Cosmological Probes: A Spectral-fitting Expanding Atmosphere Model Distance to SN 1999em

Peter Nugent, David Branch, Peter H. Hauschildt, 2004 .

Low-Temperature Opacities

David R. Alexander, Travis Barman, Peter H. Hauschildt, 2005, astro-ph/0502045.

A Grid of Non-LTE Model Atmospheres for White Dwarfs in Cataclysmic Variables

Sumner Starrfield, Peter H. Hauschildt, Jason Paul Aufdenberg, 2000 .

Exoplanet characterisation observatory

Matthew Joseph Griffin, Enzo Pascale, Sergei N. Yurchenko, 2012 .

Early Infrared Spectral Development of V1187 Scorpii (Nova Scorpii 2004 No. 2)

M. F. Bode, Matthew A. Greenhouse, D. K. Lynch, 2004 .

A Chandra Low Energy Transmission Grating Spectrometer Observation of V4743 Sagittarii: A Supersoft X-Ray Source and a Violently Variable Light Curve

J. Krautter, Koji Mukai, R. M. Wagner, 2003 .

Ab initio modeling of molecular IR spectra of astrophysical interest: Application to CH4

Ralf Schneider, Robert Warmbier, Joel M. Bowman, 2009 .

Phase-dependent Properties of Extrasolar Giant Planet Atmospheres

Travis S Barman, F. Allard, Peter H. Hauschildt, 2004 .

Infrared Spectra of Low-Mass Stars: Toward a Temperature Scale for Red Dwarfs

Graham Berriman, Sandy K. Leggett, F. Allard, 1996 .

Detecting planets around very cool dwarfs at near infrared wavelengths with the radial velocity technique

Eduardo L. Martin, Peter H. Hauschildt, P. Hauschildt, 2011, 1105.2287.

TiO and H2O Absorption Lines in Cool Stellar Atmospheres

Peter H. Hauschildt, France Allard, F. Allard, 2000, astro-ph/0008465.

The science of EChO

Enzo Pascale, Jonathan Tennyson, Gautam Vasisht, 2010, Proceedings of the International Astronomical Union.

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

Peter H. Hauschildt, France Allard, F. Allard, 1995, astro-ph/9601150.

Modeling CHANDRA low energy transmission grating spectrometer observations of classical novae with PHOENIX - I. V4743 Sagittarii

Sumner Starrfield, Peter H. Hauschildt, Jan-Uwe Ness, 2004 .

Model atmospheres and spectra: The role of dust

David R. Alexander, Tristan Guillot, Peter H. Hauschildt, 2003 .

Irradiated planets

Peter H. Hauschildt, France Allard, Travis S. Barman, 2001, astro-ph/0104262.

Time-resolved Spectroscopy of AL Comae

V. S. Dhillon, Steve Bruce Howell, Peter H. Hauschildt, 1998 .

An Effective Temperature Scale for Late-M and L Dwarfs, from Resonance Absorption Lines of Cs I and Rb I

Thierry Forveille, Eduardo L. Martin, Xavier Delfosse, 2000, astro-ph/0003033.

The limb-darkening for spherically symmetric NextGen model atmospheres: A-G main-sequence and sub-giant stars

Antonio Claret, Peter H. Hauschildt, P. Hauschildt, 2003 .

A new extensive library of PHOENIX stellar atmospheres and synthetic spectra

Ansgar Reiners, Stefan Dreizler, Tim-Oliver Husser, 2013, 1303.5632.

Phase-dependent Properties of Extrasolar Planet Atmospheres

Peter H. Hauschildt, France Allard, Travis S. Barman, 2005 .