Modeling the panchromatic spectral energy distributions of galaxies
C Conroy - Annual Review of Astronomy and Astrophysics, 2013 - annualreviews.org
The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …
property of the system, including the star-formation history, metal content, abundance …
Models of very-low-mass stars, brown dwarfs and exoplanets
F Allard, D Homeier, B Freytag - … Transactions of the …, 2012 - royalsocietypublishing.org
Within the next few years, GAIA and several instruments aiming to image extrasolar planets
will be ready. In parallel, low-mass planets are being sought around red dwarfs, which offer …
will be ready. In parallel, low-mass planets are being sought around red dwarfs, which offer …
A new set of atmosphere and evolution models for cool T–Y brown dwarfs and giant exoplanets
We present a new set of solar metallicity atmosphere and evolutionary models for very cool
brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere …
brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere …
A new extensive library of PHOENIX stellar atmospheres and synthetic spectra
TO Husser, S Wende-von Berg, S Dreizler… - Astronomy & …, 2013 - aanda.org
Aims. We present a new library of high-resolution synthetic spectra based on the stellar
atmosphere code PHOENIX that can be used for a wide range of applications of spectral …
atmosphere code PHOENIX that can be used for a wide range of applications of spectral …
Improving PARSEC models for very low mass stars
Many stellar models present difficulties in reproducing basic observational relations of very
low mass stars (VLMS), including the mass–radius relation and the optical colour …
low mass stars (VLMS), including the mass–radius relation and the optical colour …
The MUSCLES treasury survey. I. Motivation and overview
Ground-and space-based planet searches employing radial velocity techniques and transit
photometry have detected thousands of planet-hosting stars in the Milky Way. With so many …
photometry have detected thousands of planet-hosting stars in the Milky Way. With so many …
ExoMol molecular line lists–XXXIII. The spectrum of Titanium Oxide
LK McKemmish, T Masseron… - Monthly Notices of …, 2019 - academic.oup.com
Accurate line lists are crucial for correctly modelling a variety of astrophysical phenomena,
including stellar photospheres and the atmospheres of extrasolar planets. This paper …
including stellar photospheres and the atmospheres of extrasolar planets. This paper …
Stellar population synthesis at the resolution of 2003
G Bruzual, S Charlot - Monthly Notices of the Royal Astronomical …, 2003 - academic.oup.com
We present a new model for computing the spectral evolution of stellar populations at ages
between 1× 105 and 2× 1010 yr at a resolution of 3 Å across the whole wavelength range …
between 1× 105 and 2× 1010 yr at a resolution of 3 Å across the whole wavelength range …
The propagation of uncertainties in stellar population synthesis modeling. III. Model calibration, comparison, and evaluation
C Conroy, JE Gunn - The Astrophysical Journal, 2010 - iopscience.iop.org
Stellar population synthesis (SPS) provides the link between the stellar and dust content of
galaxies and their observed spectral energy distributions. In the present work, we perform a …
galaxies and their observed spectral energy distributions. In the present work, we perform a …
An optical spectroscopic study of T Tauri stars. I. Photospheric properties
Estimates of the mass and age of young stars from their location in the HR diagram are
limited by not only the typical observational uncertainties that apply to field stars, but also by …
limited by not only the typical observational uncertainties that apply to field stars, but also by …