Accuracy and precision of industrial stellar abundances
P Jofré, U Heiter, C Soubiran - Annual Review of Astronomy …, 2019 - annualreviews.org
There has been an incredibly large investment in obtaining high-resolution stellar spectra for
determining chemical abundances of stars. This information is crucial to answer …
determining chemical abundances of stars. This information is crucial to answer …
Red clump stars
L Girardi - Annual Review of Astronomy and Astrophysics, 2016 - annualreviews.org
Low-mass stars in their core-helium-burning stage define the sharpest feature present in the
color-magnitude diagrams of nearby galaxy systems: the red clump (RC). This feature has …
color-magnitude diagrams of nearby galaxy systems: the red clump (RC). This feature has …
Fast and scalable Gaussian process modeling with applications to astronomical time series
The growing field of large-scale time domain astronomy requires methods for probabilistic
data analysis that are computationally tractable, even with large data sets. Gaussian …
data analysis that are computationally tractable, even with large data sets. Gaussian …
The GALAH survey: scientific motivation
GM De Silva, KC Freeman… - Monthly Notices of …, 2015 - academic.oup.com
Abstract The Galactic Archaeology with HERMES (GALAH) survey is a large high-resolution
spectroscopic survey using the newly commissioned High Efficiency and Resolution Multi …
spectroscopic survey using the newly commissioned High Efficiency and Resolution Multi …
APOGEE data releases 13 and 14: data and analysis
The data and analysis methodology used for the SDSS/APOGEE Data Releases 13 and 14
are described, highlighting differences from the DR12 analysis presented in Holtzman et al …
are described, highlighting differences from the DR12 analysis presented in Holtzman et al …
The apache point observatory galactic evolution experiment (APOGEE)
SR Majewski, RP Schiavon… - The Astronomical …, 2017 - iopscience.iop.org
Abstract The Apache Point Observatory Galactic Evolution Experiment (APOGEE), one of the
programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic …
programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic …
The second APOKASC catalog: the empirical approach
We present a catalog of stellar properties for a large sample of 6676 evolved stars with
Apache Point Observatory Galactic Evolution Experiment spectroscopic parameters and …
Apache Point Observatory Galactic Evolution Experiment spectroscopic parameters and …
Abundances, stellar parameters, and spectra from the sdss-iii/apogee survey
ABSTRACT The SDSS-III/Apache Point Observatory Galactic Evolution Experiment
(APOGEE) survey operated from 2011–2014 using the APOGEE spectrograph, which …
(APOGEE) survey operated from 2011–2014 using the APOGEE spectrograph, which …
Revised stellar properties of Kepler targets for the Q1-17 (DR25) transit detection run
The determination of exoplanet properties and occurrence rates using Kepler data critically
depends on our knowledge of the fundamental properties (such as temperature, radius, and …
depends on our knowledge of the fundamental properties (such as temperature, radius, and …
Deep learning of multi-element abundances from high-resolution spectroscopic data
Deep learning with artificial neural networks is increasingly gaining attention because of its
potential for data-driven astronomy. However, this methodology usually does not provide …
potential for data-driven astronomy. However, this methodology usually does not provide …