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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 …
Assessing vegetation function with imaging spectroscopy
Healthy vegetation function supports diverse biological communities and ecosystem
processes, and provides crops, forest products, forage, and countless other benefits …
processes, and provides crops, forest products, forage, and countless other benefits …
The seventeenth data release of the Sloan Digital Sky Surveys: Complete release of MaNGA, MaStar, and APOGEE-2 data
N Abdurro'uf, K Accetta, C Aerts, V Silva Aguirre… - The Astrophysical …, 2022 - osti.gov
This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky
Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the …
Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the …
The seventeenth data release of the Sloan Digital Sky Surveys: Complete release of MaNGA, MaStar, and APOGEE-2 data
K Accetta, C Aerts, VS Aguirre… - The Astrophysical …, 2022 - iopscience.iop.org
The Sloan Digital Sky Surveys (SDSS) have been almost continuously observing the skies
for over 20 yr, since the project began with a first phase in 1998 (SDSS-I; York et al. 2000) …
for over 20 yr, since the project began with a first phase in 1998 (SDSS-I; York et al. 2000) …
Improving the full spectrum fitting method: accurate convolution with Gauss–Hermite functions
M Cappellari - Monthly Notices of the Royal Astronomical …, 2017 - academic.oup.com
I start by providing an updated summary of the penalized pixel-fitting (ppxf) method that is
used to extract the stellar and gas kinematics, as well as the stellar population of galaxies …
used to extract the stellar and gas kinematics, as well as the stellar population of galaxies …
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 …
Measuring reddening with Sloan Digital Sky Survey stellar spectra and recalibrating SFD
We present measurements of dust reddening using the colors of stars with spectra in the
Sloan Digital Sky Survey. We measure reddening as the difference between the measured …
Sloan Digital Sky Survey. We measure reddening as the difference between the measured …
Planck 2015 results-X. Diffuse component separation: Foreground maps
R Adam, PAR Ade, N Aghanim, MIR Alves… - Astronomy & …, 2016 - aanda.org
Planck has mapped the microwave sky in temperature over nine frequency bands between
30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz …
30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz …
The sixth data release of the radial velocity experiment (rave). i. survey description, spectra, and radial velocities
M Steinmetz, G Matijevič, H Enke, T Zwitter… - The Astronomical …, 2020 - iopscience.iop.org
Abstract The Radial Velocity Experiment (RAVE) is a magnitude-limited (9< I< 12)
spectroscopic survey of Galactic stars randomly selected in Earth's southern hemisphere …
spectroscopic survey of Galactic stars randomly selected in Earth's southern hemisphere …
Evolutionary stellar population synthesis with MILES–I. The base models and a new line index system
We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity
stellar populations (SSPs) covering the full optical spectral range at moderately high …
stellar populations (SSPs) covering the full optical spectral range at moderately high …