Astrophysics with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
Challenges for ΛCDM: An update
A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …
few years as the accuracy of cosmological observations improves. In this review we discuss …
The James Webb space telescope mission
JP Gardner, JC Mather, R Abbott, JS Abell… - Publications of the …, 2023 - iopscience.iop.org
We summarize the history, concept, scientific program, and technical performance of the
James Webb Space Telescope (JWST, Webb; Gardner et al. 2006). This paper points to and …
James Webb Space Telescope (JWST, Webb; Gardner et al. 2006). This paper points to and …
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 …
Modules for experiments in stellar astrophysics (MESA): time-dependent convection, energy conservation, automatic differentiation, and infrastructure
We update the capabilities of the open-knowledge software instrument Modules for
Experiments in Stellar Astrophysics (MESA). The new auto _ diff module implements …
Experiments in Stellar Astrophysics (MESA). The new auto _ diff module implements …
Overview of the instrumentation for the dark energy spectroscopic instrument
B Abareshi, J Aguilar, S Ahlen, S Alam… - The Astronomical …, 2022 - iopscience.iop.org
The goal of the Dark Energy Spectroscopic Instrument (DESI) is to determine the nature of
dark energy through the most precise measurement of the expansion history of the universe …
dark energy through the most precise measurement of the expansion history of the universe …
[HTML][HTML] The early data release of the Dark Energy Spectroscopic Instrument
D Collaboration, AG Adame, J Aguilar… - The Astronomical …, 2024 - escholarship.org
The Dark Energy Spectroscopic Instrument (DESI) completed its 5 month Survey Validation
in 2021 May. Spectra of stellar and extragalactic targets from Survey Validation constitute …
in 2021 May. Spectra of stellar and extragalactic targets from Survey Validation constitute …
In the realm of the Hubble tension—a review of solutions
The simplest ΛCDM model provides a good fit to a large span of cosmological data but
harbors large areas of phenomenology and ignorance. With the improvement of the number …
harbors large areas of phenomenology and ignorance. With the improvement of the number …
Improving the open cluster census-II. An all-sky cluster catalogue with Gaia DR3
EL Hunt, S Reffert - Astronomy & Astrophysics, 2023 - aanda.org
Context. Data from the Gaia satellite are revolutionising our understanding of the Milky Way.
With every new data release, there is a need to update the census of open clusters. Aims …
With every new data release, there is a need to update the census of open clusters. Aims …
Estimating distances from parallaxes. V. Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3
Stellar distances constitute a foundational pillar of astrophysics. The publication of 1.47
billion stellar parallaxes from Gaia is a major contribution to this. Despite Gaia's precision …
billion stellar parallaxes from Gaia is a major contribution to this. Despite Gaia's precision …