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 …
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 …
S Alam, M Aubert, S Avila, C Balland, JE Bautista… - Physical Review D, 2021 - APS
We present the cosmological implications from final measurements of clustering using galaxies, quasars, and Ly α forests from the completed Sloan Digital Sky Survey (SDSS) …
H Brunner, T Liu, G Lamer, A Georgakakis… - Astronomy & …, 2022 - aanda.org
Context. The eROSITA X-ray telescope on board the Spectrum-Poentgen-Gamma (SPG) observatory combines a large field of view and a large collecting area in the energy range …
H Jönsson, JA Holtzman, CA Prieto… - The Astronomical …, 2020 - iopscience.iop.org
The spectral analysis and data products in Data Release 16 (DR16; 2019 December) from the high-resolution near-infrared Apache Point Observatory Galactic Evolution Experiment …
OL Creevey, R Sordo, F Pailler, Y Frémat… - Astronomy & …, 2023 - aanda.org
Gaia Data Release 3 contains a wealth of new data products for the community. Astrophysical parameters are a major component of this release, and were produced by the …
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) …
KG Stassun, RJ Oelkers, M Paegert… - The Astronomical …, 2019 - iopscience.iop.org
We describe the catalogs assembled and the algorithms used to populate the revised TESS Input Catalog (TIC), based on the incorporation of the Gaia second data release. We also …
BD Johnson, J Leja, C Conroy… - The Astrophysical …, 2021 - iopscience.iop.org
Inference of the physical properties of stellar populations from observed photometry and spectroscopy is a key goal in the study of galaxy evolution. In recent years, the quality and …