Direct detection of WIMP dark matter: concepts and status
M Schumann - Journal of Physics G: Nuclear and Particle …, 2019 - iopscience.iop.org
The existence of dark matter as evidenced by numerous indirect observations is one of the
most important indications that there must be physics beyond the Standard Model of particle …
most important indications that there must be physics beyond the Standard Model of particle …
Neutrino mass ordering from oscillations and beyond: 2018 status and future prospects
PF De Salas, S Gariazzo, O Mena… - Frontiers in Astronomy …, 2018 - frontiersin.org
The ordering of the neutrino masses is a crucial input for a deep understanding of flavor
physics, and its determination may provide the key to establish the relationship among the …
physics, and its determination may provide the key to establish the relationship among the …
DESI 2024 VI: Cosmological constraints from the measurements of baryon acoustic oscillations
AG Adame, J Aguilar, S Ahlen, S Alam… - arXiv preprint arXiv …, 2024 - arxiv.org
We present cosmological results from the measurement of baryon acoustic oscillations
(BAO) in galaxy, quasar and Lyman-$\alpha $ forest tracers from the first year of …
(BAO) in galaxy, quasar and Lyman-$\alpha $ forest tracers from the first year of …
Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point …
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) …
galaxies, quasars, and Ly α forests from the completed Sloan Digital Sky Survey (SDSS) …
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample …
JE Bautista, R Paviot, M Vargas Magaña… - Monthly Notices of …, 2021 - academic.oup.com
We present the cosmological analysis of the configuration-space anisotropic clustering in
the completed Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic …
the completed Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic …
Planck 2018 results-VI. Cosmological parameters
We present cosmological parameter results from the final full-mission Planck measurements
of the cosmic microwave background (CMB) anisotropies, combining information from the …
of the cosmic microwave background (CMB) anisotropies, combining information from the …
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
We present the first cosmology results from large-scale structure using the full 5000 deg 2 of
imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis …
imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis …
Dark Energy Survey Year 3 results: A 2.7% measurement of baryon acoustic oscillation distance scale at redshift 0.835
We present angular diameter measurements obtained by measuring the position of baryon
acoustic oscillations (BAO) in an optimized sample of galaxies from the first three years of …
acoustic oscillations (BAO) in an optimized sample of galaxies from the first three years of …
The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15
AJ Ross, L Samushia, C Howlett… - Monthly Notices of …, 2015 - academic.oup.com
We create a sample of spectroscopically identified galaxies with z< 0.2 from the Sloan
Digital Sky Survey (SDSS) Data Release 7 (DR7), covering 6813 deg2. Galaxies are chosen …
Digital Sky Survey (SDSS) Data Release 7 (DR7), covering 6813 deg2. Galaxies are chosen …
The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between …
M Ata, F Baumgarten, J Bautista… - Monthly Notices of …, 2018 - academic.oup.com
We present measurements of the Baryon Acoustic Oscillation (BAO) scale in redshift-space
using the clustering of quasars. We consider a sample of 147 000 quasars from the …
using the clustering of quasars. We consider a sample of 147 000 quasars from the …