activity
20182025
most citedOverview of the DESI Milky Way Survey

150 citations · 356 across the 10 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2025★ 29 cited

Data Release 1 of the Dark Energy Spectroscopic Instrument

DESI Collaboration, M. Abdul Karim, A. G. Adame +306

In 2021 May the Dark Energy Spectroscopic Instrument (DESI) collaboration began a 5-year spectroscopic redshift survey to produce a detailed map of the evolving three-dimensional s…

astro-ph.CO2024★ 5 cited

Window convolution of the galaxy clustering bispectrum

Mike Shengbo Wang, Florian Beutler, J. Aguilar +25

In galaxy survey analysis, the observed clustering statistics do not directly match theoretical predictions but rather have been processed by a window function that arises from the…

astro-ph.CO2024★ 2 cited

A comparison of shrinkage estimators of the cosmological precision matrix

Marnix J. Looijmans, Mike Shengbo Wang, Florian Beutler

The determination of the covariance matrix and its inverse, the precision matrix, is critical in the statistical analysis of cosmological measurements. The covariance matrix is typ…

astro-ph.IM2023★ 7 cited

Triumvirate: A Python/C++ package for three-point clustering measurements

Mike Shengbo Wang, Florian Beutler, Naonori S. Sugiyama

Triumvirate is a Python/C++ package for measuring the three-point clustering statistics in large-scale structure (LSS) cosmological analyses. Given a catalogue of discrete particle…

astro-ph.GA2022★ 150 cited

Overview of the DESI Milky Way Survey

Andrew P. Cooper, Sergey E. Koposov, Carlos Allende Prieto +62

We describe the Milky Way Survey (MWS) that will be undertaken with the Dark Energy Spectroscopic Instrument (DESI) on the Mayall 4m telescope at the Kitt Peak National Observatory…

astro-ph.CO2020★ 16 cited

Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses

Mike Shengbo Wang, Santiago Avila, Davide Bianchi +2

Future precision cosmology from large-scale structure experiments including the Dark Energy Spectroscopic Instrument (DESI) and Euclid will probe wider and deeper cosmic volumes th…

astro-ph.CO2020★ 41 cited

Impact of Relativistic Effects on the Primordial Non-Gaussianity Signature in the Large-Scale Clustering of Quasars

Mike Shengbo Wang, Florian Beutler, David Bacon

Relativistic effects in clustering observations have been shown to introduce scale-dependent corrections to the galaxy over-density field on large scales, which may hamper the dete…

astro-ph.CO2018★ 21 cited

Cosmological Inference from Galaxy-Clustering Power Spectrum: Gaussianization and Covariance Decomposition

Mike Shengbo Wang, Will J. Percival, Santiago Avila +2

Likelihood fitting to two-point clustering statistics made from galaxy surveys usually assumes a multivariate normal distribution for the measurements, with justification based on…

astro-ph.CO2018★ 56 cited

A Unified Analysis of Four Cosmic Shear Surveys

Chihway Chang, Michael Wang, Scott Dodelson +13

In the past few years, several independent collaborations have presented cosmological constraints from tomographic cosmic shear analyses. These analyses differ in many aspects: the…