activity
20172023
most citedSymmetries and Strings of Adjoint QCD

263 citations · 342 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2023★ 1 cited

SDSS DR17: The Cosmic Slime Value Added Catalog

Matthew C. Wilde, Oskar Elek, Joseph N. Burchett +5

The "cosmic web", the filamentary large-scale structure in a cold dark matter Universe, is readily apparent via galaxy tracers in spectroscopic surveys. However, the underlying dar…

astro-ph.GA2023★ 11 cited

CGM CASBaH: The Mass Dependence of H~I Ly-Galaxy Clustering and the Extent of the CGM

Matthew C. Wilde, Kirill Tchernyshyov, Jessica K. Werk +9

We combine datasets from the CGM and CASBaH surveys to model a transition point, , between circumgalactic and intergalactic media (CGM and IGM, respectively).…

astro-ph.GA2022★ 24 cited

The CGM Survey: Quenching and the Transformation of the Circumgalactic Medium

Kirill Tchernyshyov, Jessica K. Werk, Matthew C. Wilde +9

This study addresses how the incidence rate of strong O VI absorbers in a galaxy's circumgalactic medium (CGM) depends on galaxy mass and, independently, on the amount of star form…

astro-ph.GA2022★ 5 cited

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data

Abdurro'uf, Katherine Accetta, Conny Aerts +337

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 complete…

astro-ph.GA2021★ 38 cited

The CGM Survey: Circumgalactic O VI from dwarf to massive star-forming galaxies

K. Tchernyshyov, J. K. Werk, M. C. Wilde +9

We combine 126 new galaxy-O VI absorber pairs from the CGM survey with 123 pairs drawn from the literature to examine the simultaneous dependence of the column density of O VI…

hep-th2020★ 263 cited

Symmetries and Strings of Adjoint QCD

Zohar Komargodski, Kantaro Ohmori, Konstantinos Roumpedakis +1

We revisit the symmetries of massless two-dimensional adjoint QCD with gauge group . The dynamics is not sufficiently constrained by the ordinary symmetries and anomalies. H…