activity
20162023
most citedThe Betelgeuse Project: Constraints from Rotation

33 citations · 126 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2023★ 3 cited

Galaxy bias in the era of LSST: perturbative bias expansions

Andrina Nicola, Boryana Hadzhiyska, Nathan Findlay +14

Upcoming imaging surveys will allow for high signal-to-noise measurements of galaxy clustering at small scales. In this work, we present the results of the LSST bias challenge, the…

astro-ph.CO2023★ 8 cited

Improving initialization and evolution accuracy of cosmological neutrino simulations

James M. Sullivan, J. D. Emberson, Salman Habib +1

Neutrino mass constraints are a primary focus of current and future large-scale structure (LSS) surveys. Non-linear LSS models rely heavily on cosmological simulations -- the impac…

astro-ph.CO2021★ 20 cited

An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies

James M. Sullivan, Uros Seljak, Sukhdeep Singh

We update Halo Zeldovich Perturbation Theory (HZPT), an analytic model for the two-point statistics of dark matter, to describe halo and galaxy clustering, and galaxy-matter cross-…

astro-ph.HE2020★ 10 cited

The Betelgeuse Project III: Merger Characteristics

J. M. Sullivan, S. Nance, J. Craig Wheeler

We previously proposed that Betelgeuse might have been spun up by accreting a companion of about 1 solar mass. Here we explore in more detail the possible systematics of such a mer…

astro-ph.CO2018★ 13 cited

Minimum star-forming halo mass in axion cosmology

James M. Sullivan, Shingo Hirano, Volker Bromm

Elucidating the particle physics nature of dark matter (DM) is one of the great challenges in modern science. The current lack of any direct DM detections in the laboratory heighte…

astro-ph.SR2018★ 12 cited

The Betelgeuse Project II: Asteroseismology

S. Nance, J. M. Sullivan, M. Diaz +1

We explore the question of whether the interior state of massive red supergiant supernova progenitors can be effectively probed with asteroseismology. We have computed a suite of t…