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20192023
most citedA data science platform to enable time-domain astronomy

91 citations · 188 across the 9 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2023

Insight into the Formation of Pic b through the Composition of Its Parent Protoplanetary Disk as Revealed by the Pic Moving Group Member HD 181327

Henrique Reggiani, Jhon Yana Galarza, Kevin C. Schlaufman +5

It has been suggested that Pic b has a supersolar metallicity and subsolar C/O ratio. Assuming solar carbon and oxygen abundances for the star Pic and therefore the planet'…

astro-ph.SR2023★ 6 cited

Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for SX Phoenicis Variables in the gri-Band

Chow-Choong Ngeow, Anupam Bhardwaj, Matthew J. Graham +4

SX Phoenicis (SXP) variables are short period pulsating stars that exhibit a period-luminosity (PL) relation. We derived the gri-band PL and extinction-free period-Wesenheit (PW) r…

astro-ph.SR2023★ 14 cited

A Study of Stellar Spins in 15 Open Clusters

Brian F. Healy, P. R. McCullough, Kevin C. Schlaufman +1

We analyze spectroscopic and photometric data to determine the projected inclinations of stars in 11 open clusters, placing constraints on the spin-axis distributions of six cluste…

astro-ph.SR2021★ 20 cited

Stellar Spins in the Pleiades, Praesepe, and M35 Open Clusters

Brian F. Healy, P. R. McCullough, Kevin C. Schlaufman

We analyze spectroscopic and photometric data to determine the projected inclinations of stars in three open clusters: the Pleiades, Praesepe, and M35. We determine the va…

astro-ph.SR2020

Stellar Spins in the Open Cluster NGC 2516

Brian F. Healy, P. R. McCullough

Measuring the distribution of stellar spin axis orientations in a coeval group of stars probes the physical processes underlying the stars' formation. In this paper, we use spectro…

astro-ph.SR2019

Magnetic Inflation and Stellar Mass III: Revised Parameters for the Component Stars of NSVS 07394765

Brian F. Healy, Eunkyu Han, Philip S. Muirhead +4

We perform a new analysis of the M dwarf-M dwarf eclipsing binary system NSVS 07394765 in order to investigate the reported hyper-inflated radius of one of the component stars. Our…