activity
20162024
most citedChanging the Scaling Relation: The Need For a Mean Molecular Weight Term

82 citations · 276 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2024★ 12 cited

The K2 Asteroseismic KEYSTONE sample of Dwarf and Subgiant Solar-Like Oscillators. I: Data and Asteroseismic parameters

Mikkel N. Lund, Sarbani Basu, Allyson Bieryla +19

The KEYSTONE project aims to enhance our understanding of solar-like oscillators by delivering a catalogue of global asteroseismic parameters ( and ) for 173 s…

astro-ph.SR2021★ 14 cited

Mixed Modes and Asteroseismic Surface Effects: II. Subgiant Systematics

J. M. Joel Ong, Sarbani Basu, Mikkel N. Lund +3

Models of solar-like oscillators yield acoustic modes at different frequencies than would be seen in actual stars possessing identical interior structure, due to modelling error ne…

astro-ph.SR2020★ 23 cited

Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology

Lucas S. Viani, Sarbani Basu

Core overshoot is a large source of uncertainty in constructing stellar models. Whether the amount of overshoot is constant or mass dependent is not completely known, even though m…

astro-ph.SR2020★ 21 cited

Solar cycle variation of in helioseismic data and its implications for asteroseismology

Rachel Howe, William J. Chaplin, Sarbani Basu +7

The frequency, , at which the envelope of pulsation power peaks for solar-like oscillators is an important quantity in asteroseismology. We measure for t…

astro-ph.SR2019★ 24 cited

Determining the Best Method of Calculating the Large Frequency Separation For Stellar Models

Lucas S. Viani, Sarbani Basu, Enrico Corsaro +2

Asteroseismology of solar-like oscillators often relies on the comparisons between stellar models and stellar observations in order to determine the properties of stars. The values…

astro-ph.SR2018★ 71 cited

Investigating the Metallicity-Mixing Length Relation

Lucas S. Viani, Sarbani Basu, Joel J. M. Ong +2

Stellar models typically use the mixing length approximation as a way to implement convection in a simplified manner. While conventionally the value of the mixing length parameter,…