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Measured and predicted mode visibilities for red giant branch stars observed by Kepler

The tables contain the data and model predictions shown in Fig.2 and 3 in Stello et al. 2016 (Nature,529,364) and in Fig.4 and 5 in Stello et al. 2016 (PASA, http://arxiv.org/abs/1602.05193). The data contains asteroseismic measurements of 3611 red giant branch stars observed by NASA's Kepler mission, including nu_max, delta_nu, and mode visibility. The theoretical predictions contains mode visibilities for stars with magnetic mode suppression relative to that of normal stars as well as nu_max. The structure of the tables and the columns are as follows: Data table: 13 lines of comments describing the licence agreement and the content of each column, followed by the colums of data. Model prediction table: 14 lines of comments describing the licence agreement and the content of each column, followed by the colums of model predictions.

Data and Resources

Cite this as

Dennis Stello (2016). Dataset: Measured and predicted mode visibilities for red giant branch stars observed by Kepler. http://dx.doi.org/10.4225/50/56c672381132b

Retrieved: 08:25, 06 May 2024 (GMT)

Data Portal Metadata

Field Value
Author Dennis Stello
Version 1.0
Last Updated November 2, 2016, 11:51 (Australia/Sydney)
Publish Date February 19, 2016, 12:30 (Australia/Sydney)
Data DOI http://dx.doi.org/10.4225/50/56c672381132b
Paper DOI http://dx.doi.org/10.1017/pasa.2016.9