English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

One of the most well-studied young stellar associations, Taurus-Auriga, willbe observed by the extended Kepler mission, K2, in the spring of 2017. K2Campaign 13 (C13) will be a unique opportunity to study many stars in thisyoung association at high photometric precision and cadence. Using observationsfrom the Kilodegree Extremely Little Telescope (KELT) survey, we identify"dippers", stochastic variables, and periodic variables among K2 C13 targetstars. This release of the KELT data (lightcurve data in e-tables) provides thecommunity with long-time baseline observations to assist in the understandingof the more exotic variables in the association. Transient-like phenomena ontimescales of months to years are known characteristics in the light curves ofyoung stellar objects, making contextual pre- and post-K2 observations criticalto understanding their underlying processes. We are providing a comprehensiveset of the KELT light curves for known Taurus-Auriga stars in K2 C13. Thecombined data sets from K2 and KELT should permit a broad array ofinvestigations related to star formation, stellar variability, andprotoplanetary environments.

Identification of Young Stellar Variables with KELT for K2 I: Campaign 13 Taurus Dippers and Rotators