Published July 2013 | Version Submitted + Published
Journal Article Open

100-year DASCH Light Curves of Kepler Planet-Candidate Host Stars

Abstract

We present 100 year light curves of Kepler planet-candidate host stars from the Digital Access to a Sky Century at Harvard (DASCH) project. 261 out of 997 host stars have at least 10 good measurements on DASCH scans of the Harvard plates. 109 of them have at least 100 good measurements, including 70% (73 out of 104) of all host stars with g ≤ 13 mag, and 44% (100 out of 228) of all host stars with g ≤ 14 mag. Our typical photometric uncertainty is ∼0.1–0.15 mag. No variation is found at 3σ level for these host stars, including 21 confirmed or candidate hot Jupiter systems which might be expected to show enhanced flares from magnetic interactions between dwarf primaries and their close and relatively massive planet companions.

Additional Information

© 2013 The Astronomical Society of the Pacific. Received 2013 April 28; accepted 2013 June 03; published 2013 June 14. We thank the anonymous referee for suggestions that have helped improve this article. We thank Alison Doane, Jaime Pepper, David Sliski and Robert J. Simcoe at CfA for their work on DASCH, and many volunteers who have helped digitize logbooks, clean and scan plates (http://hea‑www.harvard.edu/ DASCH/team.php). This work was supported in part by NSF grants AST0407380 and AST0909073 and now also the Cornel and Cynthia K. Sarosdy Fund for DASCH.

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Published - 671759.pdf

Submitted - 1304.7503v2.pdf

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Additional details

Identifiers

Eprint ID
41070
Resolver ID
CaltechAUTHORS:20130903-154245854

Funding

NSF
AST0407380
NSF
AST0909073
Cornel and Cynthia K. Sarosdy Fund

Dates

Created
2013-09-18
Created from EPrint's datestamp field
Updated
2021-11-10
Created from EPrint's last_modified field