CaltechAUTHORS
  A Caltech Library Service

Disentangling Blended K2 Photometry: Determining the Planetary Host Star

Payne, Alan N. and Ciardi, David R. and Kane, Stephen R. and Carter, Brad (2018) Disentangling Blended K2 Photometry: Determining the Planetary Host Star. Astronomical Journal, 156 (5). Art. No. 209. ISSN 1538-3881. https://resolver.caltech.edu/CaltechAUTHORS:20181023-083527516

[img] PDF - Published Version
See Usage Policy.

3540Kb
[img] PDF - Accepted Version
See Usage Policy.

3118Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20181023-083527516

Abstract

The presence of companion stars, whether bound or unbound, make correct identification of the planetary hosting star difficult when a planet has been detected through a photometrically blended transiting event. We present an approach that uses a combination of light curve analysis and stellar modeling to disentangle eight K2 photometrically blended binary systems that have either a confirmed or suspected planet to identify the probable host star. The key to our approach is the use of the mean stellar density, calculated using the transit geometry, as a discriminator. The approach is strongly dependent on the difference in magnitude between the stars and the observed transit depth, which is corrected by the flux ratio between the two stars. While our approach does not lead to a definitive result for all systems, we were able to determine the following for the eight systems in this case study: there are two systems where the primary was highly likely to be the planet-hosting star (>90% likelihood); three systems where the primary was likely to be the hosting star (>55% likelihood); one system where the secondary was likely to be the planet-hosting star (>55% likelihood); and two systems where we were uncertain which star was the planet-hosting star (≈50% likelihood to be either the primary or the secondary). Two systems, denoted by their EPIC number, EPIC 201546283 and EPIC 201862715, had confirmed planets, K2-27b and K2-94b, respectively, with radii of 4.0 ± 0.1 and 16.4 ± 2.9 R⊕, respectively.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-3881/aae310DOIArticle
https://arxiv.org/abs/1809.05981arXivDiscussion Paper
ORCID:
AuthorORCID
Ciardi, David R.0000-0002-5741-3047
Kane, Stephen R.0000-0002-7084-0529
Additional Information:© 2018 The American Astronomical Society. Received 2018 August 1; revised 2018 September 11; accepted 2018 September 13; published 2018 October 18.
Group:Infrared Processing and Analysis Center (IPAC)
Subject Keywords:binaries: visual – planetary systems – planets and satellites: detection – planets and satellites: fundamental parameters – stars: fundamental parameters
Issue or Number:5
Record Number:CaltechAUTHORS:20181023-083527516
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20181023-083527516
Official Citation:Alan N. Payne et al 2018 AJ 156 209
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:90345
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:23 Oct 2018 21:53
Last Modified:03 Oct 2019 20:24

Repository Staff Only: item control page