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ERRATUM: "UNDERSTANDING THE EFFECTS OF STELLAR MULTIPLICITY ON THE DERIVED PLANET RADII FROM TRANSIT SURVEYS: IMPLICATIONS FOR KEPLER, K2, AND TESS" (2015, ApJ, 805, 16)

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Published 2017 January 4 • © 2017. The American Astronomical Society. All rights reserved.
, , Citation David R. Ciardi et al 2017 ApJ 834 96 DOI 10.3847/1538-4357/834/1/96

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This is a correction for 2015 ApJ 805 16

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ciardi@ipac.caltech.edu

Author affiliations

1 NASA Exoplanet Science Institute/Caltech Pasadena, CA USA; ciardi@ipac.caltech.edu

2 Department of Physics, Southern Connecticut State University, New Haven, CT, USA

3 NASA Ames Research Center, Mountain View, CA, USA

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  1. Received 2016 October 21
  2. Accepted 2016 November 21
  3. Published

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0004-637X/834/1/96

ABSTRACT

There was an error in the published version of Equation (6); the equation should read as

\begin{eqnarray}{X}_{R}\equiv \displaystyle \frac{{R}_{p}({true})}{{R}_{p}({observed})}=\left(\displaystyle \frac{{R}_{t\star }}{{R}_{1\star }}\right)\sqrt{\displaystyle \frac{{F}_{{total}}}{{F}_{t}}}.\end{eqnarray}

The calculations and results presented in the paper utilized the correct form of the equation and are unaffected by the error in the equation. The authors sincerely regret the error.

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