This article is a correction to:
The NASA High-Resolution Speckle Interferometric Imaging Program: Validation and Characterization of Exoplanets and Their Stellar Hosts
Steve B. Howell1*
Nicholas J. Scott1
Rachel A. Matson2
Mark E. Everett3Elise Furlan4Crystal L. Gnilka1David R. Ciardi4Kathryn V. Lester1- 1NASA Ames Research Center, Moffett Field, CA, United States
- 2U.S. Naval Observatory, Washington, DC, United States
- 3NSFs National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ, United States
- 4NASA Exoplanet Science Institute, Pasadena, CA, United States
A Corrigendum on
by Steve B. Howell, Nicholas J. Scott, Rachel A. Matson, Mark E. Everett, Elise Furlan, Crystal L. Gnilka, David R. Ciardi, Kathryn V. Lester. (2021). Front. Astron. Space Sci. 10:635864. doi: 10.3389/fspas.2021.635864
Text Correction
In the original article, there were incorrect parameters listed in the last paragraph of Section 2.
A correction has been made to that paragraph as follows:
“As an aside, Robo-AO is another high-resolution imaging technique used in the optical wavelength range. Ziegler et al. (2017) discuss their results using this method for exoplanet host stars. Unlike speckle imaging, Robo-AO uses the mechanical deformable mirror techniques of IR/AO and applies them to optical light. See Ziegler et al. (2018) for details.
Ref is: @ARTICLE2018AJ....156...83Z, author = Ziegler, Carl and Law, Nicholas M. and Baranec, Christoph and Howard, Ward and Morton, Tim and Riddle, Reed and Duev, Dmitry A. and Salama, Ma¨ıssa and Jensen-Clem, Rebecca and Kulkarni, S. R., title = ”Robo-AO Kepler Survey. V. The Effect of Physically Associated Stellar Companions on Planetary Systems”, journal =, keywords = binaries: close, instrumentation: adaptive optics, methods: data analysis, methods: observational, planets and satellites: fundamental parameters, techniques: high angular resolution, Astrophysics - Earth and Planetary Astrophysics, year = 2018, month = aug, volume = 156, number = 2, eid = 83, pages = 83, doi = 10.3847/1538-3881/aace59, archivePrefix = arXiv, eprint = 1804.10208, primaryClass = astro-ph.EP, adsurl = https://ui.adsabs.harvard.edu/abs/2018AJ....156...83Z, adsnote = Provided by the SAO/NASA Astrophysics Data System.”
The authors apologize for this error and state that this does not change the scientific conclusions of the article in any way. The original article has been updated.
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Reference
Keywords: exoplanets, exoplanetary systems, binary host stars, speckle interferometry, high-resolution imaging
Citation: Howell SB, Scott NJ, Matson RA, Everett ME, Furlan E, Gnilka CL, Ciardi DR and Lester KV (2021) Corrigendum: The NASA High-Resolution Speckle Interferometric Imaging Program: Validation and Characterization of Exoplanets and Their Stellar Hosts. Front. Astron. Space Sci. 8:696011. doi: 10.3389/fspas.2021.696011
Received: 30 April 2021; Accepted: 07 May 2021;
Published: 30 September 2021.
Edited and reviewed by:
Susan Elizabeth Mullally, Space Telescope Science Institute (NASA), United StatesCopyright © 2021 Howell, Scott, Matson, Everett, Furlan, Gnilka, Ciardi and Lester. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Steve B. Howell, steve.b.howell@nasa.gov