SPECKLE CAMERA OBSERVATIONS FOR THE NASA KEPLER MISSION FOLLOW-UP PROGRAM

By S. Howell, Mark E. Everett, W. Sherry, Elliott Horch, D. Ciardi. 2011

290 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Electrical and Electronic Engineering

View Paper: https://www.semanticscholar.org/paper/6fdd44b11f91e072f9279a323601b598febb689a

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In Astronomy and Astrophysics

1. D. Charbonneau
2. Jon Fortney
3. Timothy Morton
4. J. Winn
5. J. Johnson
6. G. Marcy
7. Andrew W. Howard
8. Sara Seager

In Atomic and Molecular Physics, and Optics

1. Jon Fortney
2. Sara Seager
3. J. Winn
4. D. Charbonneau
5. J. D'esert
6. D. Deming
7. R. Gilliland
8. H. Knutson

In Electrical and Electronic Engineering

1. Timothy Morton
2. J. Winn
3. T. Brown
4. D. Charbonneau
5. Jie Li
6. Mark E. Everett
7. T. Dupuy
8. D. Latham

Citations in the corpus

• ECCENTRICITY FROM TRANSIT PHOTOMETRY: SMALL PLANETS IN KEPLER MULTI-PLANET SYSTEMS HAVE LOW ECCENTRICITIES (2015, background): “However, most of the targets from our selected sample of bright stars have been followed up with adaptive optics (Adams et al. 2012) and Speckle images (Howell et al. 2011).”
• Kepler-22b: A 2.4 EARTH-RADIUS PLANET IN THE HABITABLE ZONE OF A SUN-LIKE STAR (2011, methodology): “Based on the Kp–Ks versus J–Ks color–color relationships from Howell et al. (2011b), we derive Kp = 18.85 ± 0.1 mag, Kp = 19.9 ± 0.1 mag, and Kp = 21.8 ± 0.6 mag for 7, 8, and 10 mag fainter than the primary target in the Kepler bandpass.”
• THE IMPACT OF STELLAR MULTIPLICITY ON PLANETARY SYSTEMS. I. THE RUINOUS INFLUENCE OF CLOSE BINARY COMPANIONS (2016, background): “The optical speckle imaging programs of Howell et al. (2011), Horch et al. (2012), Everett et al. (2015) reported 9 candidate companions in common with our program.”
• Planet Hunters IX. KIC 8462852-where's the flux? (2015, methodology): “We also obtained Speckle observations of KIC 8462852 on the night of UT 2015 Oct 22 using the DSSI instrument on the WIYN telescope located on Kitt Peak (Howell et al. 2011).”
• ALMOST ALL OF KEPLER'S MULTIPLE-PLANET CANDIDATES ARE PLANETS (2012, methodology): “Details of this speckle imaging data collection and reduction precesses are fully described in Howell et al. (2011).”
• The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets (2017, background): “…a collection of highresolution imaging facilities (Lillo-Box et al. 2012, 2014; Horch et al. 2012, 2014; Everett et al. 2015; Gilliland et al. 2015; Cartier et al. 2015; Wang et al. 2015a,b; Adams et al. 2012, 2013; Dressing et al. 2014; Law et al. 2014; Baranec et al. 2016; Howell et al. 2011).”
• KEPLER-18b, c, AND d: A SYSTEM OF THREE PLANETS CONFIRMED BY TRANSIT TIMING VARIATIONS, LIGHT CURVE VALIDATION, WARM-SPITZER PHOTOMETRY, AND RADIAL VELOCITY MEASUREMENTS (2011, methodology): “We perform speckle observations at the WIYN 3.5-m telescope, using the Differential Speckle Survey Instrument (DSSI) (Horch et al. 2011; Howell et al. 2011).”
• The California-Kepler Survey. IV. Metal-rich Stars Host a Greater Diversity of Planets (2017, unknown): “…Sample 2 Alphabetical by author: Adams et al. (2012, 2013); Baranec et al. (2016); Cartier et al. (2015); Dressing et al. (2014); Everett et al. (2015); Gilliland et al. (2015); Horch et al. (2012, 2014); Howell et al. (2011); Law et al. (2014); Lillo-Box et al. (2012, 2014); Wang et al. (2015a,b).”
• THE KEPLER FOLLOW-UP OBSERVATION PROGRAM. I. A CATALOG OF COMPANIONS TO KEPLER STARS FROM HIGH-RESOLUTION IMAGING (2016, methodology): “Some of the results in this work are based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, operated by AURA, Inc., under NASA contract NAS 5-26555.”
• THE MASS OF KOI-94d AND A RELATION FOR PLANET RADIUS, MASS, AND INCIDENT FLUX (2013, methodology): “The details of the two-color speckle camera observations and the Kepler follow-up observing program are presented in Howell et al. (2011).”
• VALIDATION OF KEPLER'S MULTIPLE PLANET CANDIDATES. II. REFINED STATISTICAL FRAMEWORK AND DESCRIPTIONS OF SYSTEMS OF SPECIAL INTEREST (2014, background): “Speckle images of KOI-284 obtained on 2010 June 24 revealed two stars differing in brightness by less than one magnitude and separated from one another by slightly less than 1′′ (Howell et al. 2011).”