Sloane J. Wiktorowicz, Ph.D.

Affiliations: 
2009 Planetary Science California Institute of Technology, Pasadena, CA 
Area:
Astronomy
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"Sloane Wiktorowicz"
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Parents

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Shrinivas R. Kulkarni grad student 2009 Caltech
 (Unambiguous Black Hole Mass from Polarimetry and Application to Hot Jupiters.)
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Publications

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Bruzzone JS, Metchev S, Duchêne G, et al. (2020) Imaging the 44 au Kuiper Belt Analog Debris Ring around HD 141569A with GPI Polarimetry The Astronomical Journal. 159: 53
Greenbaum AZ, Cheetham A, Sivaramakrishnan A, et al. (2019) Performance of the Gemini Planet Imager Non-redundant Mask and Spectroscopy of Two Close-separation Binaries: HR 2690 and HD 142527 The Astronomical Journal. 157: 249
Rajan A, Rameau J, Rosa RJD, et al. (2017) Characterizing 51 Eri b from 1 to 5μm: A Partly Cloudy Exoplanet The Astronomical Journal. 154: 10
Follette KB, Rameau J, Dong R, et al. (2017) Complex Spiral Structure in the HD 100546 Transitional Disk as Revealed by GPI and MagAO The Astronomical Journal. 153: 264
Rameau J, Follette KB, Pueyo L, et al. (2017) An Optical/Near-infrared Investigation of HD 100546 b with the Gemini Planet Imager and MagAO The Astronomical Journal. 153: 244
Johnson-Groh M, Marois C, De Rosa RJ, et al. (2017) Integral Field Spectroscopy of the Low-mass Companion HD 984 B with the Gemini Planet Imager The Astronomical Journal. 153: 190
Chilcote J, Pueyo L, Rosa RJD, et al. (2017) 1–2.4μm Near-IR Spectrum of the Giant PlanetβPictoris b Obtained with the Gemini Planet Imager The Astronomical Journal. 153: 182
Konopacky QM, Rameau J, Duchêne G, et al. (2016) DISCOVERY of A SUBSTELLAR COMPANION to the NEARBY DEBRIS DISK HOST HR 2562 Astrophysical Journal Letters. 829
Nielsen EL, Rosa RJD, Wang J, et al. (2016) DYNAMICAL MASS MEASUREMENT OF THE YOUNG SPECTROSCOPIC BINARY V343 NORMAE AaAb RESOLVED WITH THE GEMINI PLANET IMAGER The Astronomical Journal. 152: 175
Millar-Blanchaer MA, Wang JJ, Kalas P, et al. (2016) IMAGING AN 80 au RADIUS DUST RING AROUND THE F5V STAR HD 157587 The Astronomical Journal. 152: 128
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