70 citations · 237 across the 8 of their papers we have counts for
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A New Analysis of the Exoplanet Hosting System HD 6434
Natalie R. Hinkel, Stephen R. Kane, Genady Pilyavsky +5
The current goal of exoplanetary science is not only focused on detecting but characterizing planetary systems in hopes of understanding how they formed, evolved, and relate to the…
Host Star Properties and Transit Exclusion for the HD 38529 Planetary System
Gregory W. Henry, Stephen R. Kane, Sharon X. Wang +13
The transit signature of exoplanets provides an avenue through which characterization of exoplanetary properties may be undertaken, such as studies of mean density, structure, and…
The HD 192263 system: planetary orbital period and stellar variability disentangled
Diana Dragomir, Stephen R. Kane, Gregory W. Henry +11
As part of the Transit Ephemeris Refinement and Monitoring Survey (TERMS), we present new radial velocities and photometry of the HD 192263 system. Our analysis of the already avai…
A Search for the Transit of HD 168443b: Improved Orbital Parameters and Photometry
Genady Pilyavsky, Suvrath Mahadevan, Stephen R. Kane +13
The discovery of transiting planets around bright stars holds the potential to greatly enhance our understanding of planetary atmospheres. In this work we present the search for tr…
TERMS Photometry of Known Transiting Exoplanets
Diana Dragomir, Stephen R. Kane, Genady Pilyavsky +10
The Transit Ephemeris Refinement and Monitoring Survey (TERMS) conducts radial velocity and photometric monitoring of known exoplanets in order to refine planetary orbits and predi…
Stellar Variability of the Exoplanet Hosting Star HD 63454
Stephen R. Kane, Diana Dragomir, David R. Ciardi +9
Of the hundreds of exoplanets discovered using the radial velocity technique, many are orbiting close to their host stars with periods less than 10 days. One of these, HD 63454, is…
Improved Orbital Parameters and Transit Monitoring for HD 156846b
Stephen R. Kane, Andrew W. Howard, Genady Pilyavsky +10
HD 156846b is a Jovian planet in a highly eccentric orbit (e = 0.85) with a period of 359.55 days. The pericenter passage at a distance of 0.16 AU is nearly aligned to our line of…