5k citations
- Space Telescope Science InstituteUS164 papers
- Centre National de la Recherche ScientifiqueFR152 papers
- University of ArizonaUS148 papers
- California Institute of TechnologyUS129 papers
- Center for Astrophysics Harvard & SmithsonianUS124 papers
- Université Bourgogne Franche-ComtéFR111 papers
- Max Planck Institute for AstronomyDE99 papers
- Johns Hopkins UniversityUS95 papers
- NSF NOIRLabUS94 papers
- Princeton UniversityUS87 papers
- National Astronomical Observatory of JapanJP85 papers
- University of California, BerkeleyUS85 papers
6 papers · 2 filters
The TESS-Keck Survey. XV. Precise Properties of 108 TESS Planets and Their Host Stars
Mason G. MacDougall, Erik A. Petigura, Gregory J. Gilbert +38
We present the stellar and planetary properties for 85 TESS Objects of Interest (TOIs) hosting 108 planet candidates which comprise the TESS-Keck Survey (TKS) sample. We combine ph…
Variability of Known Exoplanet Host Stars Observed by TESS
Emilie R. Simpson, Tara Fetherolf, Stephen R. Kane +3
Both direct and indirect methods of exoplanet detection rely upon detailed knowledge of the potential host stars. Such stellar characterization allows for accurate extraction of pl…
The two rings of (50000) Quaoar
C. L. Pereira, B. Sicardy, B. E. Morgado +66
Quaoar is a classical Trans-Neptunian Object (TNO) with an area equivalent diameter of 1,100 km and an orbital semi-major axis of 43.3 astronomical units. Based on stellar occultat…
The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory
Lauren M. Weiss, Howard Isaacson, Andrew W. Howard +17
Despite the importance of Jupiter and Saturn to Earth's formation and habitability, there has not yet been a comprehensive observational study of how giant exoplanets correlate wit…
TTV Constraints on Additional Planets in the WD 1856+534 system
Sarah Kubiak, Andrew Vanderburg, Juliette Becker +4
WD 1856+534 b (or WD 1856 b for short) is the first known transiting planet candidate around a white dwarf star. WD 1856 b is about the size of Jupiter, has a mass less than about…
Keck, Gemini, and Palomar 200-inch visible photometry of red and very-red Neptunian Trojans
B. T. Bolin, C. Fremling, A. Morbidelli +9
Neptunian Trojans (NTs), trans-Neptunian objects in 1:1 mean-motion resonance with Neptune, are generally thought to have been captured from the original trans-Neptunian protoplane…