Published July 1, 2021 | Version v1
Journal article

The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades

  • 1. Cahill Center for Astronomy & Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States)
  • 2. Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305 (United States)
  • 3. Department of Astronomy, University of California Berkeley, Berkeley, CA 94720 (United States)
  • 4. Department of Physics & Astronomy, University of California Los Angeles, Los Angeles, CA 90095 (United States)
  • 5. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States)
  • 6. Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 (United States)
  • 7. Department of Physics, University of Notre Dame, Notre Dame, IN, 46556 (United States)
  • 8. Department of Physics and Astronomy, University of Kansas, Lawrence, KS (United States)
  • 9. Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521 (United States)
  • 10. Department of Astronomy, Yale University, New Haven, CT 06511 (United States)
  • 11. Center of Excellence in Information Systems, Tennessee State University, Nashville, TN 37209 (United States)
  • 12. Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States)

Description

We present a high-precision radial velocity (RV) survey of 719 FGKM stars, which host 164 known exoplanets and 14 newly discovered or revised exoplanets and substellar companions. This catalog updated the orbital parameters of known exoplanets and long-period candidates, some of which have decades-longer observational baselines than they did upon initial detection. The newly discovered exoplanets range from warm sub-Neptunes and super-Earths to cold gas giants. We present the catalog sample selection criteria, as well as over 100,000 RV measurements, which come from the Keck-HIRES, APF-Levy, and Lick-Hamilton spectrographs. We introduce the new RV search pipeline RVSearch (https://california-planet-search.github.io/rvsearch/) that we used to generate our planet catalog, and we make it available to the public as an open-source Python package. This paper is the first study in a planned series that will measure exoplanet occurrence rates and compare exoplanet populations, including studies of giant planet occurrence beyond the water ice line, and eccentricity distributions to explore giant planet formation pathways. We have made public all radial velocities and associated data that we use in this catalog.

Availability note (English)

Available from http://dx.doi.org/10.3847/1538-4365/abe23c

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal. Supplement Series
Journal Volume
255
Journal Issue
1
Journal Page Range
[67 p.]
ISSN
0067-0049
CODEN
APJSA2

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
53081760
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S97: MATHEMATICAL METHODS AND COMPUTING;
Descriptors DEI
COMPUTERIZED SIMULATION; DETECTION; MONITORING; NEPTUNE PLANET; PYTHON; RADIAL VELOCITY; STARS
Descriptors DEC
PLANETS; PROGRAMMING LANGUAGES; SIMULATION; VELOCITY