Planets Orbiting Other Suns

By G. Marcy, R. P. Butler. 2000

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View Paper: https://www.semanticscholar.org/paper/82b9eda5b6728b802397a682172fb05d563923a6

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In Astronomy and Astrophysics

Citations in the corpus

THE PALOMAR/KECK ADAPTIVE OPTICS SURVEY OF YOUNG SOLAR ANALOGS: EVIDENCE FOR A UNIVERSAL COMPANION MASS FUNCTION (2008, methodology): “%) in 0–3 AU orbits from G and K stars: a phenomenon termed “the brown dwarf desert” (Marcy & Butler 2000).”
Search for brown-dwarf companions of stars (2010, background): “With a frequency of less than 1 % (Marcy & Butler 2000), brown-dwarf companions to solar-type stars at separations below 10 AU are much less common than planetary companions with a frequency of ∼7 % (e.g. Udry & Santos 2007) and stellar binaries with a frequency of ∼13 % (Duquennoy & Mayor 1991;…”
Imaging Polarimetric Observations of a New Circumstellar Disk System (2001, background): “With more than 50 planetary systems detected (Marcy and Butler, 2000) it is the observational clues to the premainsequence systems which are particularly scarce – only a few resolved observations of circumstellar disk systems exist.”
Dynamical Instabilities in Extrasolar Planetary Systems Containing Two Giant Planets (2000, background): “Indeed, the observed frequency of 51 Peg type systems appears much higher than would be predicted by such a dynamical scenario: in the observed sample the frequency is ∼ 20%, while among all stars searched for planetary-mass companions it is ∼ 1% (Marcy and Butler 2000).”
Extrasolar planet population synthesis - II. Statistical comparison with observations (2009, background): “For example, Marcy & Butler (2000) have estimated a frequency of brown dwarfs within 3 AU of .”
Two New Planets from the Anglo-Australian Planet Search (2001, background): “…the last 5 yr have come from precision Doppler surveys of nearby dwarf stars ranging in spectral type from late F through M4 (Mayor & Queloz 1995 ; Marcy & Butler 1998, 2000 ; Noyes et al. 1997 ; Cochran et al. 1997 ; Vogt et al. 2000 ; Kurster et al. 2000 ; Udry et al. 2000 ; Fischer et al.…”
Simulation of a Space-based Microlensing Survey for Terrestrial Extrasolar Planets (2000, methodology): “The success of the precision radial velocity technique has been spectacular (Marcy, Cochran & Mayor 2000; Perryman 2000; Marcy & Butler 2000) with the discovery of more than 70 extra-solar giant planets in the past seven years.”
Toward Spectral Classification of L and T Dwarfs: Infrared and Optical Spectroscopy and Analysis (2001, background): “…of Physics, University of Michigan, 500 East University, Ann Arbor, MI 48109. indirectly as companions to nearby stars (Becklin & Zuckerman 1988 ; Nakajima et al. 1995 ; Oppenheimer et al. 1995 ; Mayor & Queloz 1995 ; Marcy & Butler 1998, 2000 ; Butler et al. 2000 ; Marcy, Cochran, & Mayor 2000).”
MAPPING THE SHORES OF THE BROWN DWARF DESERT. II. MULTIPLE STAR FORMATION IN TAURUS–AURIGA (2011, background): “Over the past fifteen years, radial velocity surveys have discovered many short-period stellar companions and exoplanets, but relatively few companions with masses of ∼10–80MJup (e.g., Marcy & Butler 2000; Grether & Lineweaver 2006), a gap known as the “brown dwarf desert”.”
Five New Extrasolar Planets (2005, background): “The planet mass function is consistent with a power law, dN=dM / M 1:3, with increasing numbers of planets at lower masses (Marcy & Butler 2000), even after correction for detection efficiency (Jorissen et al. 2001).”
The Geometry of Resonant Signatures in Debris Disks with Planets (2002, background): “However, most of the known extrasolar planets do not resemble the Earth or Neptune; they have masses in the range of 0.3–15 Jupiter masses, and they often have significant orbital eccentricities (see, e.g., the review by Marcy & Butler 2000).”
Hubble Space Telescope NICMOS Observations of T Dwarfs: Brown Dwarf Multiplicity and New Probes of the L/T Transition (2006, background): “…Liu et al. (2006); and this study. aration brown dwarf binary desert originally suggested by Mart́ın et al. (2000) — not to be confused with the brown dwarf companion desert around solar-type stars (Marcy & Butler 2000) — remains a distinct characteristic of brown dwarf binaries in the field.”
Hubble Space Telescope Observations of Binary Very Low Mass Stars and Brown Dwarfs (2003, background): “Although brown dwarfs are extremely rare as close companions to GFK stars (Halbwachs et al. 2000; Marcy & Butler 2000), a number of studies have detected double brown dwarf systems (Martı́n, Brandner, & 1 Visiting Astronomer, Kitt Peak National Observatory, National Optical Astronomy Observatory,…”
DISCOVERY AND VALIDATION OF Kepler-452b: A 1.6 R⨁ SUPER EARTH EXOPLANET IN THE HABITABLE ZONE OF A G2 STAR (2015, background): “…more so than the BEB, BP, or HTP/HTS scenarios) because of the known paucity of brown dwarfs as spectroscopic companions to main-sequence stars within hundreds of AU, and especially G-type stars (see, e.g., Marcy & Butler 2000), whereas binaries with main-sequence companions are far more common.”
Limits on Planetary Companions from Doppler Surveys of Nearby Stars (2016, background): “…& Butler 1996), the first multi-planet system (Butler et al. 1999), the first subSaturn-mass planets (Marcy et al. 2000), the discovery of 70 of the first 100 extrasolar planets (Marcy & Butler 2000), and the first planet search completeness limits for a large sample of stars (Cumming et al. 1999).”
Mapping the Shores of the Brown Dwarf Desert. I. Upper Scorpius (2007, background): “However, they have revealed a surprising lack of brown dwarf mass companions in close orbits, with estimates suggesting frequencies of < 1% (Marcy & Butler 2000; Grether & Lineweaver 2006).”