Search Results - "Bowler, Brendan P."
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Dynamical Mass of the Young Brown Dwarf Companion PZ Tel B
Published in The Astronomical journal (01-06-2023)“…Abstract Dynamical masses of giant planets and brown dwarfs are critical tools for empirically validating substellar evolutionary models and their underlying…”
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Gaussian Process Models Impact the Inferred Properties of Giant Planets around Active Stars
Published in The Astronomical journal (01-10-2024)“…Abstract The recent development of statistical methods that can distinguish between stellar activity and dynamical signals in radial velocity (RV) observations…”
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Know thy star, know thy planet: chemo-kinematically characterizing TESS targets
Published in Monthly notices of the Royal Astronomical Society (01-01-2020)“…ABSTRACT The Transiting Exoplanet Survey Satellite (TESS) has already begun to discover what will ultimately be thousands of exoplanets around nearby cool…”
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ZODIACAL EXOPLANETS IN TIME (ZEIT). I. A NEPTUNE-SIZED PLANET ORBITING AN M4.5 DWARF IN THE HYADES STAR CLUSTER
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT Studying the properties of young planetary systems can shed light on how the dynamics and structure of planets evolve during their most formative…”
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Dynamical Mass of the Young Substellar Companion HD 984 B
Published in The Astronomical journal (01-02-2022)“…Abstract Model-independent masses of substellar companions are critical tools to validate models of planet and brown dwarf cooling, test their input physics,…”
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Direct Exoplanet Detection using Convolutional Image Reconstruction (ConStruct): A New Algorithm for Post-processing High-contrast Images
Published in The Astronomical journal (01-03-2024)“…Abstract We present a novel machine-learning approach for detecting faint point sources in high-contrast adaptive optics (AO) imaging data sets. The most…”
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Intercomparison of Brown Dwarf Model Grids and Atmospheric Retrieval Using Machine Learning
Published in The Astrophysical journal (01-09-2023)“…Abstract Understanding differences between substellar spectral data and models has proven to be a major challenge, especially for self-consistent model grids…”
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Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars
Published in The Astronomical journal (01-02-2024)“…Abstract Transiting giant planets provide a natural opportunity to examine stellar obliquities, which offer clues about the origin and dynamical histories of…”
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SPECTROSCOPIC CONFIRMATION OF YOUNG PLANETARY-MASS COMPANIONS ON WIDE ORBITS
Published in The Astrophysical journal (20-03-2014)“…We present moderate-resolution (R ~ 4000-5000) near-infrared integral field spectroscopy of the young (1-5 Myr) 6-14 M sub(jup) companions ROXs 42B b and FW…”
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THREE WIDE PLANETARY-MASS COMPANIONS TO FW TAU, ROXs 12, AND ROXs 42B
Published in The Astrophysical journal (20-01-2014)“…We report the discovery of three planetary-mass companions (M = 6-20 M sub(Jup)) in wide orbits ([rho] ~ 150-300 AU) around the young stars FW Tau…”
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Constraints on the spin evolution of young planetary-mass companions
Published in Nature astronomy (01-02-2018)“…Surveys of young star-forming regions have discovered a growing population of planetary-mass (<13 M Jup ) companions around young stars 1 . There is an ongoing…”
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Deep Paβ Imaging of the Candidate Accreting Protoplanet AB Aur b
Published in The Astronomical journal (01-04-2024)“…Abstract Giant planets grow by accreting gas through circumplanetary disks, but little is known about the timescale and mechanisms involved in the…”
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The Impact of Bayesian Hyperpriors on the Population-level Eccentricity Distribution of Imaged Planets
Published in The Astronomical journal (01-02-2023)“…Abstract Orbital eccentricities directly trace the formation mechanisms and dynamical histories of substellar companions. Here, we study the effect of…”
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PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
Published in The Astrophysical journal (01-09-2013)“…We report the discovery of an L-type companion to the young M3.5V star 2MASS J01225093-2439505 at a projected separation of 1".45 ([approx =]52 AU) as part of…”
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Near-infrared Spectroscopy of the Extrasolar Planet HR 8799 b
Published in The Astrophysical journal (01-11-2010)“…We present 2.12-2.23 Delta *mm high contrast integral field spectroscopy of the extrasolar planet HR 8799 b. Our observations were obtained with OSIRIS on the…”
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Rotation Periods, Inclinations, and Obliquities of Cool Stars Hosting Directly Imaged Substellar Companions: Spin–Orbit Misalignments Are Common
Published in The Astronomical journal (01-04-2023)“…Abstract The orientation between a star’s spin axis and a planet’s orbital plane provides valuable information about the system’s formation and dynamical…”
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Atmospheric Retrievals of the Young Giant Planet ROXs 42B b from Low- and High-resolution Spectroscopy
Published in The Astronomical journal (01-05-2024)“…Abstract Previous attempts have been made to characterize the atmospheres of directly imaged planets at low resolution ( R ∼ 10–100 s), but the presence of…”
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ELemental abundances of Planets and brown dwarfs Imaged around Stars (ELPIS). I. Potential Metal Enrichment of the Exoplanet AF Lep b and a Novel Retrieval Approach for Cloudy Self-luminous Atmospheres
Published in The Astronomical journal (01-11-2023)“…Abstract AF Lep A+b is a remarkable planetary system hosting a gas-giant planet that has the lowest dynamical mass among directly imaged exoplanets. We present…”
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Efficiently Searching for Close-in Companions Around Young M Dwarfs Using a Multiyear PSF Library
Published in The Astronomical journal (01-11-2024)“…Abstract We present Super-RDI, a unique framework for the application of reference star differential imaging (RDI) to Keck/NIRC2 high-contrast imaging…”
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SEARCHING FOR SCATTERERS: HIGH-CONTRAST IMAGING OF YOUNG STARS HOSTING WIDE-SEPARATION PLANETARY-MASS COMPANIONS
Published in The Astrophysical journal (20-08-2016)“…ABSTRACT We have conducted an angular differential imaging survey with NIRC2 at Keck in search of close-in substellar companions to a sample of seven systems…”
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