Determining the occurrence rate of giant planets orbiting low mass stars (M<0.6Msun) is a critical test of the core-accretion theory of planet formation. However the occurrence rate of these giant planets is poorly constrained from previous surveys. In this study we determine this occurrence rate using the hundreds of thousands of low-mass stars monitored in the TESS FFIs. We perform an automated transit search through light curves extracted from the TESS full frame images for low-mass dwarf stars selected using TICv8 parameters. Candidates are selected by a series of objective vetting steps that identify and reject false positive cases, particularly eclipsing binary systems and variable stars. Injection and recovery tests are used to t...
Artículo de publicación ISIDue to their higher planet–star mass ratios, M dwarfs are the easiest tar...
In this presentation, we describe the new Giant Exoplanets around M dwarf Stars (GEMS) survey initia...
peer reviewedPlanet formation theories predict a large but still undetected population of short-peri...
The Transiting Exoplanet Survey Satellite (TESS) is optimized to search nearby M dwarf stars for tra...
We analyze a volume-complete sample of 365 mid-to-late M dwarfs within 15 pc with masses between 0.1...
We analyze a volume-complete sample of 365 mid-to-late M dwarfs within 15 pc with masses between 0.1...
TESS' all-sky survey enables studies of the demographics of exoplanets around stars too rare to have...
In this work, we present the analysis of 976 814 FGKM dwarf and subgiant stars in the Transiting Exo...
Context. The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 near...
Context. With the discovery of a planetary system around the ultracool dwarf TRAPPIST-1, there has b...
The nearly all-sky TESS Full Frame Images have led to an explosion of new exoplanet discoveries. How...
Context. The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 near...
International audienceContext. Direct imaging has led to the discovery of several giant planet and b...
Searching for planets around stars with different masses probes the outcome of planetary formation f...
Ph.D. University of Hawaii at Manoa 2013.Includes bibliographical references.Low-mass stars between ...
Artículo de publicación ISIDue to their higher planet–star mass ratios, M dwarfs are the easiest tar...
In this presentation, we describe the new Giant Exoplanets around M dwarf Stars (GEMS) survey initia...
peer reviewedPlanet formation theories predict a large but still undetected population of short-peri...
The Transiting Exoplanet Survey Satellite (TESS) is optimized to search nearby M dwarf stars for tra...
We analyze a volume-complete sample of 365 mid-to-late M dwarfs within 15 pc with masses between 0.1...
We analyze a volume-complete sample of 365 mid-to-late M dwarfs within 15 pc with masses between 0.1...
TESS' all-sky survey enables studies of the demographics of exoplanets around stars too rare to have...
In this work, we present the analysis of 976 814 FGKM dwarf and subgiant stars in the Transiting Exo...
Context. The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 near...
Context. With the discovery of a planetary system around the ultracool dwarf TRAPPIST-1, there has b...
The nearly all-sky TESS Full Frame Images have led to an explosion of new exoplanet discoveries. How...
Context. The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 near...
International audienceContext. Direct imaging has led to the discovery of several giant planet and b...
Searching for planets around stars with different masses probes the outcome of planetary formation f...
Ph.D. University of Hawaii at Manoa 2013.Includes bibliographical references.Low-mass stars between ...
Artículo de publicación ISIDue to their higher planet–star mass ratios, M dwarfs are the easiest tar...
In this presentation, we describe the new Giant Exoplanets around M dwarf Stars (GEMS) survey initia...
peer reviewedPlanet formation theories predict a large but still undetected population of short-peri...