950 datasets found

Keywords: exoplanets

Filter Results
  • List of 213 planetary systems architectures

    We present a stability analysis of a large set of simulated planetary systems of three or more planets based on architectures of multiplanet systems discovered by Kepler and K2....
  • Transit time for planets in LHS 1678 System

    The nearby LHS-1678 (TOI-696) system contains two confirmed planets and a wide-orbit, likely brown-dwarf companion, which orbit an M2 dwarf with a unique evolutionary history....
  • Best-in-class TOIs for atmospheric characterisation

    JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5000 confirmed planets, more than 4000 Transiting Exoplanet...
  • <200Myr planet's hosts TESS parameters

    Within the first few hundreds of millions of years, many physical processes sculpt the eventual properties of young planets. NASA's Transiting Exoplanet Survey Satellite (TESS)...
  • DTARPS. II. 462 new TESS candidates

    The DIAmante TESS AutoRegressive Planet Search for the southern ecliptic hemisphere (DTARPS-S) project seeks to identify photometric transiting planets from 976814 southern...
  • Breakthrough listen search for intelligent life

    Never before has the detection and characterization of exoplanets via transit photometry been as promising and feasible as it is now, due to the increasing breadth and...
  • WIRC light curves of TOI-1420b

    Superpuffs are planets with exceptionally low densities ({rho}<~0.1g/cm^3^) and core masses (Mc<~5M{Earth}). Many lower-mass (Mp<~10M{Earth}) superpuffs are expected to...
  • The solar neighborhood LI. RECONS & TESS obs.

    We present the optical photometric variability of 32 planet-hosting M dwarfs within 25pc over timescales of months to decades. The primary goal of this project-A Trail to Life...
  • Radial velocity and photometry of TOI-677

    TOI-677b is part of an emerging class of "tidally detached" gas giants (a/R*>~11) that exhibit large orbital eccentricities and yet low stellar obliquities. Such sources pose...
  • OGLE-2014-BLG-0221Lb VRI light curve

    We present the analysis of the microlensing event OGLE-2014-BLG-0221, a planetary candidate event discovered in 2014. The photometric light curve is best described by a...
  • TESS-Keck Survey. XII. TOI-1347 radial velocity

    The extreme environments of ultra-short-period planets (USPs) make excellent laboratories to study how exoplanets obtain, lose, retain, and/or regain gaseous atmospheres. We...
  • TOI-1994 radial velocities with MINERVA & CHIRON

    We present the discovery of TOI-1994b, a low-mass brown dwarf transiting a hot subgiant star on a moderately eccentric orbit. TOI-1994 has an effective temperature of...
  • System properties & impact parameter variations

    We fit a dynamical model to Kepler systems that contain four or more transiting planets using the analytic method AnalyticLC and obtain physical and orbital parameters for 101...
  • Transit depth variability with TESS

    The phenomenon of transit depth variability offers a pathway through which processes such as exoplanet atmospheric activity and orbital dynamics can be studied. In this work we...
  • New mean motion resonances with exoMMR package

    The study of orbital resonances allows for the constraint of planetary properties of compact systems. We can predict a system's resonances by observing the orbital periods of...
  • Light curves and radial velocities for TOI-1899

    TOI-1899b is a rare exoplanet, a temperate warm Jupiter orbiting an M-dwarf, first discovered by Canas et al. (2020) from a TESS single-transit event. Using new radial...
  • Known exoplanet hosts parameters with TESS

    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...
  • New HIRES radial velocity data for V1298 Tau

    Mass, radius, and age measurements of young (<~100Myr) planets have the power to shape our understanding of planet formation. However, young stars tend to be extremely...
  • BD+29 2654 equivalent Widths and line abundances

    We report the discovery and Doppler mass measurement of a 7.4days 2.3R{Earth} mini-Neptune around a metal-poor K-dwarf BD+29-2654 (TOI-2018). Based on a high-resolution...
  • EXPRES. IV. Two Additional Planets Orbiting

    Thousands of exoplanet detections have been made over the last 25 years using Doppler observations, transit photometry, direct imaging, and astrometry. Each of these methods is...
You can also access this registry using the API (see API Docs).