Featured Dataverses

In order to use this feature you must have at least one published dataverse.

Publish Dataverse

Are you sure you want to publish your dataverse? Once you do so it must remain published.

Publish Dataverse

This dataverse cannot be published because the dataverse it is in has not been published.

Delete Dataverse

Are you sure you want to delete your dataverse? You cannot undelete this dataverse.

Advanced Search

1 to 9 of 9 Results
Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS MissionEmbargoed
May 30, 2024
Catherine Clark, 2024, "Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission", https://doi.org/10.48577/jpl.HFBNWC, Astronomical Journal, JPL Open Repository
Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery, the mysteries surrounding their origins remain. Here, we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-41...
The Discovery of Four Eccentric Sub-Neptunes Close to M dwarfs from TESSEmbargoed
May 1, 2024
Catherine Clark, 2024, "The Discovery of Four Eccentric Sub-Neptunes Close to M dwarfs from TESS", https://doi.org/10.48577/jpl.FCEX98, Astronomical Journal, JPL Open Repository
Sub-Neptunes with 2 − 3R⊕, which are commonly discovered around M dwarfs, are intermediate planets that bridge a gap between abundant rocky planets and rare Neptune- and Jupiter-sized ones. The orbital properties and bulk compositions of transiting sub-Neptunes give an inkling of...
The TESS-Keck Survey XX: Mass Catalog and Data ReleaseEmbargoed
Apr 29, 2024
Catherine Clark, 2024, "The TESS-Keck Survey XX: Mass Catalog and Data Release", https://doi.org/10.48577/jpl.PBE9NW, Astronomical Journal, JPL Open Repository
The Transiting Exoplanet Survey Satellite (TESS) has discovered thousands of new worlds with TESS52 planet candidates now outnumbering the total number of confirmed planets from Kepler. Owing to53 differences in survey design, TESS continues to provide planets that are more amena...
Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3Embargoed
Apr 25, 2024
Catherine Clark, 2024, "Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3", https://doi.org/10.48577/jpl.BEQHTS, Nature, JPL Open Repository
Located at the bottom of the main-sequence, ultracool dwarf stars are widespread in the solar neighborhood. Nevertheless, their extremely low luminosity has left their planetary population largely unexplored, and only one of them, TRAPPIST- 1, has so far been found to host a tran...
VaTEST III: Validation of 8 Potential Super-Earths from TESS DataEmbargoed
Apr 10, 2024
Catherine Clark, 2024, "VaTEST III: Validation of 8 Potential Super-Earths from TESS Data", https://doi.org/10.48577/jpl.HN8VQZ, Proceedings of the International Astronomical Union, JPL Open Repository
NASA’s all-sky survey mission, the Transiting Exoplanet Survey Satellite (TESS), is specifically engineered to detect exoplanets that transit bright stars. Thus far, TESS has successfully identified approximately 400 transiting exoplanets, in addition to roughly 6000 candidate ex...
Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWSTEmbargoed
Mar 15, 2024
Catherine Clark, 2024, "Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST", https://doi.org/10.48577/jpl.QZQUTU, Astronomical Journal, JPL Open Repository
JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5,000 confirmed planets, more than 4,000 TESS planet candidates are still unconfirmed and many of the best planets for atmospheric characterization may remain to be...
NGTS-28Ab: A short period transiting brown dwarfEmbargoed
Feb 15, 2024
Catherine Clark, 2024, "NGTS-28Ab: A short period transiting brown dwarf", https://doi.org/10.48577/jpl.NVKF8M, Monthly Notices of the Royal Astronomical Society, JPL Open Repository
We report the discovery of a brown dwarf orbiting a M1 host star. We first identified the brown dwarf within the Next Generation Transit Survey data, with supporting observations found in TESS sectors 11 and 38. We confirmed the discovery with follow-up photometry from the South...
The POKEMON Speckle Survey of Nearby M dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs Within 15 pcEmbargoed
Feb 14, 2024
Catherine Clark, 2024, "The POKEMON Speckle Survey of Nearby M dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs Within 15 pc", https://doi.org/10.48577/jpl.DEXXTE, Astronomical Journal, JPL Open Repository
M dwarfs are ubiquitous in our galaxy, and the rate at which they host stellar companions, and the10 properties of these companions, provides a window into the formation and evolution of the star(s),11 and of any planets that they may host. The Pervasive Overview of ‘Kompanions’...
Planet Hunters TESS V: a planetary system including a transiting mini-Neptune in the habitable zone of a bright star in a binaryEmbargoed
Jan 25, 2024
Catherine Clark, 2024, "Planet Hunters TESS V: a planetary system including a transiting mini-Neptune in the habitable zone of a bright star in a binary", https://doi.org/10.48577/jpl.NJVBHJ, Astronomical Journal, JPL Open Repository
We report on the discovery and validation of a transiting long-period mini-Neptune orbiting a bright (V = 9.0 mag) G dwarf (TOI 4633; R = 1.05 R⊙, M = 1.10 M⊙). The planet was identified in data from the Transiting Exoplanet Survey Satellite by citizen scientists taking part in t...
Add Data

Sign up or log in to create a dataverse or add a dataset.

Sign Up Log In
Share Dataverse

Share this dataverse on your favorite social media networks.

Link Dataverse
Reset Modifications

Are you sure you want to reset the selected metadata fields? If you do this, any customizations (hidden, required, optional) you have done will no longer appear.