NUV and FUV measurements of planet host stars

R. O.Parke Loyd (Contributor)
Evgenya Shkolnik (Creator)
A. Schneider (Creator)
Tyler Richey-Yowell (Creator)
Travis Barman (Creator)
Sarah Peacock (Creator)
Isabella Pagano (Creator)

Dataset

Description

VizieR online Data Catalogue associated with article published in journal Astronomical Journal (AAS) with title 'Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap.' (bibcode: 2020ApJ...890...23L)

Date made available	2021
Publisher	Strasbourg Astronomical Data Center

DOI
10.26093/cds/vizier.18900023

Access Dataset

Refer to CDS usage

1 Article

Current Population Statistics Do Not Favor Photoevaporation over Core-powered Mass Loss as the Dominant Cause of the Exoplanet Radius Gap
Loyd, R. O. P., Shkolnik, E. L., Schneider, A. C., Richey-Yowell, T., Barman, T. S., Peacock, S. & Pagano, I., Feb 10 2020, In: Astrophysical Journal. 890, 1, 23.
Research output: Contribution to journal › Article › peer-review

Open Access
29 Scopus citations

NUV and FUV measurements of planet host stars

Description

DOI

Access Dataset

Research output

Current Population Statistics Do Not Favor Photoevaporation over Core-powered Mass Loss as the Dominant Cause of the Exoplanet Radius Gap

Cite this