Neptune-like planets low-density overabundance (Cubillos+ 2017)

We compiled our sample by collecting and cross-checking the lists of exoplanets from the NASA Exoplanet Archive (http://exoplanetarchive.ipac.caltech.edu), the Exoplanets Data Explorer (http://exoplanets.org, Han et al. 2014PASP..126..827H), and The Extrasolar Planets Encyclopaedia (http://exoplanet.eu, Schneider et al. 2012, ASP Conf. Ser. 461, 447). We selected the targets with measured planetary radii and masses, whose mass is less than ~2 Neptune masses (Mp<30M-{Eeath}). We adopted stellar rotational angular velocity ({Omage}_rot) from McQuillan, Mazeh & Aigrain (2013, Cat. J/ApJ/775/L11) and ages from Morton et al. (2016, Cat. J/ApJ/822/86). Our final sample consists of 167 planets (Table A1).

Identifier
Source http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/MNRAS/466/1868
Related Identifier https://ui.adsabs.harvard.edu/abs/2017MNRAS.466.1868C
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_datacite&identifier=ivo://CDS.VizieR/J/MNRAS/466/1868
Provenance
Creator Cubillos P., Erkaev N.V., Juvan I., Fossati L., Johnstone C.P., Lammer H., Lendl M., Odert P., Kislyakova K.G.
Publisher CDS
Contributor International Virtual Observatory Alliance (IVOA)
Publication Year 2020
Rights public
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Format text/xml+votable
Version 15-Oct-2019
Discipline Astrophysics and Astronomy