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Aaron C. Rizzuto
Researcher at University of Texas at Austin
Publications - 107
Citations - 3975
Aaron C. Rizzuto is an academic researcher from University of Texas at Austin. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 33, co-authored 103 publications receiving 3103 citations. Previous affiliations of Aaron C. Rizzuto include University of Sydney & Macquarie University.
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Journal ArticleDOI
How to Constrain Your M Dwarf. II. The Mass-Luminosity-Metallicity Relation from 0.075 to 0.70 Solar Masses
Journal ArticleDOI
How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$
Andrew W. Mann,Trent J. Dupuy,Adam L. Kraus,Eric Gaidos,Megan Ansdell,Michael J. Ireland,Aaron C. Rizzuto,Chao-Ling Hung,Jason A. Dittmann,Samuel Factor,Gregory A. Feiden,Raquel A. Martinez,Dary Ruíz-Rodríguez,Pa Chia Thao +13 more
TL;DR: The mass-luminosity relation for late-type stars has long been a critical tool for estimating stellar masses as mentioned in this paper, and there is a growing need for both a higher-precision relation and a better understanding of systematic effects (e.g., metallicity).
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Zodiacal exoplanets in time (zeit). iii. a short-period planet orbiting a pre-main-sequence star in the upper scorpius ob association
Andrew W. Mann,Elisabeth R. Newton,Aaron C. Rizzuto,Jonathan Irwin,Gregory A. Feiden,Eric Gaidos,Gregory N. Mace,Adam L. Kraus,David James,Megan Ansdell,David Charbonneau,Kevin R. Covey,Michael J. Ireland,Daniel T. Jaffe,Marshall C. Johnson,Benjamin Kidder,Andrew Vanderburg +16 more
TL;DR: In this article, a super-Neptune-sized (5.04(-0.37) + 0.34) R-circle plus) planet transiting K2-33 (2MASS J16101473-1919095), a late-type (M3) pre-main-sequ...
Journal ArticleDOI
Zodiacal exoplanets in time (zeit). iv. seven transiting planets in the praesepe cluster
Andrew W. Mann,Eric Gaidos,Andrew Vanderburg,Aaron C. Rizzuto,Megan Ansdell,Jennifer Vanessa Medina,Gregory N. Mace,Adam L. Kraus,Kimberly R. Sokal +8 more
TL;DR: In this paper, a search for transiting planets in the ~800 Myr old Praesepe (Beehive, M44) Cluster from K2 light curves is presented. But the authors only identify seven candidates, six of which are statistically validated to be real planets, the last of which requires more data.
Journal ArticleDOI
Multidimensional Bayesian membership analysis of the Sco OB2 moving group
TL;DR: In this paper, a new high-mass membership of the nearby Sco OB2 association based on Hipparcos positions, proper motions and parallaxes, and radial velocities taken from the 2nd Catalogue of Radial Velocities with Astrometric Data (CRVAD-2) was presented.