L
Luca Rizzi
Researcher at W.M. Keck Observatory
Publications - 94
Citations - 5352
Luca Rizzi is an academic researcher from W.M. Keck Observatory. The author has contributed to research in topics: Galaxy & Red-giant branch. The author has an hindex of 32, co-authored 87 publications receiving 4629 citations. Previous affiliations of Luca Rizzi include University of Hawaii & University of Padua.
Papers
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Journal ArticleDOI
Cosmicflows-2: the data
R. Brent Tully,Hélène M. Courtois,Hélène M. Courtois,Andrew E. Dolphin,J. Richard Fisher,Philippe Héraudeau,Bradley A. Jacobs,Igor D. Karachentsev,Dmitry Makarov,Lidia Makarova,Sofia Mitronova,Luca Rizzi,Edward J. Shaya,Jenny G. Sorce,Po-Feng Wu +14 more
TL;DR: Cosmicflows-2 as mentioned in this paper is a compilation of distances and peculiar velocities for over 8000 galaxies, and the largest contributions come from the luminosity-line width correlation for spirals, the Tully-Fisher relation (TFR), and the related fundamental plane relation for E/S0 systems.
Journal ArticleDOI
The Extragalactic Distance Database
R. Brent Tully,Luca Rizzi,Edward J. Shaya,Hélène M. Courtois,Hélène M. Courtois,Dmitry Makarov,Dmitry Makarov,Bradley A. Jacobs +7 more
TL;DR: A database can be accessed on the Web at http://eddifa.hawaii.edu that was developed to promote access to information related to galaxy distances as mentioned in this paper, where tables from many literature sources have been gathered and enhanced with links through a distinct galaxy naming convention.
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Our Peculiar Motion Away from the Local Void
R. Brent Tully,Edward J. Shaya,Igor D. Karachentsev,Hélène M. Courtois,Dale D. Kocevski,Luca Rizzi,Alan Peel +6 more
TL;DR: In this article, the peculiar velocity of the Local Group of galaxies manifested in the cosmic microwave background dipole is found to decompose into three dominant components, the nearest being a velocity discontinuity at 7 Mpc, the second being an attraction on scales larger than 3000 km s−1 and centered near the direction of the Centaurus Cluster.
Journal ArticleDOI
Tip of the Red Giant Branch Distances. II. Zero-Point Calibration
Luca Rizzi,R. Brent Tully,Dmitry Makarov,Dmitry Makarov,Dmitry Makarov,Lidia Makarova,Lidia Makarova,Lidia Makarova,Andrew E. Dolphin,Shoko Sakai,Edward J. Shaya +10 more
TL;DR: The zero point of the red giant branch (TRGB) was established with a statistical accuracy of 1%, modulo the uncertainty in the magnitude of the horizontal branch, with a typical rms uncertainty of 3% in individual galaxy distances at high Galactic latitude as mentioned in this paper.
Posted Content
The Extragalactic Distance Database
R. Brent Tully,Luca Rizzi,Edward J. Shaya,Hélène M. Courtois,Hélène M. Courtois,Dmitry Makarov,Dmitry Makarov,Bradley A. Jacobs +7 more
TL;DR: In this article, the authors present a database for information related to galaxy distances and compare results both at the levels of parameters and techniques, leading to increasing homogeneity and consistency of distance measurements.