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Dana I. Casetti-Dinescu

Researcher at Southern Connecticut State University

Publications -  72
Citations -  5381

Dana I. Casetti-Dinescu is an academic researcher from Southern Connecticut State University. The author has contributed to research in topics: Stars & Proper motion. The author has an hindex of 28, co-authored 71 publications receiving 5116 citations. Previous affiliations of Dana I. Casetti-Dinescu include Yale University & Wesleyan University.

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The ninth data release of the sloan digital sky survey: First spectroscopic data from the sdss-iii baryon oscillation spectroscopic survey

Christopher P. Ahn, +259 more
TL;DR: In this paper, the authors presented the first spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS) for the Sloan Digital Sky Survey III (SDSS-III) dataset.
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The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey

Christopher P. Ahn, +225 more
TL;DR: In this paper, the Sloan Digital Sky Survey III (SDSS-III) presented the first spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS), along with the data presented in previous data releases.
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The southern proper motion program. iv. the spm4 catalog

TL;DR: The Yale/San Juan Southern Proper Motion Catalog (SPM4) as mentioned in this paper contains absolute proper motions, celestial coordinates, and B, V photometry for over 103 million stars and galaxies between the south celestial pole and -20{sup 0} declination.
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Chemical Abundances and Kinematics in Globular Clusters and Local Group Dwarf Galaxies and Their Implications for Formation Theories of the Galactic Halo

TL;DR: In this article, detailed abundances of a variety of elements between the halo and all dwarf galaxies studied to date, including both dwarf spheroidals and irregulars, were compared.
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Kinematic decoupling of globular clusters with the extended horizontal branch

TL;DR: In this article, the authors show that about 25% of the Milky Way globular clusters (GCs) exhibit unusually extended color distribution of stars in the core helium-burning horizontal-branch (HB) phase.