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Institution

University of California, Santa Cruz

EducationSanta Cruz, California, United States
About: University of California, Santa Cruz is a education organization based out in Santa Cruz, California, United States. It is known for research contribution in the topics: Galaxy & Population. The organization has 15541 authors who have published 44120 publications receiving 2759983 citations. The organization is also known as: UCSC & UC, Santa Cruz.
Topics: Galaxy, Population, Star formation, Redshift, Planet


Papers
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Journal ArticleDOI
Brian Yanny1, Constance M. Rockosi2, Heidi Jo Newberg3, Gillian R. Knapp4, Jennifer K. Adelman-McCarthy1, Bonnie Alcorn1, S. Allam1, Carlos Allende Prieto5, Carlos Allende Prieto6, Deokkeun An7, K. S. J. Anderson8, K. S. J. Anderson9, Scott F. Anderson10, Coryn A. L. Bailer-Jones11, Steve Bastian1, Timothy C. Beers12, Eric F. Bell11, Vasily Belokurov13, Dmitry Bizyaev9, Norm Blythe9, John J. Bochanski10, William N. Boroski1, Jarle Brinchmann14, J. Brinkmann9, Howard Brewington9, Larry N. Carey10, Kyle M. Cudworth15, Michael L. Evans10, Nick Evans13, Evalyn Gates15, Boris T. Gänsicke16, Bruce Gillespie9, G. F. Gilmore13, Ada Nebot Gomez-Moran, Eva K. Grebel17, Jim Greenwell10, James E. Gunn4, Cathy Jordan9, Wendell Jordan9, Paul Harding18, Hugh C. Harris, John S. Hendry1, Diana Holder9, Inese I. Ivans4, Željko Ivezić10, Sebastian Jester11, Jennifer A. Johnson7, Stephen M. Kent1, S. J. Kleinman9, Alexei Y. Kniazev11, Jurek Krzesinski9, Richard G. Kron15, Nikolay Kuropatkin1, Svetlana Lebedeva1, Young Sun Lee12, R. French Leger1, Sébastien Lépine19, Steve Levine, Huan Lin1, Dan Long9, Craig P. Loomis4, Robert H. Lupton4, O. Malanushenko9, Viktor Malanushenko9, Bruce Margon2, David Martínez-Delgado11, P. M. McGehee20, Dave Monet, Heather L. Morrison18, Jeffrey A. Munn, Eric H. Neilsen1, Atsuko Nitta9, John E. Norris21, Daniel Oravetz9, Russell Owen10, Nikhil Padmanabhan22, Kaike Pan9, R. S. Peterson1, Jeffrey R. Pier, Jared Platson1, Paola Re Fiorentin23, Paola Re Fiorentin11, Gordon T. Richards24, Hans-Walter Rix11, David J. Schlegel22, Donald P. Schneider25, Matthias R. Schreiber26, Axel Schwope, Valena C. Sibley1, Audrey Simmons9, Stephanie A. Snedden9, J. Allyn Smith27, Larry Stark10, Fritz Stauffer9, Matthias Steinmetz, Christopher Stoughton1, Mark SubbaRao15, Mark SubbaRao28, Alexander S. Szalay29, Paula Szkody10, Aniruddha R. Thakar29, Sivarani Thirupathi12, Douglas L. Tucker1, A. Uomoto30, Daniel E. Vanden Berk25, S. Vidrih17, Yogesh Wadadekar31, Yogesh Wadadekar4, S. Watters9, R. Wilhelm32, Rosemary F. G. Wyse29, Jean Yarger9, Daniel B. Zucker13 
TL;DR: The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey as mentioned in this paper obtained approximately 240,000 moderate-resolution spectra from 3900 to 9000 of fainter Milky Way stars (14.0 10 per resolution element).
Abstract: The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained {approx}240,000 moderate-resolution (R {approx} 1800) spectra from 3900 {angstrom} to 9000 {angstrom} of fainter Milky Way stars (14.0 10 per resolution element, stellar atmospheric parameters are estimated, including metallicity, surface gravity, and effective temperature. SEGUE obtained 3500 deg{sup 2} of additional ugriz imaging (primarily at low Galactic latitudes) providing precise multicolor photometry ({sigma}(g, r, i) {approx} 2%), ({sigma}(u, z) {approx} 3%) and astrometry ({approx}0.1) for spectroscopic target selection. The stellar spectra, imaging data, and derived parameter catalogs for this survey are publicly available as part of Sloan Digital Sky Survey Data Release 7.

1,133 citations

01 Jan 2007
TL;DR: It is shown that appearance models for these three problems can be evaluated using a cumulative matching curve on a standardized dataset, and that this one curve can be converted to a synthetic reacquisition or disambiguation rate for tracking.
Abstract: Traditionally, appearance models for recognition, reacquisition and tracking problems have been evaluated independently using metrics applied to a complete system. It is shown that appearance models for these three problems can be evaluated using a cumulative matching curve on a standardized dataset, and that this one curve can be converted to a synthetic reacquisition or disambiguation rate for tracking. A challenging new dataset for viewpoint invariant pedestrian recognition (VIPeR) is provided as an example. This dataset contains 632 pedestrian image pairs from arbitrary viewpoints. Several baseline methods are tested on this dataset and the results are presented as a benchmark for future appearance models and matchin methods.

1,121 citations

Journal ArticleDOI
04 Jun 1987-Nature
TL;DR: Chemical footprinting shows that several classes of antibiotics protect concise sets of highly conserved nucleotides in 16S ribosomal RNA when bound to ribosomes, having strong implications for the mechanism of action of these antibiotics and for the assignment of functions to specific structural features of 16S rRNA.
Abstract: Chemical footprinting shows that several classes of antibiotics (streptomycin, tetracycline, spectinomycin, edeine, hygromycin and the neomycins) protect concise sets of highly conserved nucleotides in 16S ribosomal RNA when bound to ribosomes These findings have strong implications for the mechanism of action of these antibiotics and for the assignment of functions to specific structural features of 16S rRNA

1,116 citations

Journal ArticleDOI
TL;DR: Substantial data support the hypothesis that partially folded intermediates are key precursors to aggregates, that aggregation involves specific intermolecular interactions and that most aggregates involve beta sheets.

1,115 citations

Journal ArticleDOI
Jennifer K. Adelman-McCarthy1, Marcel A. Agüeros2, S. Allam1, S. Allam3  +149 moreInstitutions (47)
TL;DR: The fourth data release of the Sloan Digital Sky Survey (SDSS) as discussed by the authors includes all survey-quality data taken through 2004 June, including five-band photometric data for 180 million objects selected over 6670 deg2 and 673,280 spectra of galaxies, quasars and stars selected from 4783 deg2 of those imaging data using the standard SDSS target selection algorithms.
Abstract: This paper describes the Fourth Data Release of the Sloan Digital Sky Survey (SDSS), including all survey-quality data taken through 2004 June. The data release includes five-band photometric data for 180 million objects selected over 6670 deg2 and 673,280 spectra of galaxies, quasars, and stars selected from 4783 deg2 of those imaging data using the standard SDSS target selection algorithms. These numbers represent a roughly 27% increment over those of the Third Data Release; all the data from previous data releases are included in the present release. The Fourth Data Release also includes an additional 131,840 spectra of objects selected using a variety of alternative algorithms, to address scientific issues ranging from the kinematics of stars in the Milky Way thick disk to populations of faint galaxies and quasars.

1,110 citations


Authors

Showing all 15733 results

NameH-indexPapersCitations
David J. Schlegel193600193972
David R. Williams1782034138789
John R. Yates1771036129029
David Haussler172488224960
Evan E. Eichler170567150409
Anton M. Koekemoer1681127106796
Mark Gerstein168751149578
Alexander S. Szalay166936145745
Charles M. Lieber165521132811
Jorge E. Cortes1632784124154
M. Razzano155515106357
Lars Hernquist14859888554
Aaron Dominguez1471968113224
Taeghwan Hyeon13956375814
Garth D. Illingworth13750561793
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202351
2022328
20212,157
20202,353
20192,209
20182,157