Downloads provided by UsageCountsTHE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III
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Dawson, K.; Schlegel, D.; Ahn, C.; Anderson, S.; Aubourg, É.; Bailey, S.; Barkhouser, R.; +158 Authors
Dawson, K.; Schlegel, D.; Ahn, C.; Anderson, S.; Aubourg, É.; Bailey, S.; Barkhouser, R.; Bautista, J.; Beifiori, A.; Berlind, A.; Bhardwaj, V.; Bizyaev, D.; Blake, C.; Blanton, M.; Blomqvist, M.; Bolton, A.; Borde, A.; Bovy, J.; Brandt, W.; Brewington, H.; Brinkmann, J.; Brown, P.; Brownstein, J.; Bundy, K.; Busca, N.; Carithers, W.; Carnero, A.; Carr, M.; Chen, Y.; Comparat, J.; Connolly, N.; Cope, F.; Croft, R.; Cuesta, A.; da Costa, L.; Davenport, J.; Delubac, T.; de Putter, R.; Dhital, S.; Ealet, A.; Ebelke, G.; Eisenstein, D.; Escoffier, S.; Fan, X.; Ak, N.; Finley, H.; Font-Ribera, A.; Génova-Santos, R.; Gunn, J.; Guo, H.; Haggard, D.; Hall, P.; Hamilton, J.; Harris, B.; Harris, D.; Ho, S.; Hogg, D.; Holder, D.; Honscheid, K.; Huehnerhoff, J.; Jordan, B.; Jordan, W.; Kauffmann, G.; Kazin, E.; Kirkby, D.; Klaene, M.; Kneib, J.; Le Goff, J.; Lee, K.; Long, D.; Loomis, C.; Lundgren, B.; Lupton, R.; Maia, M.; Makler, M.; Malanushenko, E.; Malanushenko, V.; Mandelbaum, R.; Manera, M.; Maraston, C.; Margala, D.; Masters, K.; McBride, C.; McDonald, P.; McGreer, I.; McMahon, R.; Mena, O.; Miralda-Escudé, J.; Montero-Dorta, A.; Montesano, F.; Muna, D.; Myers, A.; Naugle, T.; Nichol, R.; Noterdaeme, P.; Nuza, S.; Olmstead, M.; Oravetz, A.; Oravetz, D.; Owen, R.; Padmanabhan, N.; Palanque-Delabrouille, N.; Pan, K.; Parejko, J.; Pâris, I.; Percival, W.; Pérez-Fournon, I.; Pérez-Ràfols, I.; Petitjean, P.; Pfaffenberger, R.; Pforr, J.; Pieri, M.; Prada, F.; Price-Whelan, A.; Raddick, M.; Rebolo, R.; Rich, J.; Richards, G.; Rockosi, C.; Roe, N.; Ross, A.; Ross, N.; Rossi, G.; Rubiño-Martin, J.; Samushia, L.; Sánchez, A.; Sayres, C.; Schmidt, S.; Schneider, D.; Scóccola, C.; Seo, H.; Shelden, A.; Sheldon, E.; Shen, Y.; Shu, Y.; Slosar, A.; Smee, S.; Snedden, S.; Stauffer, F.; Steele, O.; Strauss, M.; Streblyanska, A.; Suzuki, N.; Swanson, M.; Tal, T.; Tanaka, M.; Thomas, D.; Tinker, J.; Tojeiro, R.; Tremonti, C.; Magaña, M.; Verde, L.; Viel, M.; Wake, D.; Watson, M.; Weaver, B.; Weinberg, D.; Weiner, B.; West, A.; White, M.; Wood-Vasey, W.; Yeche, C.; Zehavi, I.; Zhao, G.; Zheng, Z.;
THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III
The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large scale structure. BOSS uses 1.5 million luminous galaxies as faint as i=19.9 over 10,000 square degrees to measure BAO to redshifts z<0.7. Observations of neutral hydrogen in the Lyman alpha forest in more than 150,000 quasar spectra (g<22) will constrain BAO over the redshift range 2.15
49 pages, 16 figures, accepted by AJ
France, France, France, Spain, Spain, United States, Turkey, Australia, United Kingdom, France, Italy, France
- UNIVERSITE D'AIX MARSEILLE France
- Pennsylvania State University United States
- Columbia University United States
- National Institute for Astrophysics Italy
- Centre national de la recherche scientifique France
ACTIVE GALACTIC NUCLEI, Cosmology and Gravitation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], LY-ALPHA FOREST, FOS: Physical sciences, QUASAR TARGET SELECTION, Astronomy & Astrophysics, Surveys, Astrophysics, LUMINOUS RED GALAXIES, HIGH-REDSHIFT QUASARS, 530, LARGE-AREA TELESCOPE, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], surveys, Observacions astronòmiques, observations [Cosmology], Observations, /dk/atira/pure/core/subjects/cosmology, [SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Science & Technology, Cosmologia, DIGITAL-SKY-SURVEY, Cosmology: observations, Cosmology and Extragalactic Astrophysics, 520, Cosmology, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], cosmology: observations, Physical Sciences, Astronomia, PRINCIPAL COMPONENT ANALYSIS, PROBING DARK ENERGY, BROAD-ABSORPTION-LINE, Astronomical observations, Astrophysics - Cosmology and Nongalactic Astrophysics
ACTIVE GALACTIC NUCLEI, Cosmology and Gravitation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], LY-ALPHA FOREST, FOS: Physical sciences, QUASAR TARGET SELECTION, Astronomy & Astrophysics, Surveys, Astrophysics, LUMINOUS RED GALAXIES, HIGH-REDSHIFT QUASARS, 530, LARGE-AREA TELESCOPE, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], surveys, Observacions astronòmiques, observations [Cosmology], Observations, /dk/atira/pure/core/subjects/cosmology, [SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Science & Technology, Cosmologia, DIGITAL-SKY-SURVEY, Cosmology: observations, Cosmology and Extragalactic Astrophysics, 520, Cosmology, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], cosmology: observations, Physical Sciences, Astronomia, PRINCIPAL COMPONENT ANALYSIS, PROBING DARK ENERGY, BROAD-ABSORPTION-LINE, Astronomical observations, Astrophysics - Cosmology and Nongalactic Astrophysics
selected citations These citations are derived from selected sources.This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).2K popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Top 0.01% influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Top 0.1% impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Top 0.01% views 95 downloads 155 - 95views155downloads
selected citations
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These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP!influenceInfluence provided by BIP!
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Influence provided by BIP!impulseImpulse provided by BIP!
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
Impulse provided by BIP!viewsViews provided by UsageCounts
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Downloads provided by UsageCounts 2K
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