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1. Full Text The ninth data release of the sloan digital sky survey: First spectroscopic data from the sdss-iii baryon oscillation spectroscopic survey
by Ahn, Christopher P and Alexandroff, Rachael and Allende Prieto, Carlos and Anderson, Scott F and Anderton, Timothy and Andrews, Brett H and Aubourg, Éric and Bailey, Stephen and Balbinot, Eduardo and Barnes, Rory and Bautista, Julian and Beers, Timothy C and Beifiori, Alessandra and Berlind, Andreas A and Bhardwaj, Vaishali and Bizyaev, Dmitry and Blake, Cullen H and Blanton, Michael R and Blomqvist, Michael and Bochanski, John J and Bolton, Adam S and Borde, Arnaud and Bovy, Jo and Brandt, W.N and Brinkmann, J and Brown, Peter J and Brownstein, Joel R and Bundy, Kevin and Busca, N.G and Carithers, William and Carnero, Aurelio R and Carr, Michael A and Casetti-Dinescu, Dana I and Chen, Yanmei and Chiappini, Cristina and Comparat, Johan and Connolly, Natalia and Crepp, Justin R and Cristiani, Stefano and Croft, Rupert A. C and Cuesta, Antonio J and Da Costa, Luiz N and Davenport, James R. A and Dawson, Kyle S and De Putter, Roland and De Lee, Nathan and Delubac, Timothée and Dhital, Saurav and Ealet, Anne and Ebelke, Garrett L and Edmondson, Edward M and Eisenstein, Daniel J and Escoffier, S and Esposito, Massimiliano and Evans, Michael L and Fan, Xiaohui and Femenía Castellá, Bruno and Fernández Alvar, Emma and Ferreira, Leticia D and Filiz Ak, N and Finley, Hayley and Fleming, Scott W and Font-Ribera, Andreu and Frinchaboy, Peter M and García-Hernández, D.A and Pérez, A. E. García and Ge, Jian and Génova-Santos, R and Gillespie, Bruce A and Girardi, Léo and González Hernández, Jonay I and Grebel, Eva K and Gunn, James E and Guo, Hong and Haggard, Daryl and Hamilton, Jean-Christophe and Harris, David W and Hawley, Suzanne L and Hearty, Frederick R and Ho, Shirley and Hogg, David W and Holtzman, Jon A and Honscheid, Klaus and Huehnerhoff, J and Ivans, Inese I and Ivezić, Željko and Jacobson, Heather R and Jiang, Linhua and Johansson, Jonas and Johnson, Jennifer A and Kauffmann, Guinevere and Kirkby, David and Kirkpatrick, Jessica A and Klaene, Mark A and Knapp, Gillian R and Kneib, Jean-Paul and Le Goff, Jean-Marc and Leauthaud, Alexie and Lee, Khee-Gan and Lee, Young Sun and ... and Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States) and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States) and Brookhaven National Laboratory (BNL), Upton, NY (United States)
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 12/2012, Volume 203, Issue 2, pp. 21 - 13
The Sloan Digital Sky Survey III (SDSS-III) presents the first spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS). This ninth data... 
surveys | catalogs | atlases | TARGET SELECTION | STAR-FORMING GALAXIES | POPULATION SYNTHESIS | RESOLUTION | VALIDATION | MODELS | ASTRONOMY & ASTROPHYSICS | SEGUE | SCALE | MILKY-WAY | Stellar spectra | Quasars | Spectroscopy | Metallicity | Stars | Imaging | Sky surveys (astronomy) | Spectra | Estimates | Cosmologia | Astronomical observations | Observacions astronòmiques | Spectrum analysis | Cosmology | Atles | Espectroscòpia | Atlases | ASTRONOMY AND ASTROPHYSICS
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2. Full Text The clustering of galaxies in the SDSS‐III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Release 9 spectroscopic galaxy sample
by Anderson, Lauren and Aubourg, Eric and Bailey, Stephen and Bizyaev, Dmitry and Blanton, Michael and Bolton, Adam S and Brinkmann, J and Brownstein, Joel R and Burden, Angela and Cuesta, Antonio J and da Costa, Luiz A. N and Dawson, Kyle S and de Putter, Roland and Eisenstein, Daniel J and Gunn, James E and Guo, Hong and Hamilton, Jean‐Christophe and Harding, Paul and Ho, Shirley and Honscheid, Klaus and Kazin, Eyal and Kirkby, David and Kneib, Jean‐Paul and Labatie, Antoine and Loomis, Craig and Lupton, Robert H and Malanushenko, Elena and Malanushenko, Viktor and Mandelbaum, Rachel and Manera, Marc and Maraston, Claudia and McBride, Cameron K and Mehta, Kushal T and Mena, Olga and Montesano, Francesco and Muna, Demetri and Nichol, Robert C and Nuza, Sebastián E and Olmstead, Matthew D and Oravetz, Daniel and Padmanabhan, Nikhil and Palanque‐Delabrouille, Nathalie and Pan, Kaike and Parejko, John and Pâris, Isabelle and Percival, Will J and Petitjean, Patrick and Prada, Francisco and Reid, Beth and Roe, Natalie A and Ross, Ashley J and Ross, Nicholas P and Samushia, Lado and Sánchez, Ariel G and Schlegel, David J and Schneider, Donald P and Scóccola, Claudia G and Seo, Hee‐Jong and Sheldon, Erin S and Simmons, Audrey and Skibba, Ramin A and Strauss, Michael A and Swanson, Molly E. C and Thomas, Daniel and Tinker, Jeremy L and Tojeiro, Rita and Magaña, Mariana Vargas and Verde, Licia and Wagner, Christian and Wake, David A and Weaver, Benjamin A and Weinberg, David H and White, Martin and Xu, Xiaoying and Yèche, Christophe and Zehavi, Idit and Zhao, Gong‐Bo
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2012, Volume 427, Issue 4, pp. 3435 - 3467
ABSTRACT We present measurements of galaxy clustering from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey... 
cosmology: observations | large‐scale structure of Universe | dark energy | distance scale | cosmological parameters | Cosmology: Observations | Cosmological parameters | Dark energy | Large-scale structure of Universe | Distance scale | TARGET SELECTION | COSMOLOGICAL IMPLICATIONS | large-scale structure of Universe | HALO OCCUPATION DISTRIBUTION | LUMINOUS RED GALAXIES | SCALE FLUCTUATIONS | PARAMETER CONSTRAINTS | DIGITAL SKY SURVEY | SYSTEMATIC UNCERTAINTIES | ASTRONOMY & ASTROPHYSICS | POWER-SPECTRUM ANALYSIS | Surveys | Galaxies | Spectra | Cluster analysis | Acoustics | Stars & galaxies | Spectrum analysis | Oscillators | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics
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3. Full Text Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation
by Wojtak, R and Old, L and Mamon, G.A and Pearce, F.R and de Carvalho, R and Sifón, C and Gray, M.E and Skibba, R.A and Croton, D and Bamford, S and Gifford, D and von der Linden, A and Muñoz-Cuartas, J.C and Müller, V and Pearson, R.J and Rozo, E and Rykoff, E and Saro, A and Sepp, T and Tempel, E and SLAC National Accelerator Lab., Menlo Park, CA (United States)
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2018, Volume 481, Issue 1, pp. 324 - 340
The primary difficulty in measuring dynamical masses of galaxy clusters from galaxy data lies in the separation between true cluster members from interloping... 
Galaxies: clusters: general | Galaxies: kinematics and dynamics | Galaxies: haloes | Cosmology: observations | Methods: statistical | Methods: numerical | LUMINOSITY | galaxies: clusters: general | PROFILES | ALGORITHM | CATALOGS | methods: numerical | COSMOLOGICAL CONSTRAINTS | HALO MODEL | DEPENDENCE | methods: statistical | VELOCITY DISPERSIONS | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | cosmology: observations | galaxies: kinematics and dynamics | SATELLITE GALAXIES | galaxies: haloes | Physics - Cosmology and Nongalactic Astrophysics | ASTRONOMY AND ASTROPHYSICS
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4. Full Text Galaxy Cluster Mass Reconstruction Project - II. Quantifying scatter and bias using contrasting mock catalogues
by Old, L and Wojtak, R and Mamon, G.A and Skibba, R.A and Pearce, F.R and Croton, D and Bamford, S and Behroozi, P and de Carvalho, R and Muñoz-Cuartas, J.C and Gifford, D and Gray, M.E and von der Linden, A and Merrifield, M.R and Muldrew, S.I and Müller, V and Pearson, R.J and Ponman, T.J and Rozo, E and Rykoff, E and Saro, A and Sepp, T and Sifón, C and Tempel, E and SLAC National Accelerator Lab., Menlo Park, CA (United States)
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 449, Issue 2, pp. 1897 - 1920
This paper is the second in a series in which we perform an extensive comparison of various galaxy-based cluster mass estimation techniques that utilize the... 
Galaxies: kinematics and dynamics | Galaxies: haloes | Cosmology: observations | Methods: statistical | Methods: numerical | LARGE-SCALE STRUCTURE | MORPHOLOGY-DENSITY RELATION | OF-FRIENDS ALGORITHM | methods: numerical | GROUP FINDER | DARK-MATTER HALOS | methods: statistical | INTERNAL VELOCITY DISPERSIONS | DIGITAL SKY SURVEY | RED-SEQUENCE | ASTRONOMY & ASTROPHYSICS | SDSS | X-RAY | cosmology: observations | galaxies: kinematics and dynamics | galaxies: haloes | ASTRONOMY AND ASTROPHYSICS
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5. Full Text Cosmological constraints from the clustering of the Sloan Digital Sky Survey DR7 luminous red galaxies
by Reid, Beth A and Percival, Will J and Eisenstein, Daniel J and Verde, Licia and Spergel, David N and Skibba, Ramin A and Bahcall, Neta A and Budavari, Tamas and Frieman, Joshua A and Fukugita, Masataka and Gott, J. Richard and Gunn, James E and Ivezić, Željko and Knapp, Gillian R and Kron, Richard G and Lupton, Robert H and McKay, Timothy A and Meiksin, Avery and Nichol, Robert C and Pope, Adrian C and Schlegel, David J and Schneider, Donald P and Stoughton, Chris and Strauss, Michael A and Szalay, Alexander S and Tegmark, Max and Vogeley, Michael S and Weinberg, David H and York, Donald G and Zehavi, Idit
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 404, Issue 1, pp. 60 - 85
We present the power spectrum of the reconstructed halo density field derived from a sample of luminous red galaxies (LRGs) from the Sloan Digital Sky Survey... 
cosmology: observations | large‐scale structure of Universe | galaxies: statistics | galaxies: haloes | Galaxies: statistics | Galaxies: haloes | Cosmology: observations | Large-scale structure of Universe | SPECTROSCOPIC TARGET SELECTION | GRAVITATIONAL-INSTABILITY | HUBBLE-SPACE-TELESCOPE | large-scale structure of Universe | PROBE WMAP OBSERVATIONS | HALO OCCUPATION DISTRIBUTION | DENSITY FIELD | ASTRONOMY & ASTROPHYSICS | REDSHIFT SURVEY | SCALE | DATA RELEASE | POWER-SPECTRUM ANALYSIS | Surveys | Particle accelerators | Galaxies | Anisotropy | Astronomy | Force and energy | Luminosity | Cosmology | Dark matter | Star maps | Stars & galaxies | Physics - Cosmology and Nongalactic Astrophysics
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6. Full Text The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function
by Sánchez, Ariel G and Scóccola, C. G and Ross, A. J and Percival, W and Manera, M and Montesano, F and Mazzalay, X and Cuesta, A. J and Eisenstein, D. J and Kazin, E and McBride, C. K and Mehta, K and Montero-Dorta, A. D and Padmanabhan, N and Prada, F and Rubiño-Martín, J. A and Tojeiro, R and Xu, X and Magaña, M. Vargas and Aubourg, E and Bahcall, N. A and Bailey, S and Bizyaev, D and Bolton, A. S and Brewington, H and Brinkmann, J and Brownstein, J. R and Gott, J. Richard and Hamilton, J. C and Ho, S and Honscheid, K and Labatie, A and Malanushenko, E and Malanushenko, V and Maraston, C and Muna, D and Nichol, R. C and Oravetz, D and Pan, K and Ross, N. P and Roe, N. A and Reid, B. A and Schlegel, D. J and Shelden, A and Schneider, D. P and Simmons, A and Skibba, R and Snedden, S and Thomas, D and Tinker, J and Wake, D. A and Weaver, B. A and Weinberg, David H and White, Martin and Zehavi, I and Zhao, G
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 9/2012, Volume 425, Issue 1, pp. 415 - 437
Abstract We obtain constraints on cosmological parameters from the spherically averaged redshift-space correlation function of the CMASS Data Release 9 (DR9)... 
large‐scale structure of Universe | cosmological parameters | Large-scale structure of Universe | Cosmological parameters | POWER-SPECTRUM | HUBBLE-SPACE-TELESCOPE | large-scale structure of Universe | PROBE WMAP OBSERVATIONS | DARK ENERGY | ACOUSTIC-OSCILLATIONS | LUMINOUS RED GALAXIES | DIGITAL SKY SURVEY | SYSTEMATIC UNCERTAINTIES | ASTRONOMY & ASTROPHYSICS | REDSHIFT SURVEY | DATA RELEASE | Atoms & subatomic particles | Astrophysics | Dark matter | Spectrum analysis | Stars & galaxies | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Cosmology and Extra-Galactic Astrophysics | Physics
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7. Full Text The clustering of galaxies in the SDSS-III baryon oscillation spectroscopic survey: Baryon acoustic oscillations in the data releases 10 and 11 galaxy samples
by Anderson, Lauren and Aubourg, Élric and Bailey, Stephen and Beutler, Florian and Bhardwaj, Vaishali and Blanton, Michael and Bolton, Adam S and Brinkmann, J and Brownstein, Joel R and Burden, Angela and Chuang, Chia-Hsun and Cuesta, Antonio J and Dawson, Kyle S and Eisenstein, Daniel J and Escoffier, Stephanie and Gunn, James E and Guo, Hong and Ho, Shirley and Honscheid, Klaus and Howlett, Cullan and Kirkby, David and Lupton, Robert H and Manera, Marc and Maraston, Claudia and McBride, Cameron K and Mena, Olga and Montesano, Francesco and Nichol, Robert C and Nuza, Sebastián E and Olmstead, Matthew D and Padmanabhan, Nikhil and Palanque-Delabrouille, Nathalie and Parejko, John and Percival, Will J and Petitjean, Patrick and Prada, Francisco and Price-Whelan, Adrian M and Reid, Beth and Roe, Natalie A and Ross, Ashley J and Ross, Nicholas P and Sabiu, Cristiano G and Saito, Shun and Samushia, Lado and Sánchez, Ariel G and Schlegel, David J and Schneider, Donald P and Scoccola, Claudia G and Seo, Hee-Jong and Skibba, Ramin A and Strauss, Michael A and C. Swanson, Molly E and Thomas, Daniel and Tinker, Jeremy L and Tojeiro, Rita and Magaña, Mariana Vargas and Verde, Licia and Wake, David A and Weaver, Benjamin A and Weinberg, David H and White, Martin and Xu, Xiaoying and Yèche, Christophe and Zehavi, Idit and Zhao, Gong-Bo
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, Volume 441, Issue 1, pp. 24 - 62
We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations (BAO) in the clustering of galaxies... 
Cosmological parameters | Dark energy | Cosmology: observations | Large-scale structure of Universe | Distance scale | CALIBRATION | HUBBLE-SPACE-TELESCOPE | large-scale structure of Universe | dark energy | distance scale | TO 0.5 | LUMINOUS RED GALAXIES | EVOLUTION | CENT DISTANCE | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | cosmology: observations | SCALE | UNIVERSE | cosmological parameters | POWER-SPECTRUM ANALYSIS | Cosmologia | Astrofísica | Espectroscòpia de microones | Astrophysics | Astronomical observations | Observacions astronòmiques | Microwave spectroscopy | Cosmology
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