학술논문

The Baryon Oscillation Spectroscopic Survey of SDSS-III
Document Type
Working Paper
Author
Dawson, Kyle S.Schlegel, David J.Ahn, Christopher P.Anderson, Scott F.Aubourg, ÉricBailey, StephenBarkhouser, Robert H.Bautista, Julian E.Beifiori, AlessandraBerlind, Andreas A.Bhardwaj, VaishaliBizyaev, DmitryBlake, Cullen H.Blanton, Michael R.Blomqvist, MichaelBolton, Adam S.Borde, ArnaudBovy, JoBrandt, W. N.Brewington, HowardBrinkmann, JonBrown, Peter J.Brownstein, Joel R.Bundy, KevinBusca, N. G.Carithers, WilliamCarnero, Aurelio R.Carr, Michael A.Chen, YanmeiComparat, JohanConnolly, NataliaCope, FrancesCroft, Rupert A. C.Cuesta, Antonio J.da Costa, Luiz N.Davenport, James R. A.Delubac, Timothéede Putter, RolandDhital, SauravEalet, AnneEbelke, Garrett L.Eisenstein, Daniel J.Escoffier, S.Fan, XiaohuiAk, N. FilizFinley, HayleyFont-Ribera, AndreuGénova-Santos, R.Gunn, James E.Guo, HongHaggard, DarylHall, Patrick B.Hamilton, Jean-ChristopheHarris, BenHarris, David W.Ho, ShirleyHogg, David W.Holder, DianaHonscheid, KlausHuehnerhoff, JoeJordan, BeatriceJordan, Wendell P.Kauffmann, GuinevereKazin, Eyal A.Kirkby, DavidKlaene, Mark A.Kneib, Jean-PaulGoff, Jean-Marc LeLee, Khee-GanLong, Daniel C.Loomis, Craig P.Lundgren, BrittLupton, Robert H.Maia, Marcio A. G.Makler, MartinMalanushenko, ElenaMalanushenko, ViktorMandelbaum, RachelManera, MarcMaraston, ClaudiaMargala, DanielMasters, Karen L.McBride, Cameron K.McDonald, PatrickMcGreer, Ian D.McMahon, RichardMena, OlgaMiralda-Escudé, JordiMontero-Dorta, Antonio D.Montesano, FrancescoMuna, DemitriMyers, Adam D.Naugle, TracyNichol, Robert C.Noterdaeme, PasquierNuza, Sebastián E.Olmstead, Matthew D.Oravetz, AudreyOravetz, Daniel J.Owen, RussellPadmanabhan, NikhilPalanque-Delabrouille, NathaliePan, KaikeParejko, John K.Pâris, IsabellePercival, Will J.Pérez-Fournon, IsmaelPérez-Ràfols, IgnasiPetitjean, PatrickPfaffenberger, RobertPforr, JaninePieri, Matthew M.Prada, FranciscoPrice-Whelan, Adrian M.Raddick, M. JordanRebolo, RafaelRich, JamesRichards, Gordon T.Rockosi, Constance M.Roe, Natalie A.Ross, Ashley J.Ross, Nicholas P.Rossi, GrazianoRubiño-Martin, J. A.Samushia, LadoSánchez, Ariel G.Sayres, ConorSchmidt, Sarah J.Schneider, Donald P.Scóccola, C. G.Seo, Hee-JongShelden, AlainaSheldon, ErinShen, YueShu, YipingSlosar, AnžeSmee, Stephen A.Snedden, Stephanie A.Stauffer, FritzSteele, OliverStrauss, Michael A.Streblyanska, AlinaSuzuki, NaoSwanson, Molly E. C.Tal, TomerTanaka, MasayukiThomas, DanielTinker, Jeremy L.Tojeiro, RitaTremonti, Christy A.Magana, M. VargasVerde, LiciaViel, MatteoWake, David A.Watson, MikeWeaver, Benjamin A.Weinberg, David H.Weiner, Benjamin J.West, Andrew A.White, MartinWood-Vasey, W. M.Yeche, ChristopheZehavi, IditZhao, Gong-BoZheng, Zheng
Source
Subject
Astrophysics - Cosmology and Nongalactic Astrophysics
Language
Abstract
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 2.15Comment: 49 pages, 16 figures, accepted by AJ