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    • The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey 

      Tegmark, Max; Blanton, Michael; Strauss, Michael; Hoyle, Fiona; Schlegel, David; Scoccimarro, Roman; Vogeley, Michael; Weinberg, David; Zehavi, Idit; Berlind, Andreas; Budavari, Tamás; Connolly, Andrew; Eisenstein, Daniel James; Finkbeiner, Douglas; Frieman, Joshua; Gunn, James; Hamilton, Andrew; Hui, Lam; Jain, Bhuvnesh; Johnston, David; Kent, Stephen; Lin, Huan; Nakajima, Reiko; Nichol, Robert; Ostriker, Jeremiah; Pope, Adrian; Scranton, Ryan; Seljak, Uroš; Sheth, Ravi; Stebbins, Albert; Szalay, Alexander; Szapudi, István; Verde, Licia; Xu, Yongzhong; Annis, James; Bahcall, Neta; Brinkmann, J.; Burles, Scott; Castander, Francisco; Csabai, Istvan; Loveday, Jon; Doi, Mamoru; Fukugita, Masataka; Gott, J.; Hennessy, Greg; Hogg, David; Ivezić, Željko; Knapp, Gillian; Lamb, Don; Lee, Brian; Lupton, Robert; McKay, Timothy; Kunszt, Peter; Munn, Jeffrey; O'Connell, Liam; Peoples, John; Pier, Jeffrey; Richmond, Michael; Rockosi, Constance; Schneider, Donald; Stoughton, Christopher; Tucker, Douglas; Berk, Daniel; Yanny, Brian; York, Donald (IOP Publishing, 2004)
      We measure the large-scale real-space power spectrum P(k) by using a sample of 205,443 galaxies from the Sloan Digital Sky Survey, covering 2417 effective square degrees with mean redshift z ≈ 0.1. We employ a matrix-based ...