The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data

Early photometric data from the Sloan Digital Sky Survey (SDSS) contain angular positions for 1.5 million galaxies. In companion papers, the angular correlation function $w(\theta)$ and 2D power spectrum $C_l$ of these galaxies are presented. Here we invert Limber's equation to extract the 3D p...

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Detalles Bibliográficos
Autores principales: Dodelson, Scott, Narayanan, Vijay K., Tegmark, Max, Scranton, Ryan, Budavari, Tamas, Connolly, Andrew, Csabai, Istvan, Eisenstein, Daniel, Frieman, Joshua A., Gunn, James E., Hui, Lam, Jain, Bhuvnesh, Johnston, David, Kent, Stephen M., Loveday, Jon, Nichol, Robert C., O'Connell, Liam, Scoccimarro, Roman, Sheth, Ravi K., Stebbins, Albert, Strauss, Michael A., Szalay, Alexander S., Szapudi, Istvan, Vogeley, Michael S., Zehavi, Idit, Annis, James, Bahcall, Neta A., Brinkman, Jon, Doi, Mamoru, Fukugita, Masataka, Hennessy, Greg, Ivezic, Zeljko, Knapp, Gillian R., Kunszt, Peter, Lamb, Don Q., Lee, Brian C., Lupton, Robert H., Munn, Jeffrey A., Peoples, John, Pier, Jeffrey R., Rockosi, Constance, Schlegel, David, Stoughton, Christopher, Tucker, Douglas L., Yanny, Brian, York, Donald G.
Lenguaje:eng
Publicado: 2001
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1086/340225
http://cds.cern.ch/record/530960

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