Higher order moments of the angular distribution of galaxies from early Sloan Digital Sky Survey data

István Szapudi, Joshua A. Frieman, Roman Scoccimarro, Alexander S. Szalay, Andrew J. Connolly, Scott Dodelson, Daniel J. Eisenstein, James E. Gunn, David Johnston, Stephen Kent, Jon Loveday, Avery Meiksin, Robert C. Nichol, Ryan Scranton, Albert Stebbins, Michael S. Vogeley, James Annis, Neta A. Bahcall, J. Brinkman, István CsabaiMamoru Doi, Masataka Fukugita, Željko Ivezić, Rita S.J. Kim, Gillian R. Knapp, Don Q. Lamb, Brian C. Lee, Robert H. Lupton, Timothy A. McKay, Jeff Munn, John Peoples, Jeff Pier, Constance Rockosi, David Schlegel, Christopher Stoughton, Douglas L. Tucker, Brian Yanny, Donald G. York

Research output: Contribution to journalReview article

40 Scopus citations

Abstract

We present initial results for counts in cell statistics of the angular distribution of galaxies in early data from the Sloan Digital Sky Survey (SDSS). We analyze a rectangular stripe 2°.5 wide, covering approximately 160 deg2, containing over 106 galaxies in the apparent magnitude range 18 < r′ < 22, with areas of bad seeing, contamination from bright stars, ghosts, and high galactic extinction masked out. This survey region, which forms part of the SDSS early data release, is the same as that for which two-point angular clustering statistics have recently been computed. The third and fourth moments of the cell counts, s 3 (skewness) and s4 (kurtosis), constitute the most accurate measurements to date of these quantities (for r′ < 21) over angular scales 0°.015-0°.3. They display the approximate hierarchical scaling expected from nonlinear structure formation models and are in reasonable agreement with the predictions of Λ-dominated cold dark matter models with galaxy biasing that suppresses higher order correlations at small scales. The results are, in general, consistent with previous measurements in the APM, EDSGC, and Deeprange surveys. These results suggest that the SDSS imaging data are free of systematics to a high degree and will therefore enable determination of the skewness and kurtosis to 1% and less then 10%, as predicted earlier.

Original languageEnglish (US)
Pages (from-to)75-85
Number of pages11
JournalAstrophysical Journal
Volume570
Issue number1 I
DOIs
StatePublished - May 1 2002

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: clusters: general
  • Large-scale structure of universe

Fingerprint Dive into the research topics of 'Higher order moments of the angular distribution of galaxies from early Sloan Digital Sky Survey data'. Together they form a unique fingerprint.

  • Cite this

    Szapudi, I., Frieman, J. A., Scoccimarro, R., Szalay, A. S., Connolly, A. J., Dodelson, S., Eisenstein, D. J., Gunn, J. E., Johnston, D., Kent, S., Loveday, J., Meiksin, A., Nichol, R. C., Scranton, R., Stebbins, A., Vogeley, M. S., Annis, J., Bahcall, N. A., Brinkman, J., ... York, D. G. (2002). Higher order moments of the angular distribution of galaxies from early Sloan Digital Sky Survey data. Astrophysical Journal, 570(1 I), 75-85. https://doi.org/10.1086/339574