pith. sign in

R. Cen

Identifiers

  • name variant R. Cen 0.60 · backfill

Papers (18)

  1. What Powers Lyman alpha Blobs? astro-ph.GA · 2015 · author #5
  2. Building galaxies by accretion and in-situ star formation astro-ph.CO · 2012 · author #2
  3. Probing the first galaxies with the SKA astro-ph.CO · 2010 · author #4
  4. Tracing the Warm Hot Intergalactic Medium in the local Universe astro-ph · 2004 · author #3
  5. WHIM emission and the cluster soft excess: a model comparison astro-ph · 2004 · author #3
  6. Physical effects on the Lyman-alpha forest flux power spectrum: damping wings, ionizing radiation fluctuations, and galactic winds astro-ph · 2004 · author #3
  7. The Linear Theory Power Spectrum from the Lyman-alpha Forest in the Sloan Digital Sky Survey astro-ph · 2004 · author #3
  8. Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy astro-ph · 2004 · author #8
  9. Precision Cosmology from the Lyman-alpha Forest: Power Spectrum and Bispectrum astro-ph · 2003 · author #4
  10. The Mass-To-Light Function: Antibias and Omega_m astro-ph · 2000 · author #2
  11. The Santa Barbara cluster comparison project: a comparison of cosmological hydrodynamics solutions astro-ph · 1999 · author #7
  12. Steps toward the power spectrum of matter. III. The primordial spectrum astro-ph · 1998 · author #8
  13. Steps toward the power spectrum of matter. II. The biasing correction with sigma_8 normalization astro-ph · 1998 · author #6
  14. Steps toward the power spectrum of matter. I.The mean spectrum of galaxies astro-ph · 1998 · author #9
  15. New Statistical Measures of the Lya Forest Spectra for Accurate Comparison to Theoretical Models astro-ph · 1997 · author #8
  16. The Opacity of the Lyman Alpha Forest and Implications for Omega_{baryon} and the Ionizing Background astro-ph · 1996 · author #8
  17. The Local Group as a test of cosmological models astro-ph · 1996 · author #3
  18. Can Standard Cosmological Models Explain the Observed Abell Cluster Bulk Flow? astro-ph · 1994 · author #2

Mentions

  • 1206.0295 #2 · backfill · confidence 0.70 R. Cen
  • 1009.0950 #4 · backfill · confidence 0.70 R. Cen

Frequent Coauthors