Cosmological MonteCarlo
Primordial power spectrum reconstruction
astro-ph/0302306

• Fig. 1: constraints on n_run
• Fig. 2a: constraints on large-scale cut-off
• Fig. 2b: Large scale multipoles from WMAP with models (below)
• Fig. 3: 16 bins, contributions to the C_l
• Fig. 4: 16 bin shape reconstruction (above plot)
• Fig. 5: 16 bins, constraints on cosmological parameters
• Fig. 6: Constraints on break model parameters
• Fig. 7: Samples from the break model posterior

Please e-mail any questions to Sarah Bridle or Antony Lewis.