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arxiv: 0807.0624 · v1 · pith:V5VIGJRPnew · submitted 2008-07-03 · 🌌 astro-ph · physics.data-an

A Markov Chain Monte Carlo Algorithm for analysis of low signal-to-noise CMB data

classification 🌌 astro-ph physics.data-an
keywords algorithmsignal-to-noisegibbsmovesampleranalysiscarlochain
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We present a new Monte Carlo Markov Chain algorithm for CMB analysis in the low signal-to-noise regime. This method builds on and complements the previously described CMB Gibbs sampler, and effectively solves the low signal-to-noise inefficiency problem of the direct Gibbs sampler. The new algorithm is a simple Metropolis-Hastings sampler with a general proposal rule for the power spectrum, C_l, followed by a particular deterministic rescaling operation of the sky signal. The acceptance probability for this joint move depends on the sky map only through the difference of chi-squared between the original and proposed sky sample, which is close to unity in the low signal-to-noise regime. The algorithm is completed by alternating this move with a standard Gibbs move. Together, these two proposals constitute a computationally efficient algorithm for mapping out the full joint CMB posterior, both in the high and low signal-to-noise regimes.

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