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POKER: Estimating the power spectrum of diffuse emission with complex masks and at high angular resolution

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arxiv 1111.0766 v1 pith:77LQCTWL submitted 2011-11-03 astro-ph.CO

POKER: Estimating the power spectrum of diffuse emission with complex masks and at high angular resolution

classification astro-ph.CO
keywords angulardiffuseemissionestimatorhighpokerpowerresolution
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We describe the implementation of an angular power spectrum estimator in the flat sky approximation. POKER (P. Of k EstimatoR) is based on the MASTER algorithm developped by Hivon and collaborators in the context of CMB anisotropy. It works entirely in discrete space and can be applied to arbitrary high angular resolution maps. It is therefore particularly suitable for current and future infrared to sub-mm observations of diffuse emission, whether Galactic or cosmological.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Testing masking effectiveness using multi-line image cubes based on COSMOS2020 for [CII] line intensity mapping at $z_{[CII]} > 3.5$

    astro-ph.GA 2026-06 unverdicted novelty 3.0

    Simulations from COSMOS2020 show masking recovers [CII] above 300 GHz in ideal conditions but noise prevents useful S/N until near the end of 2000-hour observations.