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R. Stompor

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • last author1

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.CO2
ORCID 0000-0002-9777-3813
same name
  • R. Stompor — 3 papers, h 86

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedComponent separation methods for the Planck mission

256 citations · 462 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.CO2009★ 4 cited

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…

astro-ph.CO2009★ 90 cited

Polarized CMB power spectrum estimation using the pure pseudo-cross-spectrum approach

J. Grain, M. Tristram, R. Stompor

We extend the pure pseudo-power-spectrum formalism proposed recently in the context of the Cosmic Microwave Background polarized power spectra estimation by Smith (2006) to incorpo…

astro-ph2008★ 256 cited

Component separation methods for the Planck mission

S. M. Leach, J. -F. Cardoso, C. Baccigalupi +27

The Planck satellite will map the full sky at nine frequencies from 30 to 857 GHz. The CMB intensity and polarization that are its prime targets are contaminated by foreground emis…

astro-ph2008★ 112 cited

Maximum Likelihood algorithm for parametric component separation in CMB experiments

R. Stompor, S. Leach, F. Stivoli +1

We discuss an approach to the component separation of microwave, multi-frequency sky maps as those typically produced from Cosmic Microwave Background (CMB) Anisotropy data sets. T…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.