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researcher

R. Stompor

15 papers here

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

author position
  • middle author4

Across the 4 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO10
  • astro-ph.IM3
  • astro-ph2
ORCID 0000-0002-9777-3813
same name
  • R. Stompor — 170 papers, h 86
  • R. Stompor — 8 papers, h 8
  • R. Stompor — 4 papers

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

activity
19982016
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 13.5k across the 15 of their papers we have counts for

collaborators
Showing 2015Show all

4 papers · 1 filter

astro-ph.CO2015★ 183 cited

Planck 2015 results. XXI. The integrated Sachs-Wolfe effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +229

This paper presents a study of the ISW effect from the Planck 2015 temperature and polarization data release. The CMB is cross-correlated with different LSS tracers: the NVSS, SDSS…

astro-ph.CO2015★ 10.6k cited

Planck 2015 results. XIII. Cosmological parameters

Planck Collaboration, P. A. R. Ade, N. Aghanim +259

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary…

astro-ph.CO2015★ 40 cited

Planck 2015 results. I. Overview of products and scientific results

Planck Collaboration, R. Adam, P. A. R. Ade +352

The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submilli…

astro-ph.IM2015★ 40 cited

Modeling atmospheric emission for CMB ground-based observations

J. Errard, P. A. R. Ade, Y. Akiba +72

Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies t…

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