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M. I. R. Alves

3 papers here

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

author position
  • middle author1

Across the 1 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
ORCID 0009-0007-4003-4650
same name
  • M. I. R. Alves — 1 paper

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 citedPlanck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust

422 citations · 617 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2014★ 422 cited

Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust

Planck Collaboration, P. A. R. Ade, N. Aghanim +199

This paper presents the large-scale polarized sky as seen by Planck HFI at 353 GHz, which is the most sensitive Planck channel for dust polarization. We construct and analyse large…

astro-ph.GA2014★ 190 cited

Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization

Planck Collaboration, P. A. R. Ade, M. I. R. Alves +177

Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We make use of the Planck 353 GHz I, Q, and U Stokes maps as du…

astro-ph.GA2014★ 5 cited

The pros and cons of the inversion method approach to derive 3D dust emission properties of the ISM: the Hi-GAL field centred on (l,b)=(30∘,0∘)

Alessio Traficante, Roberta Paladini, Mathieu Compiegne +13

Herschel FIR continuum data obtained as part of the Hi-GAL survey have been used, together with the GLIMPSE 8 μm and MIPSGAL 24 μm data, to attempt the first 3D-decomposition o…

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