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S. Galli

128 papers hereh-index 7650.5k citations253 works total

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

author position
  • sole author1
  • first author10
  • middle author44
  • last author1

Across the 56 of 128 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO91
  • astro-ph.GA15
  • astro-ph.IM14
  • astro-ph2
  • astro-ph.EP2
  • astro-ph.HE2
same name
  • S. Galli — 21 papers, h 5
  • S. Galli — 8 papers
  • S. Galli — 3 papers, h 1
  • S. Galli — 1 paper, h 19
  • S. Galli — 1 paper, h 2
  • S. Galli — 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

activity
20082026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 27.8k across the 126 of their papers we have counts for

collaborators
Showing 2016 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2016★ 33 cited

Exploring Cosmic Origins with CORE: Extragalactic sources in Cosmic Microwave Background maps

G. De Zotti, J. Gonzalez-Nuevo, M. Lopez-Caniego +121

We discuss the potential of a next generation space-borne Cosmic Microwave Background (CMB) experiment for studies of extragalactic sources. Our analysis has particular bearing on…

astro-ph.GA2016★ 26 cited

Planck intermediate results. XLV. Radio spectra of northern extragalactic radio sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +202

Continuum spectra covering centimetre to submillimetre wavelengths are presented for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on f…

astro-ph.GA2016★ 25 cited

Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap

Planck Collaboration, N. Aghanim, M. I. R. Alves +165

We study the statistical properties of interstellar dust polarization at high Galactic latitude, using the Stokes parameter Planck maps at 353 GHz. Our aim is to advance the unders…

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