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researcher

F. Santos

33 papers hereh-index 211.3k citations51 works total

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

author position
  • first author6
  • middle author26

Across the 32 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA24
  • astro-ph.IM5
  • astro-ph.SR4
same name
  • F. Santos — 73 papers, h 29
  • F. Santos — 69 papers, h 34
  • F. Santos — 10 papers, h 20
  • F. Santos — 10 papers, h 8
  • F. Santos — 5 papers, h 4
  • F. Santos — 4 papers, h 2

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
20102026
most citedBalloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle Dispersion

114 citations · 1.3k across the 33 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.GA2016★ 40 cited

Magnetically Dominated Parallel Interstellar Filaments at the Infrared Dark Cloud G14.225-0.506

Fabio P. Santos, Gemma Busquet, Gabriel A. P. Franco +2

The G14.225-0.506 infrared dark cloud (IRDC G14.2) displays a remarkable complex of parallel dense molecular filaments projected on the plane of the sky. Previous dust emission and…

astro-ph.IM2016★ 18 cited

Instrumental performance and results from testing of the BLAST-TNG receiver, submillimeter optics, and MKID arrays

Nicholas Galitzki, Peter Ade, Francesco E. Angile +39

Polarized thermal emission from interstellar dust grains can be used to map magnetic fields in star forming molecular clouds and the diffuse interstellar medium (ISM). The Balloon-…

astro-ph.GA2016★ 18 cited

Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud

Fabio P. Santos, Peter A. R. Ade, Francesco E. Angile +27

We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight with polarized emission data at submillimeter (sub-mm) wave…

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