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researcher

P. García

6 papers hereh-index 4196 citations7 works total

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

author position
  • first author2
  • middle author3

Across the 5 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA5
  • astro-ph.CO1
same name
  • P. García — 13 papers, h 19
  • P. García — 11 papers, h 14
  • P. García — 6 papers, h 2
  • P. García — 4 papers, h 7
  • P. García — 3 papers
  • P. García — 3 papers, h 5

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
20162026
most citedCCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

101 citations · 141 across the 6 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.CO2021★ 101 cited

CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

Prime collaboration, M. Aravena, J. E. Austermann +84

We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for ded…

astro-ph.GA2021★ 6 cited

Warm ISM in the Sgr A Complex. II. The [C/N] abundance ratio traced by [CII] 158 um and [NII] 205 um observations toward the Arched Filaments at the Galactic center

P. García, N. Abel, M. Röllig +2

Aims. We aim to investigate the I([CII]) versus I([NII]) integrated intensity behavior in the AF region in order to assess the [CII] emission contribution from the H II region, whi…

astro-ph.GA2021★ 24 cited

GASTON: Galactic Star Formation with NIKA2. Evidence for the mass growth of star-forming clumps

A. J. Rigby, N. Peretto, R. Adam +44

Determining the mechanism by which high-mass stars are formed is essential for our understanding of the energy budget and chemical evolution of galaxies. By using the New IRAM KIDs…

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