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researcher

J. González-López

8 papers hereh-index 441 citations9 works total

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

author position
  • middle author7

Across the 7 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA8
same name
  • J. González-López — 60 papers, h 13
  • J. González-López — 12 papers, h 15
  • J. González-López — 2 papers, h 7
  • J. González-López — 1 paper, h 7
  • J. González-López — 1 paper, h 3
  • J. González-López — 1 paper, h 56

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
20202025
most citedThe ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies

26 citations · 72 across the 8 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.GA2025★ 26 cited

The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies

R. Herrera-Camus, J. González-López, N. Förster Schreiber +44

We present the ALMA-CRISTAL survey, an ALMA Cycle 8 Large Program designed to investigate the physical properties of star-forming galaxies at 4≲z≲6 through spat…

astro-ph.GA2025

The ALMA-CRISTAL survey: weak evidence for star-formation driven outflows in z∼5 main-sequence galaxies

Jack E. Birkin, Justin S. Spilker, Rodrigo Herrera-Camus +23

There is a broad consensus from theory that stellar feedback in galaxies at high redshifts is essential to their evolution, alongside conflicting evidence in the observational lite…

astro-ph.GA2025★ 9 cited

Spatially resolved dust properties over 50 kpc in a hyperluminous galaxy merger at z=4.6

Román Fernández Aranda, Tanio Díaz Santos, Evanthia Hatziminaoglou +19

We present spatially resolved dust-continuum ALMA observations from rest-frame ∼60 to ∼600 μm (bands 3-10) of the hyperluminous hot dust-obscured galaxy (hot DOG) WISE…

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