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P. Pérez-González

87 papers hereh-index 293.3k citations94 works total

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

author position
  • first author3
  • middle author68
  • last author1

Across the 72 of 87 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA75
  • astro-ph.CO9
  • astro-ph1
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • P. Pérez-González — 213 papers, h 71
  • P. Pérez-González — 27 papers, h 5
  • P. Pérez-González — 18 papers, h 12
  • P. Pérez-González — 18 papers, h 7
  • P. Pérez-González — 11 papers, h 3

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 citedA CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars

365 citations · 4k across the 86 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.GA2019

Rest-frame FUV-to-FIR view of Lyman break galaxies at z∼3: Templates and dust attenuation

J. Álvarez-Márquez, D. Burgarella, V. Buat +2

This work explores from a statistical point of view the rest-frame Far-ultraviolet (FUV) to Far-infrared (FIR) emission of a population of Lyman break galaxies (LBGs) at z∼3 t…

astro-ph.GA2019★ 11 cited

A deeper look at the dust attenuation law of star-forming galaxies at high redshift

M. Tress, I. Ferreras, P. G. Pérez-González +4

A diverse range of dust attenuation laws is found in star-forming galaxies. In particular, Tress et al. (2018) studied the SHARDS survey to constrain the NUV bump strength (B) and…

astro-ph.GA2019★ 81 cited

ALMA 200-parsec Resolution Imaging of Smooth Cold Dusty Disks in Typical z∼3 Star-Forming Galaxies

W. Rujopakarn, E. Daddi, G. H. Rieke +14

We present high-fidelity, 30 milliarcsecond (200-pc) resolution ALMA rest-frame 240 μm observations of cold dust emission in three typical main-sequence star-forming galaxies (SF…

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