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P. Sánchez-Blázquez

3 papers hereh-index 223 citations4 works total

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
same name
  • P. Sánchez-Blázquez — 35 papers, h 39
  • P. Sánchez-Blázquez — 19 papers, h 29
  • P. Sánchez-Blázquez — 10 papers, h 22
  • P. Sánchez-Blázquez — 8 papers, h 4

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

most citedStellar associations powering HII regions $\unicode{x2013}$ I. Defining an evolutionary sequence

25 citations · 25 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2026

Determining star formation histories and age-metallicity relations with convolutional neural networks

Enrique Galceran, Patricia Sánchez-Blázquez, Artemi Camps-Fariña +8

We aim to develop a state-of-the-art tool to infer detailed star formation histories (SFHs) and age-metallicity relations from realistic observational data, while mitigating classi…

astro-ph.GA2023

Probing the Star Formation Main Sequence down to 108 M⊙​ at 1.0<z<3.0

Rosa M. Mérida, Pablo G. Pérez-González, Patricia Sánchez-Blázquez +8

We investigate the star formation main sequence (MS) (SFR-M⋆​) down to 108−9M⊙​ using a sample of 34,061 newly-discovered ultra-faint ($27\lesssim i \less…

astro-ph.GA2023★ 25 cited

Stellar associations powering HII regions $\unicode{x2013}$ I. Defining an evolutionary sequence

Fabian Scheuermann, Kathryn Kreckel, Ashley T. Barnes +30

Connecting the gas in HII regions to the underlying source of the ionizing radiation can help us constrain the physical processes of stellar feedback and how HII regions evolve ove…

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