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M. Pérez-Torres

12 papers hereh-index 581 citations10 works total

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

author position
  • middle author11

Across the 11 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE7
  • astro-ph.GA3
  • astro-ph.EP1
  • astro-ph.SR1
same name
  • M. Pérez-Torres — 155 papers, h 51
  • M. Pérez-Torres — 19 papers, h 12
  • M. Pérez-Torres — 14 papers, h 1
  • M. Pérez-Torres — 8 papers, h 5
  • M. Pérez-Torres — 5 papers, h 3
  • M. Pérez-Torres — 3 papers, h 0

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
20172026
most citedThe Close AGN Reference Survey (CARS): Comparative analysis of the structural properties of star-forming and non-star-forming galaxy bars

31 citations · 129 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2024★ 2 cited

A multi-frequency, multi-epoch radio continuum study of the Arches cluster with the VLA

M. Cano-González, R. Schödel, A. Alberdi +4

The Arches cluster, one of the most massive clusters in the Milky Way, is located about 30 pc in projection from the central massive black hole. With its high mass, young age, and…

astro-ph.GA2023★ 2 cited

Supernova environments in J-PLUS. Normalized Cumulative Rank distributions and stellar population synthesis, combining narrow- and broad-band filters

Raul González-Díaz, Lluís Galbany, Tuomas Kangas +26

We study the local environmental properties of 418 supernovae (SNe) of all types using data from the Javalambre Photometric Local Universe Survey (J-PLUS), which includes 5 broad-…

astro-ph.GA2019★ 31 cited

The Close AGN Reference Survey (CARS): Comparative analysis of the structural properties of star-forming and non-star-forming galaxy bars

Justus Neumann, Dimitri A. Gadotti, Lutz Wisotzki +12

The absence of star formation in the bar region that has been reported for some galaxies can theoretically be explained by shear. However, it is not clear how star-forming (SF) bar…

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