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L. Aguilar

3 papers here

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.HE2
  • astro-ph.SR1
ORCID 0009-0000-9810-4702
same name
  • L. Aguilar — 17 papers, h 16
  • L. Aguilar — 6 papers, h 5
  • L. Aguilar — 6 papers, h 3
  • L. Aguilar — 3 papers, h 6
  • L. Aguilar — 2 papers, h 4
  • L. Aguilar — 2 papers, h 29

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 citedA magnetar powers the luminous supernova 2023pel, associated with a long gamma-ray burst

6 citations · 7 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025★ 1 cited

Hydrodynamical modeling of SN 2025kg associated with the Fast X-ray Transient EP250108a

L. M. Roman Aguilar, M. C. Bersten

Supernovae (SNe) associated with X-Ray Flashes (XRFs) are extremely rare. Therefore, the discovery of each new object in this class offers a unique opportunity to improve our under…

astro-ph.HE2025★ 6 cited

A magnetar powers the luminous supernova 2023pel, associated with a long gamma-ray burst

L. M. Roman Aguilar, M. M. Saez, K. Ertini +1

We explore SN 2023pel, the most recent event associated with gamma-ray bursts (GRBs), specifically GRB 230812B. SN 2023pel has a high luminosity and low expansion velocities compar…

astro-ph.SR2023

The progenitor of SN 2023ixf from hydrodynamical modelling

M. C. Bersten, M. Orellana, G. Folatelli +5

Context: Supernova (SN) 2023ixf is among the most nearby Type II SNe in the last decades. As such, there is a wealth of observational data of both the event itself and of the assoc…

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