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A. Frasca

4 papers hereh-index 213 citations5 works total

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

author position
  • middle author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.SR2
same name
  • A. Frasca — 86 papers, h 38
  • A. Frasca — 40 papers, h 23
  • A. Frasca — 13 papers
  • A. Frasca — 10 papers, h 4
  • A. Frasca — 8 papers, h 2
  • A. Frasca — 8 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
20152025
collaborators

4 papers

astro-ph.SR2025

The Gaia-ESO Survey: Projected Rotational Velocities of B stars in the Carina Nebula

W. Santos, S. Daflon, J. V. Sales Silva +19

The Carina Nebula is an active star-forming region with several open clusters rich in massive OB stars, thus making it an optimal target for studying stellar properties such as rot…

astro-ph.HE2023

Extreme photometric and polarimetric variability of blazar S4 0954+65 at its maximum optical and γ-ray brightness levels

C. M. Raiteri, M. Villata, M. I. Carnerero +64

In 2022 the BL Lac object S4 0954+65 underwent a major variability phase, reaching its historical maximum brightness in the optical and γ-ray bands. We present optical photometri…

astro-ph.HE2015

Discovery of a Highly Polarized Optical Microflare in the Blazar S5 0716+714 During 2014 WEBT Campaign

Gopal Bhatta, Arti Goyal, Michal Ostrowski +42

The occurrence of low-amplitude flux variations in blazars on hourly timescales, commonly known as microvariability, is still a widely debated subject in high-energy astrophysics.…

astro-ph.SR2015

The Gaia-ESO Survey: Catalogue of Hα emission stars

Gregor Traven, Tomaž Zwitter, Sophie Van Eck +18

We discuss the properties of Hα emission stars across the sample of 22035 spectra from the Gaia-ESO Survey internal data release, observed with the GIRAFFE instrument and largely…

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