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researcher

G. Pignata

3 papers here

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

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.SR1
same name
  • G. Pignata — 63 papers, h 35
  • G. Pignata — 31 papers, h 35
  • G. Pignata — 24 papers
  • G. Pignata — 18 papers, h 35
  • G. Pignata — 3 papers, h 6
  • G. Pignata — 1 paper, h 2

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
20202025
most citedSN 2018is: a low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases

15 citations · 15 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025★ 15 cited

SN 2018is: a low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases

R. Dastidar, K. Misra, S. Valenti +31

We present a comprehensive photometric and spectroscopic study of the Type IIP SN 2018is. The V-band luminosity and the expansion velocity at 50 days post-explosion are −15.1$\…

astro-ph.HE2024

SN 2023tsz: A helium-interaction driven supernova in a very low-mass galaxy

B. Warwick, J. Lyman, M. Pursiainen +49

SN 2023tsz is a Type Ibn supernova (SNe Ibn) discovered in an extremely low-mass host. SNe Ibn are an uncommon subtype of stripped-envelope core-collapse SNe. They are characterise…

astro-ph.SR2020

Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv

K. Ackley, L. Amati, C. Barbieri +151

On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. Preliminary analysis of the GW data suggests that the event was likely…

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