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G. Ricigliano

4 papers hereh-index 6111 citations11 works total

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

author position
  • first author1
  • middle author3

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

fields
  • astro-ph.HE4

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.HE2026

JWST observations of SN 2024abup: First Detection of CO in a broad-lined Type Ic Supernova and Constraints on r-process Nucleosynthesis

Manisha Shrestha, Lindsey A. Kwok, David J. Sand +42

SN 2024abup is a nearby broad-lined Type Ic supernova (SN Ic-bl) in NGC 0681 at a distance of 23.3 \pm 1.6 Mpc. As energetic explosions of massive stars, SNe Ic-bl are considered a…

astro-ph.HE2026

Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories

E. Loffredo, N. Hazra, U. Dupletsa +13

Next-generation gravitational wave (GW) observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, will observe binary neutron star (BNS) mergers across cosmic history…

astro-ph.HE2025

56Ni production in long-lived binary neutron star merger remnants

Maximilian Jacobi, Fabio Magistrelli, Eleonora Loffredo +5

We investigate the nucleosynthesis and kilonova emission based on numerical-relativity binary neutron star merger simulations that incorporate a two-moment neutrino-transport schem…

astro-ph.HE2025

Modeling the emission lines from r-process elements in Supernova nebulae

Giacomo Ricigliano, Kenta Hotokezaka, Almudena Arcones

The origin of heavy r-process elements in the universe is still a matter of great debate, with a confirmed scenario being neutron star (NS) mergers. Additional relevant sites could…

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