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C. Palomba

4 papers hereh-index 114 citations3 works total

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • gr-qc3
  • astro-ph.IM1
same name
  • C. Palomba — 81 papers, h 97
  • C. Palomba — 74 papers
  • C. Palomba — 5 papers
  • C. Palomba — 2 papers
  • C. Palomba — 2 papers
  • C. Palomba — 2 papers

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

collaborators

4 papers

gr-qc2026

A semicoherent resampling method for long-transient gravitational wave searches with applications to subsolar-mass primordial black-hole binaries

Neil Lu, Cristiano Palomba, Ornella J. Piccinni +1

Resampling removes the modeled phase evolution of a frequency-evolving signal, transforming it into a monochromatic one. We introduce a novel implementation for long-transient grav…

astro-ph.IM2026

Search for Long-Transient Gravitational Waves from Supernova SN2023ixf using GFH-v2 Pipeline

Sandhya Sajith Menon, Lorenzo Pierini, Pia Astone +24

We present a directed search for long-transient gravitational waves from the possible newborn magnetar remnant of SN2023ixf, a nearby Type II core-collapse supernova in the M101 ga…

gr-qc2026

Alternative neural-network follow-up for all-sky FrequencyHough in continuous gravitational-wave searches

Martina Di Cesare, Pia Astone, Rosario De Rosa +3

Continuous gravitational waves are long-lived signals emitted by spinning neutron stars (NSs) or boson clouds around black holes. While the Milky Way is expected to host $\mathrm{O…

gr-qc2023

A semi-coherent generalization of the 5-vector method to search for continuous gravitational waves

S. D'Antonio, C. Palomba, P. Astone +8

The emission of continuous gravitational waves (CWs), with duration much longer than the typical data taking runs, is expected from several sources, notably spinning neutron stars,…

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