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researcher

R. Poggiani

36 papers hereh-index 9555k citations555 works total

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

author position
  • sole author3
  • middle author16

Across the 19 of 36 papers where every author was matched, so the position is known.

fields
  • gr-qc24
  • astro-ph.SR4
  • astro-ph.HE3
  • astro-ph.CO2
  • hep-ex2
  • astro-ph.IM1
same name
  • R. Poggiani — 77 papers
  • R. Poggiani — 5 papers
  • R. Poggiani — 2 papers
  • R. Poggiani — 2 papers
  • R. Poggiani — 1 paper
  • R. Poggiani — 1 paper

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
20012026
most citedAdvanced Virgo: a 2nd generation interferometric gravitational wave detector

4.2k citations · 7.3k across the 34 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2025★ 11 cited

Limits on the Ejecta Mass During the Search for Kilonovae Associated with Neutron Star-Black Hole Mergers: A case study of S230518h, GW230529, S230627c and the Low-Significance Candidate S240422ed

M. Pillas, S. Antier, K. Ackley +78

Neutron star-black hole (NSBH) mergers, detectable via their gravitational-wave (GW) emission, are expected to produce kilonovae (KNe). Four NSBH candidates have been identified an…

astro-ph.HE2020★ 27 cited

Chandra High Energy Transmission Gratings Spectra of V3890 Sgr

Marina Orio, Jeremy J. Drake, Jan-Uwe Ness +13

The recurrent nova (RN) V3890 Sgr was observed during the 7th day after the onset of its most recent outburst, with the Chandra ACIS-S camera and High Energy Transmission Gratings…

astro-ph.HE2019★ 149 cited

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1130

We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis,…

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