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M. L. Planas

4 papers hereh-index 252.7k citations74 works total

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

author position
  • first author3
  • last author1

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

fields
  • gr-qc3
  • astro-ph.HE1
same name
  • M. L. Planas — 5 papers
  • M. L. Planas — 2 papers
  • M. L. Planas — 1 paper
  • M. L. Planas — 1 paper
  • M. L. Planas — 1 paper
  • M. L. Planas — 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

collaborators

4 papers

gr-qc2025

Hybrid waveforms for precessing quasi-circular binary systems

Joan Llobera-Querol, Sascha Husa, Maria de Lluc Planas

The demand for long and accurate gravitational waveforms is increasing as we prepare for the next generation of detectors and seek to improve current waveform models. However, nume…

astro-ph.HE2025

First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers

Maria de Lluc Planas, Sascha Husa, Antoni Ramos-Buades +1

The gravitational wave event GW200105 was the first confident neutron star-black hole (NSBH) merger identified by the LIGO-Virgo-KAGRA collaboration. A recent analysis by Morras et…

gr-qc2025

Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures

Maria de Lluc Planas, Antoni Ramos-Buades, Cecilio García-Quirós +3

We present a reanalysis of 17 gravitational-wave events detected with Advanced LIGO and Advanced Virgo in their first three observing runs, using the new IMRPhenomTEHM model -- a p…

gr-qc2025

Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits

Maria de Lluc Planas, Antoni Ramos-Buades, Cecilio García-Quirós +3

We introduce IMRPhenomTEHM, a new phenomenological time-domain model for eccentric aligned-spin binary black holes. Building upon the accurate quasi-circular IMRPhenomTHM model, IM…

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