Pith. sign in

REVIEW 6 cited by

Narrowing RIFT: Focused simulation-based-inference for interpreting exceptional GW sources

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2505.11655 v1 pith:2F67VGJ3 submitted 2025-05-16 astro-ph.IM gr-qc

Narrowing RIFT: Focused simulation-based-inference for interpreting exceptional GW sources

classification astro-ph.IM gr-qc
keywords inferenceriftalgorithmefficientlyeventsexceptionalparametersources
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The Rapid Iterative FiTting (RIFT) parameter inference algorithm provides a simulation-based inference approach to efficient, highly-parallelized parameter inference for GW sources. Previous editions of RIFT have conservatively optimized for robust inference about poorly constrained observations. In this paper, we summarize algorithm enhancements and operating point choices to enable inference for more exceptional compact binaries. Using the previously-reported RIFT/asimov interface to efficiently perform analyses on events with reproducible settings consistent with past work, we demonstrate that the latest version of RIFT can efficiently analyze events with multiple costly models including the effects of precession or eccentricity.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Population Properties of Binary Black Holes with Eccentricity

    astro-ph.HE 2026-02 conditional novelty 8.0

    First joint population inference on binary black hole eccentricity from GWTC-4 bounds the eccentric branching ratio below 5% at 90% confidence, with results consistent with quasi-circular models but highly model-dependent.

  2. Assessing the imprint of eccentricity in GW signatures using two independent waveform models

    astro-ph.HE 2026-05 conditional novelty 5.0

    Dual-model analysis of 162 GW sources disfavors eccentricity for most events but finds potential evidence in GW200129, GW231001, and GW231123.

  3. Measuring Eccentricity and Addressing Waveform Systematics in GW231123

    gr-qc 2025-12 conditional novelty 5.0

    Reanalysis of GW231123 shows no significant eccentricity, with parameter estimate differences explained by waveform model disagreements at strong spin precession.

  4. Kilonovae and Long-duration Gamma-ray Bursts

    astro-ph.HE 2025-09 unverdicted novelty 5.0

    Kilonova-like emissions after long GRBs GRB211211A and GRB230307A are consistent with collapsar nucleosynthesis using a single weak r-process component without lanthanide-rich material.

  5. Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620

    gr-qc 2025-07 unverdicted novelty 5.0

    Bayesian parameter estimation with targeted eccentric numerical-relativity waveforms yields eccentricity estimates of e20 ≈ 0.2 for GW200208_22 and e10 ≈ 0.19 for GW190620, reinforcing the eccentric hypothesis.

  6. Gravitational Wave Hyperbolic Catalog: Reanalyzing High-Mass Gravitational Wave Signals Using Hyperbolic Waveforms

    gr-qc 2026-05 unverdicted novelty 4.0

    Reanalysis finds GW190521 prefers hyperbolic waveforms over quasi-circular precessing ones with ln Bayes factor 3.71, while other high-mass events and GW231123 favor the latter; mock signals indicate distinguishabilit...