Pith. sign in

REVIEW 2 cited by

DeepTTV: Deep Learning Prediction of Hidden Exoplanet From Transit Timing Variations

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 2409.04557 v1 pith:TFUMEN2K submitted 2024-09-06 astro-ph.EP astro-ph.IMcs.LG

classification astro-ph.EPastro-ph.IMcs.LG
keywords transitapproachdeepinformationlearningmassmcmctiming
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
abstract

Transit timing variation (TTV) provides rich information about the mass and orbital properties of exoplanets, which are often obtained by solving an inverse problem via Markov Chain Monte Carlo (MCMC). In this paper, we design a new data-driven approach, which potentially can be applied to problems that are hard to traditional MCMC methods, such as the case with only one planet transiting. Specifically, we use a deep learning approach to predict the parameters of non-transit companion for the single transit system with transit information (i.e., TTV, and Transit Duration Variation (TDV)) as input. Thanks to a newly constructed \textit{Transformer}-based architecture that can extract long-range interactions from TTV sequential data, this previously difficult task can now be accomplished with high accuracy, with an overall fractional error of $\sim$2\% on mass and eccentricity.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

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

  1. Estimating Orbital Parameters of Direct Imaging Exoplanet Using Neural Network

    astro-ph.EP 2025-10 conditional novelty 4.0 of 10

    Warm-starting parallel-tempered MCMC with flow-matching posterior proposals infers β Pictoris b's orbit about 78-365× faster than conventional samplers with comparable posteriors, though the comparison is not fully ap...

  2. Three-Dimensional Orbital Architectures and Detectability of Adjacent Companions to Hot Jupiters

    astro-ph.EP 2025-05 conditional novelty 4.0 of 10

    Stellar spin-down can knock outer companions to hot Jupiters out of the transiting plane, biasing transit surveys against them, while inner companions remain detectable.

Pith tools