{"title":"DeepTTV:根据凌日时间变化对隐藏系外行星进行深度学习预测","authors":"Chen Chen, Lingkai Kong, Gongjie Li, Molei Tao","doi":"arxiv-2409.04557","DOIUrl":null,"url":null,"abstract":"Transit timing variation (TTV) provides rich information about the mass and\norbital properties of exoplanets, which are often obtained by solving an\ninverse problem via Markov Chain Monte Carlo (MCMC). In this paper, we design a\nnew data-driven approach, which potentially can be applied to problems that are\nhard to traditional MCMC methods, such as the case with only one planet\ntransiting. Specifically, we use a deep learning approach to predict the\nparameters of non-transit companion for the single transit system with transit\ninformation (i.e., TTV, and Transit Duration Variation (TDV)) as input. Thanks\nto a newly constructed \\textit{Transformer}-based architecture that can extract\nlong-range interactions from TTV sequential data, this previously difficult\ntask can now be accomplished with high accuracy, with an overall fractional\nerror of $\\sim$2\\% on mass and eccentricity.","PeriodicalId":501163,"journal":{"name":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","volume":"181 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"DeepTTV: Deep Learning Prediction of Hidden Exoplanet From Transit Timing Variations\",\"authors\":\"Chen Chen, Lingkai Kong, Gongjie Li, Molei Tao\",\"doi\":\"arxiv-2409.04557\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Transit timing variation (TTV) provides rich information about the mass and\\norbital properties of exoplanets, which are often obtained by solving an\\ninverse problem via Markov Chain Monte Carlo (MCMC). In this paper, we design a\\nnew data-driven approach, which potentially can be applied to problems that are\\nhard to traditional MCMC methods, such as the case with only one planet\\ntransiting. Specifically, we use a deep learning approach to predict the\\nparameters of non-transit companion for the single transit system with transit\\ninformation (i.e., TTV, and Transit Duration Variation (TDV)) as input. Thanks\\nto a newly constructed \\\\textit{Transformer}-based architecture that can extract\\nlong-range interactions from TTV sequential data, this previously difficult\\ntask can now be accomplished with high accuracy, with an overall fractional\\nerror of $\\\\sim$2\\\\% on mass and eccentricity.\",\"PeriodicalId\":501163,\"journal\":{\"name\":\"arXiv - PHYS - Instrumentation and Methods for Astrophysics\",\"volume\":\"181 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-06\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Instrumentation and Methods for Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.04557\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.04557","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
DeepTTV: Deep Learning Prediction of Hidden Exoplanet From Transit Timing Variations
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.