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翻訳待ち:High-Resolution Imaging for Statistical Validation of TESS Planet Candidates

AI サービスが一時的に利用できないため、復旧後に翻訳を補完します。ソース概要:--> [Submitted on 21 Aug 2026] Title:Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates View a PDF of the paper titled Assessing the Impact of High-Resolution Imaging on…

ソースHacker News AI著者: mikecollier

AI サービスが一時的に利用できないため、復旧後に翻訳を補完します。

--> [Submitted on 21 Aug 2026] Title:Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates View a PDF of the paper titled Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates, by Michael Collier and 40 other authors View PDF HTML (experimental) Abstract:High-resolution imaging is widely used to constrain false-positive scenarios in exoplanet validation, but it is a finite follow-up resource that reaches only a subset of candidates, and its population-level impact on validation outcomes has not been quantified through controlled removal experiments. Using an automated pipeline built on TRICERATOPS, we compute the false-positive probability (FPP) of 443 TESS planet candidates. For the 264 planet candidates with high-resolution imaging observations, we compute FPP with and without the corresponding contrast curves, allowing us to quantify the impact of the additional data. We find that 72% of 68 contrast-curve bearing validated planets would fail validation without their adopted contrast curves. The fraction requiring imaging decreases with increasing planet size, from 100% below $1.7~R_\oplus$ to $33\%$ above $4~R_\oplus$: within our sample and TRICERATOPS-based analysis, the availability of high-resolution imaging directly limits the yield of small-planet validation and the supply of validated targets for atmospheric characterization. Our analysis statistically validates 64 new TESS planets with sizes spanning 0.94 to 7.83 $R_\oplus$ across hosts of spectral type M through F. Four of these are highly amenable to JWST observations based on the transmission and emission spectroscopy metrics, and each achieves validation only with its imaging constraint. Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM) Cite as: arXiv:2608.21560 [astro-ph.EP] (or arXiv:2608.21560v1 [astro-ph.EP] for this version) https://doi.org/10.48550/arXiv.2608.21560 arXiv-issued DOI via DataCite (pending registration) Submission history From: Steven Giacalone [view email] [v1] Fri, 21 Aug 2026 18:51:06 UTC (570 KB) Full-text links: Access Paper: View a PDF of the paper titled Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates, by Michael Collier and 40 other authors View PDF HTML (experimental) TeX Source view license Current browse context: astro-ph.EP new | recent | 2026-08 Change to browse by: astro-ph astro-ph.IM References & Citations NASA ADS Google Scholar Semantic Scholar Loading... Data provided by: Bibliographic Tools Bibliographic and Citation Tools Bibliographic Explorer Toggle Bibliographic Explorer (What is the Explorer?) Connected Papers Toggle Connected Papers (What is Connected Papers?) Litmaps Toggle Litmaps (What is Litmaps?) scite.ai Toggle scite Smart Citations (What are Smart Citations?) Code, Data, Media Code, Data and Media Associated with this Article alphaXiv Toggle alphaXiv (What is alphaXiv?) Links to Code Toggle CatalyzeX Code Finder for Papers (What is CatalyzeX?) DagsHub Toggle DagsHub (What is DagsHub?) GotitPub Toggle Gotit.pub (What is GotitPub?) Huggingface Toggle Hugging Face (What is Huggingface?) ScienceCast Toggle ScienceCast (What is ScienceCast?) Demos Demos Replicate Toggle Replicate (What is Replicate?) Spaces Toggle Hugging Face Spaces (What is Spaces?) Spaces Toggle TXYZ.AI (What is TXYZ.AI?) Related Papers Recommenders and Search Tools Link to Influence Flower Influence Flower (What are Influence Flowers?) Core recommender toggle CORE Recommender (What is CORE?) IArxiv recommender toggle IArxiv Recommender (What is IArxiv?) Author Venue Institution Topic About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs. Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)