{"paper":{"title":"The Impact of Non-Uniform Thermal Structure on the Interpretation of Exoplanet Emission Spectra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Jacob Bean, Jonathan J. Fortney, Kevin B. Stevenson, Laura Kreidberg, Michael R. Line, Vivien Parmentier, Y. Katherina Feng","submitted_at":"2016-07-12T04:20:42Z","abstract_excerpt":"The determination of atmospheric structure and molecular abundances of planetary atmospheres via spectroscopy involves direct comparisons between models and data. While varying in sophistication, most model-spectra comparisons fundamentally assume \"1D\" model physics. However, knowledge from general circulation models and of solar system planets suggests that planetary atmospheres are inherently \"3D\" in their structure and composition. We explore the potential biases resulting from standard \"1D\" assumptions within a Bayesian atmospheric retrieval framework. Specifically, we show how the assumpt"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.03230","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}