{"paper":{"title":"The MUSCLES Treasury Survey III: X-ray to Infrared Spectra of 11 M and K Stars Hosting Planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Alexander Brown, Allison Youngblood, Christian Schneider, Cynthia S. Froning, Feng Tian, Jeffrey Linsky, Kevin France, Renyu Hu, R. O. Parke Loyd, Sarah Rugheimer, Seth Redfield","submitted_at":"2016-04-16T17:34:28Z","abstract_excerpt":"We present a catalog of panchromatic spectral energy distributions (SEDs) for 7 M and 4 K dwarf stars that span X-ray to infrared wavelengths (5 {\\AA} - 5.5 {\\mu}m). These SEDs are composites of Chandra or XMM-Newton data from 5 - ~50 {\\AA}, a plasma emission model from ~50 - 100 {\\AA}, broadband empirical estimates from 100 - 1170 {\\AA}, HST data from 1170 - 5700 {\\AA}, including a reconstruction of stellar Ly{\\alpha} emission at 1215.67 {\\AA}, and a PHOENIX model spectrum from 5700 - 55000 {\\AA}. Using these SEDs, we computed the photodissociation rates of several molecules prevalent in plan"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.04776","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"}