{"paper":{"title":"The first Hi-GAL observations of the outer Galaxy: a look to star formation in the third Galactic quadrant in the longitude range 216.5 < l < 225.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. M. Di Giorgio, A. Mizuno, D. Elia, D. Ikhenaode, D. Polychroni, E. Schisano, H. Yamamoto, K. L. J. Rygl, L. Olmi, L. Piazzo, M. Benedettini, M. Pestalozzi, M. Veneziani, N. Schneider, S. Molinari, S. Pezzuto, T. Hayakawa, T. Onishi, Y. Fukui, Y. Maruccia","submitted_at":"2013-04-27T11:32:01Z","abstract_excerpt":"We present the first Herschel PACS and SPIRE photometric observations in a portion of the outer Galaxy ($216.5^{\\circ} \\lesssim \\ell \\lesssim 225.5^{\\circ}$ and $-2^{\\circ} \\lesssim b \\lesssim 0^{\\circ}$) as a part of the Hi-GAL survey. The maps between 70 and 500 $\\mu$m, the derived column density and temperature maps, and the compact source catalog are presented. NANTEN CO(1-0) line observations are used to derive cloud kinematics and distances, so that we can estimate distance-dependent physical parameters of the compact sources (cores and clumps) having a reliable spectral energy distribut"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.7358","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"}