{"paper":{"title":"Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ($-71.0^{\\circ}< \\ell < 67.0^{\\circ}$)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Baldeschi, A. Costa, A. Di Giorgio, A. Hajnal, A. Mercurio, A. Noriega-Crespo, A. P. Whitworth, A. Traficante, A. Zavagno, B. M. T. Maiolo, C. Buemi, C. Trigilio, D. Elia, D. J. Eden, D. Polychroni, D. Russeil, D. Ward-Thompson, E. Fiorellino, E. Schisano, E. Sciacca, F. Bufano, F. Faustini, F. Motte, F. Piacentini, F. Strafella, F. Vitello, F. Wyrowski, G. Joncas, G. Li Causi, G. L. Pilbratt, G. Riccio, G. Umana, H. Arab, H. Sano, H. Yamamoto, J. Bally, J. C. Mottram, J. P. Bernard, K. A. Marsh, K. L. J. Rygl, K. Tachihara, K. Torii, L. Calzoletti, L. Cambr\\'esy, L. Olmi, L. Piazzo, L. Testi, M. A. Thompson, M. Bandieramonte, M. Benedettini, M. Brescia, M. G. Hoare, M. Huang, M. Merello, M. Molinaro, M. Pestalozzi, M. T. Beltr\\'an, M. Veneziani, N. Billot, N. Marchili, N. Peretto, N. Schneider, P. Garc\\'ia-Lario, P. G. Martin, P. Kacsuk, P. Leto, P. M\\`ege, P. Natoli, P. Palmerim, P. Schilke, R. Butora, R. Cesaroni, R. Paladini, R. Plume, S. Cavuoti, S. E. Jaffa, S. E. Ragan, S. J. Liu, S. Martinavarro-Armengol, S. Molinari, S. Pezzuto, T. Hayakawa, T. J. T. Moore, U. Becciani, Y. Fukui, Y. Maruccia","submitted_at":"2017-06-04T09:29:57Z","abstract_excerpt":"Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $\\mu$m. We present a band-merged catalogue of spatially matched sources and their properties derived from fits to the spectral energy distributions (SEDs) and heliocentric distances, based on the photometric catalogs presented in Molinari et al. (2016a), covering the portion of Galactic plane $-71.0^{\\circ}< \\ell < 67.0^{\\circ}$. The band-merged catalogue contains 100922 sources with a regular SED, 24584 of which show a 70 $\\mu$m counterpart and are thus considered "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.01046","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"}