{"paper":{"title":"Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Abergel, A. Chrysostomou, A. M. Di Giorgio, A. Noriega-Crespo, A. Roy, A. Traficante, A. Zavagno, B. Ali, B. Schulz, B. Sibthorpe, B. Swinyard, C. Battersby, C. Brunt, C. C. Popescu, C. Joblin, C. Waelkens, D. Elia, D. Ikhenaode, D. J. Marshall, D. Paradis, D. Polychroni, D. Russeil, D. Stamatellos, D. Ward-Thompson, E. Schisano, E. Sturm, F. Boulanger, F. Faustini, F. Massi, F. Motte, F. Piacentini, F. Schuller, F. Strafella, F. Wyrowski, G. A. Fuller, G. De Gasperis, G. Joncas, G. Lagache, G. S. Stringfellow, G. Umana, G. White, H. A. Smith, H. Parsons, H. W. Yorke, I. Ristorcelli, J. A. Rod\\'on, J. Bally, J. Blommaert, J. Brand, J. Cernicharo, J. C. Mottram, J. F. Robitaille, J. Glenn, J. M. Kirk, J. Neves, J. P. Baluteau, J. P. Bernard, J. Z. Li, K. Ganga, L. A. Montier, L. Anderson, L. A. Wilcock, L. Calzoletti, L. Morgan, L. Olmi, L. Piazzo, L. Spinoglio, L. Testi, L. Valenziano, M. A. Miville-Deschenes, M. A. Thompson, M. Barlow, M. Benedettini, M. Burton, M. Cohen, M. Compiegne, M. D. Smith, M. Hoare, M. Huang, M. J. Griffin, M. Juvela, M. Marengo, M. Matsuura, M. Pestalozzi, M. Pomar\\`es, M. Sauvage, M. T. Beltr\\'an, M. Veneziani, N. Billot, N. Flagey, N. Peretto, N. Schneider, P. Andr\\'e, P. Caselli, P. De Bernardis, P. F. Goldsmith, P. Garcia-Lario, P. Martin, P. Natoli, P. Royer, P. Saraceno, P. Schilke, Q. Zhang, R. Cesaroni, R. J. Tuffs, R. Paladini, R. Plume, R. Taylor, R. Vavrek, S. Bontemps, S. Carey, S. Chakrabarti, S. D. Lord, S. Masi, S. Molinari, S. Pezzuto, S. Viti, T. G. Mueller, T. L. Lim, T. Moore, T. Robitaille, V. Minier, W. T. Reach, Y. Fukui","submitted_at":"2010-05-18T20:24:16Z","abstract_excerpt":"We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands. We outline our data reduction strategy and present some science highlights on the two observed 2{\\deg} x 2{\\deg} tiles approximately centered at l=30{\\deg} and l=59{\\deg}. The two regions are extremely rich in intense and highly structured extended emission which shows a widespread organization in filaments. Source SEDs can be built for hundreds of objects in the two fields, and physical parameters can be extracted"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.3317","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"}