{"paper":{"title":"AKARI mid-infrared slitless spectroscopic survey of star-forming galaxies at $z\\lesssim 0.5$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(10) RAL Space, 11, 11), (11) Department of Physics, 12), (12) Oxford Astrophysics, (13) National Optical Astronomy Observatory, 14), (14) CRAL, (15) Graduate School of Science, (16) Graduate School of Science, 17), (17) Center for Planetary Science, (18) Laboratoire d'Astrophysique de Marseille, (19) National Astronomical Observatory of Japan, (20) Korea Astronomy, (21) Instituto de Astronom\\'ia Campus Ensenada, (22) Physics Section, 23), (23) Department of Astronomy, (2) Institute of Space, 3), (3) Japan Space Forum, (4) Division of Astronomy, (5) Dark Cosmology Centre, 6), (6) National Tsing Hua University, (7) Steward Observatory, (8) Astronomy Program, 9), (9) Subaru Telescope, Astronautical Science, Astronomy, Astrophysics, C. Pearson (10, D. Burgarella (18), Denys Wilkinson Building, Department of Physics, E. Egami (7), Faculty of Humanities, F. Mazyed (18), F. Usui (16, G. J. White (10, Graduate School of Science, H. Hanami (22), H. Inami (13, H. Matsuhara (2), H. M. Lee (8), Institute of Astronomy, Iwate University, Japan Aerospace Exploration Agency, J. D\\'iaz Tello (21), J.-H. Kim (8, Kobe University, Kyoto University), M. Im (8), M. Imanishi (19), M. Malkan (4), Nagoya University, National Astronomical Observatory of Japan, Niels Bohr Institute, Observatoire de Lyon, Seoul National University, Social Sciences, S. Oyabu (15), Space Science Institute, S. Serjeant (11), STFC Rutherford Appleton Laboratory, T. Goto (5, The Open University, The University of Tokyo, T. Ishigaki (22) ((1) Academia Sinica, T. Miyaji (21), T. Nakagawa (2), T. Takagi (2, T. T. Takeuchi (15), T. Wada (2), Universidad Nacional Aut\\'onoma de M\\'exico, University of Arizona, University of California, University of Copenhagen, University of Oxford, W.-S. Jeong (20), Y. Ohyama (1), Y. Toba (1","submitted_at":"2018-08-14T07:39:43Z","abstract_excerpt":"Deep MIR surveys have revealed numerous strongly star-forming galaxies at redshift z~<2. Their MIR fluxes are produced by a combination of continuum and PAH emission features. The PAH features can dominate the total MIR flux, but are difficult to measure without spectroscopy. We aim to study star-forming galaxies by using a blind spectroscopic survey at MIR wavelengths to understand evolution of their star formation rate (SFR) and specific SFR up to z~=0.5, by paying particular attention to their PAH properties. We conducted a low-resolution (R~=50) slitless spectroscopic survey at 5-13um of 9"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.04566","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"}