{"paper":{"title":"HerMES: Candidate Gravitationally Lensed Galaxies and Lensing Statistics at Submillimeter Wavelengths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Boselli, A. Cabrera-Lavers, A. Cava, A. Conley, A. Franceschini, A. Hyde, A. I. Harris, A. J. Baker, A. J. Smith, A. Omont, A. Papageorgiou, Asantha Cooray, A. Streblyanska, A. Strom, B. O'Halloran, B. Schulz, C. Bridge, C. D. Dowell, C. Frazer, C. K. Xu, C. M. Casey, C. P. Pearson, D. Burgarella, D. Farrah, D. L. Clements, D. L. Shupe, D. Riechers, D. Rigopoulou, D. Scott, D. T. Frayer, E. A. Gonz\\'alez Solares, E. Chapin, E. Hatziminaoglou, E. Ibar, Francesco De Bernardis, G. Lagache, G. Marsden, Hai Fu, H. Aussel, H. T. Nguyen, I. G. Roseboom, I. P\\'erez-Fournon, J. Bock, J. Calanog, J. D. Vieira, J. Glenn, J. M. Carpenter, Julie L. Wardlow, L. Levenson, L. Marchetti, L. Wang, L. Yan, M. A. Gurwell, M. B\\'ethermin, M. Griffin, M. J. Page, M. Negrello, M. Pohlen, M. Rowan-Robinson, M. Symeonidis, M. Trichas, M. Vaccari, M. Viero, M. Zemcov, N. Castro-Rodr\\'iguez, N. Scoville, N. Seymour, P. Chanial, P. Cox, P. Ferrero, P. Martinez-Navajas, P. Panuzzo, R. Blundell, R. Gavazzi, R. Hopwood, R. J. Ivison, R. Neri, R. S. Bussmann, S. C. Chapman, S. Dye, S. Eales, S. J. Oliver, S. Kim, V. Arumugam, V. Buat","submitted_at":"2012-05-16T20:00:00Z","abstract_excerpt":"We present a list of 13 candidate gravitationally lensed submillimeter galaxies (SMGs) from 95 square degrees of the Herschel Multi-tiered Extragalactic Survey, a surface density of 0.14\\pm0.04deg^{-2}. The selected sources have 500um flux densities (S_500) greater than 100mJy. Gravitational lensing is confirmed by follow-up observations in 9 of the 13 systems (70%), and the lensing status of the four remaining sources is undetermined. We also present a supplementary sample of 29 (0.31\\pm0.06deg^{-2}) gravitationally lensed SMG candidates with S_500=80--100mJy, which are expected to contain a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.3778","kind":"arxiv","version":2},"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"}