{"paper":{"title":"Discovery of a Multiply-Lensed Submillimeter Galaxy in Early HerMES Herschel/SPIRE Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Beelen, A. Blain, A. Conley, A. Cooray, A. Franceschini, A.J. Baker, A.J. Smith, A. Mahabal, A.M.J. Mortier, A. Omont, A. Papageorgiou, A. Verma, B.J. Naylor, B. Schulz, C. Bridge, C.D. Dowell, C.K. Xu, C. Maraston, C.M. Bradford, C.P. Pearson, D. Brisbin, D. Burgarella, D. Farrah, D. Frayer, D.L. Clements, D.L. Shupe, Douglas Scott, D. Riechers, D. Wiebe, E.A. Gonz\\'alez Solares, E. Chapin, E. Ibar, E. Murphy, E. Valiante, G. Marsden, G. Raymond, G. Rodighiero, G. Wright, G. Zeimann, H. Fu, H. Matsuhara, H.T. Nguyen, I.G. Roseboom, I. P\\'erez-Fournon, I. Valtchanov, J. Bock, J.D. Vieira, J.E. Aguirre, J. Glenn, J.I. Rawlings, J. Kamenetzky, J.M. Carpenter, J. Zmuidzinas, K.E. Tugwell, K. Scott, L. Earle, L. Levenson, L. Marchetti, L. Vigroux, L. Wang, M.A. Gurwell, M. Griffin, M. Halpern, M. Jarvis, M.J. Page, M. Krips, M. Pohlen, M.P. Viero, M. Rowan-Robinson, M. Symeonidis, M. Vaccari, M. Zemcov, N. Christopher, N. Rangwala, N. Seymour, P. Chanial, P. Cox, P.D. Maloney, P. Serra, R. Auld, R. Blundell, R. Gavazzi, R.J. Ivison, R. Lupu, R. Neri, S. Eales, S.G. Djorgovski, S.J. Oliver, S. Kim, T.P. Ellsworth-Bowers","submitted_at":"2011-04-20T20:00:01Z","abstract_excerpt":"We report the discovery of a bright ($f(250\\mum) > 400$ mJy), multiply-lensed submillimeter galaxy \\obj\\ in {\\it\n  Herschel}/SPIRE Science Demonstration Phase data from the HerMES project. Interferometric 880\\mum\\ Submillimeter Array observations resolve at least four images with a large separation of $\\sim 9\\arcsec$. A high-resolution adaptive optics $K_p$ image with Keck/NIRC2 clearly shows strong lensing arcs. Follow-up spectroscopy gives a redshift of $z=2.9575$, and the lensing model gives a total magnification of $\\mu \\sim 11 \\pm 1$. The large image separation allows us to study the mult"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.4113","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"}