EBEX, THE E AND B EXPERIMENT

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dc.contributor.authorDIDIER, JOY
dc.contributor.authorABOOBAKER, ASAD M.
dc.contributor.authorADE, PETER
dc.contributor.authorAUBIN, FRANQOIS
dc.contributor.authorBACCIGALUPI, CARLO
dc.contributor.authorHelson, Kyle
dc.contributor.authoret al
dc.date.accessioned2022-06-24T20:20:41Z
dc.date.available2022-06-24T20:20:41Z
dc.date.issued2014
dc.descriptionProceedings, 49th Rencontres de Moriond on Cosmology : La Thuile, Italy, March 15-22, 2014en_US
dc.descriptionAuthors: JOY DIDIER, ASAD M. ABOOBAKER, PETER ADE, FRANQOIS AUBIN, CARLO BACCIGALUPI, KEVIN BANDURA, CHAOYUN BA, JULIAN BORRILL, BIKRAMJIT CHANDRA, DANIEL CHAPMAN, MATT DOBBS, JULIEN GRAIN , WILL GRAINGER, SHAUL HANANY, KYLE HELSON, SETH HILLBRAND, GENE HILTON, HANNES HUBMAYR, KENT IRWIN, BRADLEY JOHNSON, ANDREW JAFFE, TERRY JONES, TED KISNER, JEFF KLEIN, ANDREI KOROTKOV, ADRIAN LEE, LORNE LEVINSON, MICHELE LIMON, KEVIN MACDERMID, AMBER MILLER, MICHAEL MILLIGAN, ENZO PASCALE, GIUSEPPE PUGLISI, KATE RAACH, BRITT REICHBORN-KJENNERUD, CARL REINTSEMA, ILAN SAGIV, GRAEME SMECHER, RADEK STOMPOR, MA
dc.description.abstractThe E and B experiment (EBEX) is a balloon-borne telescope designed to measure the polarization of the cosmic microwave background radiation as well as that from Galactic dust. The instrument is equipped with a 1.5 meter aperture Gregorian-Dragone telescope, providing an 8' beam at three frequency bands centered on 150, 250 and 410 GHz. Polarimetry is achieved by rotating an achromatic half-wave plate on a superconducting magnetic bearing. In January 2013, EBEX completed 11 days of observations in a flight over Antarctica covering 6000 square degrees of the sky. Thls marks the first time that arrays with about= 1000 transition-edge sensor bolometers have made science observations on a balloon-borne platform. These proceedings describe the EBEX instrument, the science flight and the status of the data analysis.en_US
dc.description.sponsorshipEBEX is a NASA supported mission through grant numbers NNXOSAG40G and NNX07 AP36H. We thank Columbia Scientific Balloon Facility for their enthusiastic support of EBEX. We also acknowledge support from NSF, CNRS, Minnesota Super Computing Institute, Minnesota and Rhode Island Space Grant Consortia, the Science and Technology Facilities Council in the UK, Sigma Xi, and funding from collaborating institutions. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the office of Science of the U.S. Department of Energy under contract No. DE-AC02-05CH11231. The McGill authors acknowledge funding from the Canadian Space Agency, Natural Sciences and Engineering Research Council, Canadian Institute for Advanced Research, Canadian Foundation for Innovation and Canada Research Chairs program.en_US
dc.description.urihttps://inspirehep.net/files/6d437eb9c7d12accec9e6945d3a0c6bfen_US
dc.format.extent4 pagesen_US
dc.genreConference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2jxgw-czlb
dc.identifier.citationDidier, Joy et al. EBEX, the E and B Experiment. Proceedings, 49th Rencontres de Moriond on Cosmology : La Thuile, Italy, March 15-22, 2014, 41-44. https://inspirehep.net/literature/1337574en_US
dc.identifier.urihttp://hdl.handle.net/11603/25047
dc.language.isoen_USen_US
dc.publisherINSPIREen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleEBEX, THE E AND B EXPERIMENTen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0001-9238-4918en_US

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