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dc.contributor.authorFahim, N.
dc.contributor.authorPrada, F.
dc.contributor.authorKneib, J. P.
dc.contributor.authorGonzález de Rivera Peces, Guillermo José 
dc.contributor.authorHörler, P.
dc.contributor.authorSánchez, J.
dc.contributor.authorAzzaro, M.
dc.contributor.authorBecerril, S.
dc.contributor.authorBleuler, H.
dc.contributor.authorBouri, M.
dc.contributor.authorCastaño, J.
dc.contributor.authorGarrido, J.
dc.contributor.authorGillet, D.
dc.contributor.authorGómez, C.
dc.contributor.authorGómez, M. A.
dc.contributor.authorGonzález-Arroyo España, Antonio 
dc.contributor.authorJenni, L.
dc.contributor.authorMakarem, L.
dc.contributor.authorYepes Alonso, Gustavo 
dc.contributor.authorArrillaga, X.
dc.contributor.authorCarrera, M. A.
dc.contributor.authorDiego, R.
dc.contributor.authorCharif, M.
dc.contributor.authorHug, M.
dc.contributor.authorLachat, C.
dc.contributor.otherUAM. Departamento de Física Teóricaes_ES
dc.contributor.otherGrupo de Investigacion HCTLabes_ES
dc.contributor.otherInstituto de Física Teórica (IFT)es_ES
dc.date.accessioned2018-07-27T14:47:58Z
dc.date.available2018-07-27T14:47:58Z
dc.date.issued2015-06-11
dc.identifier.citationMonthly Notices of Royal Astronomical Society 450.1 (2015): 794–806en_US
dc.identifier.issn0035-8711 (print)es_ES
dc.identifier.issn1365-2966 (online)es_ES
dc.identifier.urihttp://hdl.handle.net/10486/684487
dc.descriptionThis article has been accepted for publication in Monthly Notices of Royal Astronomical Society © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserveden_US
dc.description.abstractMassive spectroscopic survey are becoming trendy in astrophysics and cosmology, as they can address new fundamental knowledge such as understanding the formation of the Milky Way and probing the nature of the mysterious dark energy. To enable massive spectroscopic surveys, new technology has been developed to place thousands of optical fibres at a given position on a focal plane. This technology needs to be: (1) accurate, with micrometer positional accuracy; (2) fast to minimize overhead; (3) robust to minimize failure; and (4) low cost. In this paper, we present the development, properties, and performance of a new single 8-mm in diameter fibre positioner robot, using two 4-mm DC-brushless gearmotors, that allows us to achieve accuracies up to 0.07 arcsec (5 μm). This device has been developed in the context of the Dark Energy Spectroscopic Instrumenten_US
dc.description.sponsorshipWe acknowledge support from the Spanish MICINNs Consolider-Ingenio 2010 Program me under grant MultiDark CSD2009-00064, HEPHACOS S2009/ESP-1473, and MINECO Centro de Excelencia Severo Ochoa Programme under grant SEV-2012-0249. We also thank the support from a CSIC-AVS contract through MICINN grant AYA2010-21231-C02- 01, and CDTI grant IDC-20101033; and support from the Spanish MINECO research grants AYA2012-31101 and FPA2012-34694. JPK, PH and LM acknowledge support from the ERC advanced grant LIDA and from an SNF Interdisciplinary grant.en_US
dc.format.extent13 pag.es_ES
dc.format.mimetypeapplication/pdfen
dc.language.isoengen
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
dc.relation.ispartofMonthly Notices of Royal Astronomical Societyen_US
dc.rights© 2015 The Authorses_ES
dc.subject.otherInstrumentation: spectrographsen_US
dc.subject.otherLargescale structure of Universeen_US
dc.subject.otherSurveysen_US
dc.subject.otherTechniques: spectroscopicen_US
dc.titleAn 8-mm diameter fibre robot positioner for massive spectroscopy surveysen_US
dc.typearticleen
dc.subject.ecienciaFísicaes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1093/mnras/stv541es_ES
dc.identifier.doi10.1093/mnras/stv541es_ES
dc.identifier.publicationfirstpage794es_ES
dc.identifier.publicationissue1es_ES
dc.identifier.publicationlastpage806es_ES
dc.identifier.publicationvolume450es_ES
dc.relation.projectIDGobierno de España. CSD2009-00064es_ES
dc.relation.projectIDGobierno de España. S2009/ESP-1473es_ES
dc.relation.projectIDGobierno de España. AYA2012-31101es_ES
dc.relation.projectIDGobierno de España. FPA2012-34694es_ES
dc.relation.projectIDComunidad de Madrid. S2009/ESP-1473/HEPHACOSes_ES
dc.relation.projectIDGobierno de España. SEV-2012-0249es_ES
dc.relation.projectIDGobierno de España. IDC-20101033es_ES
dc.relation.projectIDGobierno de España. AYA2010-21231-C02-01es_ES
dc.type.versioninfo:eu-repo/semantics/submittedVersionen
dc.rights.accessRightsopenAccessen
dc.authorUAMGonzález-Arroyo España, Antonio (259863)
dc.authorUAMYepes Alonso, Gustavo (260625)
dc.facultadUAMFacultad de Ciencias


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