dc.contributor.author | Ortiz García, David | |
dc.contributor.author | Casas Reinares, Francisco Javier | |
dc.contributor.author | Ruiz Lombera, Rubén | |
dc.contributor.author | Mirapeix Serrano, Jesús María | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2018-03-09T13:03:19Z | |
dc.date.available | 2018-04-30T02:45:12Z | |
dc.date.issued | 2017-04-10 | |
dc.identifier.issn | 0034-6748 | |
dc.identifier.issn | 1089-7623 | |
dc.identifier.other | ESP2015-70646-C2-1-R | es_ES |
dc.identifier.other | CSD2010-00064 | es_ES |
dc.identifier.uri | http://hdl.handle.net/10902/13268 | |
dc.description.abstract | In this paper, a microwave interferometer prototype with a near-infra-red optical correlator is proposed as a solution to get a large-format interferometer with hundreds of receivers for radio astronomy applications. A 10 Gbits/s Lithium Niobate modulator has been tested as part of an electro-optic correlator up-conversion stage that will be integrated in the interferometer prototype. Its internal circuitry consists of a single-drive modulator biased by a SubMiniature version A (SMA) connector allowing to up-convert microwave signals with bandwidths up to 12.5 GHz to the near infrared band. In order to characterize it, a 12 GHz tone and a bias voltage were applied to the SMA input using a polarization tee. Two different experimental techniques to stabilize the modulator operation point in its minimum optical carrier output power are described. The best achieved results showed a rather stable spectrum in amplitude and wavelength at the output of the modulator with an optical carrier level 23 dB lower than the signal of interest. On the other hand, preliminary measurements were made to analyze the correlation stage, using 4f and 6f optical configurations to characterize both the antenna/fiber array configuration and the corresponding point spread function. | es_ES |
dc.description.sponsorship | This work was supported by the Ministerio de Economía y Competitividad, Spain, under the Plan Nacional de I+D+i project with Reference No. ESP2015-70646-C2-1-R cofinanced with EU FEDER funds and the CONSOLIDER INGENIO 2010 programme under the Reference No. CSD2010-00064. The authors would like to thank Félix Gracia from Instituto Astrofísico de Canarias (IAC) for his assistance and help. | es_ES |
dc.format.extent | 8 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | American Institute of Physics | es_ES |
dc.rights | © 2017 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in Review of Scientific Instruments, 2017, 88(4), 044702 and may be found at https://doi.org/10.1063/1.4979811 | * |
dc.source | Review of Scientific Instruments, 2017, 88(4), 044702 | es_ES |
dc.title | Electro-optic correlator for large-format microwave interferometry: Up-conversionand correlation stages performance analysis | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1063/1.4979811 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1063/1.4979811 | |
dc.type.version | publishedVersion | es_ES |