Front-end y Back-end de un radiotelescopio de 100-200 MHz orientado al estudio cosmológico de la Época de Reionización

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dc.contributor.advisorRodrı́guez Ferreira, Julián
dc.contributor.advisorRestrepo Gaitán, Óscar Alberto
dc.contributor.advisorAcevedo Cárdenas, Efrén Darío
dc.contributor.authorPerilla Mosquera, Felipe
dc.contributor.evaluatorChaparro Molano, Germán
dc.contributor.evaluatorBustos Placencia, Ricardo
dc.date.accessioned2022-09-23T21:54:30Z
dc.date.available2022-09-23T21:54:30Z
dc.date.created2022-09-15
dc.date.embargoEnd2024-09-15
dc.date.issued2022-09-15
dc.description.abstractRadio astronomy as an observational technique used in Astronomy allows experimental validation of theoretical models based on the study of electromagnetic cosmic waves. Technically, it uses dedicated instrumentation (radio telescopes) to acquire such signals. The study, based on the emission of 21-cm of neutral hydrogen at frequen- cies between 100 and 200 MHz, allows us to examine a scientific case of open study called Epoch of Reionization (EoR) in which we seek to compare physics models with experimental measurements. The reionization epoch is a link in the universe’s study in a primordial epoch, which allows us to understand the dynamic systems present at that epoch based on the behavior of electromagnetic waves. This project is based on simulations and measurements of the subsystems and the development of a software solution for data pre-processing, compatible with SDRs receivers. The aim is to validate the response of the antenna and the subsystems to establish the feasibility to use Software Defined Radio (SDR) technology devices as receivers for low-frequency radio telescopes. This project contributes to radio astronomy initiatives underway at the Universidad Industrial de Santander (UIS), which seek to position the university as a national and regional reference in this area of study.
dc.description.abstractenglishRadio astronomy as an observational technique used in Astronomy allows experimental validation of theoretical models based on the study of electromagnetic cosmic waves. Technically, it uses dedicated instrumentation (radio telescopes) to acquire such signals. The study, based on the emission of 21-cm of neutral hydrogen at frequen- cies between 100 and 200 MHz, allows us to examine a scientific case of open study called Epoch of Reionization (EoR) in which we seek to compare physics models with experimental measurements. The reionization epoch is a link in the universe’s study in a primordial epoch, which allows us to understand the dynamic systems present at that epoch based on the behavior of electromagnetic waves. This project is based on simulations and measurements of the subsystems and the development of a software solution for data pre-processing, compatible with SDRs receivers. The aim is to validate the response of the antenna and the subsystems to establish the feasibility to use Software Defined Radio (SDR) technology devices as receivers for low-frequency radio telescopes. This project contributes to radio astronomy initiatives underway at the Universidad Industrial de Santander (UIS), which seek to position the university as a national and regional reference in this area of study.
dc.description.degreelevelMaestría
dc.description.degreenameMagíster en Ingeniería de Telecomunicaciones 
dc.format.mimetypeapplication/pdf
dc.identifier.instnameUniversidad Industrial de Santander
dc.identifier.reponameUniversidad Industrial de Santander
dc.identifier.repourlhttps://noesis.uis.edu.co
dc.identifier.urihttps://noesis.uis.edu.co/handle/20.500.14071/11781
dc.language.isoeng
dc.publisherUniversidad Industrial de Santander
dc.publisher.facultyFacultad de Ingeníerias Fisicomecánicas
dc.publisher.programMaestría en Ingeniería de Telecomunicaciones
dc.publisher.schoolEscuela de Ingenierías Eléctrica, Electrónica y Telecomunicaciones
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rights.accessrightsinfo:eu-repo/semantics/openAccess
dc.rights.coarhttp://purl.org/coar/access_right/c_abf2
dc.rights.creativecommonsAtribución-NoComercial-SinDerivadas 4.0 Internacional (CC BY-NC-ND 4.0)
dc.rights.licenseAttribution-NonCommercial 4.0 International (CC BY-NC 4.0)
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subject.keywordRadiotelescope
dc.subject.keywordSDR
dc.subject.keywordradioastronomy
dc.titleFront-end y Back-end de un radiotelescopio de 100-200 MHz orientado al estudio cosmológico de la Época de Reionización
dc.title.englishFront-end and Back-end of a 100-200 MHz radio telescope focused on the cosmological study of the Epoch of Reionization
dc.type.coarhttp://purl.org/coar/resource_type/c_bdcc
dc.type.hasversionhttp://purl.org/coar/version/c_b1a7d7d4d402bcce
dc.type.localTesis/Trabajo de grado - Monografía - Maestría
dspace.entity.type
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