Study of the Spectral Response of Sky Quality Measurers

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dc.contributor.advisorRibas, Salvador J., 1978-
dc.contributor.authorCosta Ferrer, Laura
dc.date.accessioned2022-09-02T07:59:20Z
dc.date.available2022-09-02T07:59:20Z
dc.date.issued2022-06
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: Salvador J. Ribasca
dc.description.abstractThe aim of this project is to study the spectral response of two sky quality measurers, SQM and TESS-W, and compare the instrumental sky brightness obtained by these two photometers with the sky brightness obtained synthetically using its spectral response and night sky spectra from Montsec (Lleida), measured by SAND-4B spectrometer. We are going to analyze the difference between the magnitude measured by SQM and TESS-W to study if the atmospheric emission (airglow) at red wavelengths triggers the difference between the sky brightness measured by the previously mentioned instruments at the Montsecca
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttps://hdl.handle.net/2445/188640
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Costa, 2022
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física
dc.subject.classificationFotometria astronòmicacat
dc.subject.classificationCelcat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherAstronomical photometryeng
dc.subject.otherSkyeng
dc.subject.otherBachelor's theseseng
dc.titleStudy of the Spectral Response of Sky Quality Measurerseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca

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Treballs Finals de Grau (TFG) - Física