• español
  • English
  • français
  • Deutsch
  • português (Brasil)
  • italiano
    • español
    • English
    • français
    • Deutsch
    • português (Brasil)
    • italiano
    • español
    • English
    • français
    • Deutsch
    • português (Brasil)
    • italiano
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    Listar

    Todo UVaDOCComunidadesPor fecha de publicaciónAutoresMateriasTítulos

    Mi cuenta

    Acceder

    Estadísticas

    Ver Estadísticas de uso

    Compartir

    Ver ítem 
    •   UVaDOC Principal
    • TRABAJOS FIN DE ESTUDIOS
    • Trabajos Fin de Grado UVa
    • Ver ítem
    •   UVaDOC Principal
    • TRABAJOS FIN DE ESTUDIOS
    • Trabajos Fin de Grado UVa
    • Ver ítem
    • español
    • English
    • français
    • Deutsch
    • português (Brasil)
    • italiano

    Exportar

    RISMendeleyRefworksZotero
    • edm
    • marc
    • xoai
    • qdc
    • ore
    • ese
    • dim
    • uketd_dc
    • oai_dc
    • etdms
    • rdf
    • mods
    • mets
    • didl
    • premis

    Citas

    Por favor, use este identificador para citar o enlazar este ítem:https://uvadoc.uva.es/handle/10324/63339

    Título
    Llegando a los límites del bajo brillo superficial en la imagen de IC1101
    Autor
    Paisán García, Ángel
    Director o Tutor
    Buitrago Alonso, FernandoAutoridad UVA
    Editor
    Universidad de Valladolid. Facultad de CienciasAutoridad UVA
    Año del Documento
    2023
    Titulación
    Grado en Física
    Resumen
    Since the invention of the telescope in 1608, numerous technological breakthroughs have allowed us to improve the quality of the technology around us, while at the same time increasing our understanding of the Universe and our curiosity. In this End of Degree Assignment, I will try to take advantage of the latest technological advances in astronomy to study the largest galaxy ever found, IC1101. The theoretical background related with Extragalactic Astrophysics will be presented introducing concepts such us magnitude, black body, CCD, redshift, etc. In addition, the computational background utilized during this work will also be explained. I carried out a photometric study of IC1101 determining its surface brightness profile and mass profiles among other observables. Furthermore, I will also show how the IC1101 image was taken, and I will compute the external part of the PSF of its images. This analysis will help us obtaining information about the mysterious IC1101 galaxy. It should be emphasized that, in order to accomplish the present work, I had to develop several programs in Python as well as read and understand many Astrophysical concepts which helped me to obtain a first insight on what research really is.
    Palabras Clave
    Astrofísica
    Galaxias
    Fotometría
    Departamento
    Departamento de Física Teórica, Atómica y Óptica
    Idioma
    spa
    URI
    https://uvadoc.uva.es/handle/10324/63339
    Derechos
    openAccess
    Aparece en las colecciones
    • Trabajos Fin de Grado UVa [30857]
    Mostrar el registro completo del ítem
    Ficheros en el ítem
    Nombre:
    TFG-G6680.pdf
    Tamaño:
    4.551Mb
    Formato:
    Adobe PDF
    Thumbnail
    Visualizar/Abrir
    Attribution-NonCommercial-NoDerivatives 4.0 InternacionalLa licencia del ítem se describe como Attribution-NonCommercial-NoDerivatives 4.0 Internacional

    Universidad de Valladolid

    Powered by MIT's. DSpace software, Version 5.10