Formación Académica

  • Ingeniero Civil Electricista, licenciado en Ciencias de la Ingeniería, Universidad de Chile.
  • Doctor en Ciencias de la Ingeniería con mención en Ingeniería Eléctrica, Universidad de Concepción.

Cursos que dicta

Pregrado

  • Ondas Electromagnéticas.
  • Circuitos Eléctricos II.
  • Antenas y Enlaces de Microondas.
  • Radio-Telescopios.
  • Fundamentos de las comunicaciones.

Producción Científica

Proyectos

  • 2019: “Estación monitora Radio Telescopio FYST”. Observatorio CCAT.
  • 2019: “Radio Telescopio MIST”. China-Chile Joint Research Fund.
  • 2018: “Radio Telescopio MIST”. BIP-UCSC 106.
  • 2018: “Radio Telescopio MIST”. Quimal/Conicyt 180003.
  • 2017: “Characterization of a new site for astronomy in Chile”. Comité Mixto ESO – Gobierno de Chile.
  • 2017: “Medición de PWV en el sitio de MARI-UCSC usando radiómetro de 183 GHz”. DIN-UCSC.
  • “2014-2015: “First step towards the construction of a Low-Frequency Telescope: RFI site-testing with MARI-UCSC”, Quimal/Conicyt (130005).
  • 2014: “Hands-on microwave receiver experiments for a new Radio Lab at UCSC”, Comité Mixto ESO – Gobierno de Chile.
  • 2014: “Proyecto GAVRT en Liceo de Isla de Pascua”, FAE-UCSC.
  • 2015: “Academic front-end for the Radio Lab at UCSC”, Comité Mixto ESO – Gobierno de Chile”.

Publicaciones

  • Cortés, F., et al (2020), “Twenty years of precipitable water vapor measurements in the Chajnantor area”. A&A, 640, A126.
  • Xu, Z., et al (2020), “Two-year Cosmology Large Angular Scale Surveyor (CLASS) observations: 40 GHz telescope pointing, beam profile, window function, and polarization performance”. ApJ, 891, Issue 2, 134.
  • Petroff, M., et al (2020), “Two-year Cosmology Large Angular Scale Surveyor (CLASS) observations: A first detection of atmospheric circular polarization at Q band”. ApJ, 889, Issue 2, 120.
  • Padilla, I., et al (2020), “Two-year Cosmology Large Angular Scale Surveyor (CLASS) observations: A measurement of circular polarization at 40 GHz”. ApJ, 889, Issue 2, 105.
  • Appel, J., et al (2019), “On-sky performance of the CLASS Q-band telescope”. ApJ, 876, Issue 2, 126.
  • Cortés F. et al. (2016), “Analysis of the distribution of precipitable water vapor in the Chajnantor area”, Radio Science, 51, 1166.
  • “Bustos R. et al. (2014), “Parque Astronómico de Atacama: an ideal site for millimeter, submillimeter, and mid-infrared astronomy”, PASP, 126, 1126.
  • QUIET collaboration (2013), “The QUIET Instrument”, Ap. J., 768, 9.
  • Rodríguez R. et al. (2012), “New capabilities for the Southern 1.2m mm-Wave Telescope”. Proc. SPIE 8452, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI, 845231.
  • QUIET collaboration (2012), “Second season QUIET observations: measurements of the CMB polarization power spectrum at 95 GHz”, Ap. J., 760, Issue 2, 145.
  • Taylor A. et al. (2011), “The Cosmic Background Imager 2”, MNRAS, 418, Issue 4, 2720.
  • Bustos R. et al. (2011), “Radiometer development at UdeC and PWV data at Chajnantor”. Astronomical Site Testing Data in Chile, RevMexAA, 41, 104-104.
  • QUIET collaboration (2011), “”First season QUIET observations: measurements of CMB polarization power spectra at 43 GHz in the multipole range 25 <= l <= 475”, Ap. J., 741, Issue 2, 111.
  • Vidal M. et al. (2011), “”Dust-correlated cm-wavelength continuum emission on translucent clouds ζ Oph and LDN 1780”, MNRAS, 414, Issue 3, 2424-2435.
  • Richards J. et al. (2011), “”Blazars in the Fermi era: The OVRO 40-m telescope monitoring program”, Ap. J. S., 194, Issue 2, id. 29.
  • Dickinson C. et al. (2010), “”IR-correlated 31 GHz radio emission from Orion East”, MNRAS, 407, Issue 4, 2223.
  • Angelakis E. et al. (2009), “”Multi-frequency measurements of the NVSS foreground sources in the Cosmic Background Imager fields. I. Data release”, A&A, 501, Issue 2, 801.
  • Sievers J. et al. (2009), “”Cosmological results from five years of 30 GHz CMB intensity measurements with the Cosmic Background Imager”, Preprint arXiv:0901.4540.
  • Sievers J. et al. (2007), “”Implications of the Cosmic Background Imager polarization data”, Ap. J., 660, 976.
  • Reeves R. et al. (2006), “Polarization spectrum of CMB obtained from the CBI”, RevMexAA, 26, 121.
  • Bustos R. (2005), “”The CBI project and latest results”, The Cool Universe: Observing the Cosmic Down. ASP Conference Series. 344, 37.
  • Readhead A. et al. (2004), “”Polarization Observations with the Cosmic Background Imager”, Science, 306, 836.
  • Readhead A. et al. (2004), “”Extended Mosaic Observations with the Cosmic Background Imager”, Ap. J., 609, 498.
  • Bustos R. (2002), “”2002: The driest and coldest summer”, ALMA Memo Serie 433.
  • Bustos R. (2001), “”Summer climate over Chajnantor”, ALMA Memo Serie 379.
  • Bustos R. et al. (2000), “”52 Years of climatological data for the Chajnantor area”, ALMA Memo Serie 333.
  • Bustos R. et al. (2000), “”UHF radio propagation experiment through the inversion capping Santiago (Chile) during an air pollution episode”. Environmental Technology, 21, 809.”

Líneas de investigación

  • Astro-Ingeniería
  • Recepción de señales analógicas
  • Enlaces de microondas
  • Antenas
  • Instrumentación
  • Estudio de calidad de sitios astronómicos