Felipe Meza-ObandoInstituto Tecnológico de Costa Rica | TEC · Escuela de Ingeniería Electrónica
Felipe Meza-Obando
MSEE-DSP and MAA
About
4
Publications
2,026
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Introduction
Felipe Meza currently teaches at the Postgraduate School @ University of Costa Rica and @ Tecnológico de Costa Rica. Also is researcher @ Tecnológico de Costa Rica in LIANA and PARMA. Felipe does research in Electronic Engineering and Astrophysics in particular, the application of Machine Learning to Astrophysical problems, involving classification and prediction.
Additional affiliations
January 2017 - December 2019
Position
- External Collaborator
Description
- Currently collaborator in the Radio Telescope Project (ML and data analytics researcher). In 2018 Professor of Fundamental Astronomy, and in 2017 Professor of Data Mining in the Academic Master in Bioinformatics at the University of Costa Rica.
August 2015 - December 2018
January 2018 - June 2020
Position
- Researcher
Description
- Currently Professor of Machine Learning, Big Data, Pattern Recognition and Digital Communications at Master Program in Electronic Engineering and Data Science Program in Computer Department.
Publications
Publications (4)
La determinación del corrimiento al rojo, factor conocido como z, se obtiene a partir de las variaciones en la longitud de onda del espectro de la galaxia u objeto lejano, dicha variación se da entre la medición en la Tierra del elemento presente en la galaxia y la medición directamente en el objeto mediante espectroscopia. A partir del valor z, es...
The NASA Kepler mission operated for 4 years in space, and observed one field uninterruptedly, providing very high precision (1 ppm) light curves for around 160 000 stars with a high focus on the exploration of exoplanets.
However, Kepler lost two of its reaction wheels in 2014, and since then, it is
bound to observe along the Ecliptic Plane (EP),...
El estudio de binarias eclipsantes resulta de gran interés debido a que algunos tipos muestran periodos cortos de variabilidad en las curvas de luz, algunas veces en el orden de unas cuantas horas, lo anterior, facilita su medición desde observatorios en tierra. En este artículo presentamos el análisis de la observación y los resultados que derivar...
![Figura 2. Tránsito Planetario [Fuente: Nikola Smolenski, Wikimedia Commons]](profile/Felipe-Meza-Obando/publication/311487362/figure/fig8/AS:668652709896196@1536430637150/Figura-2-Transito-Planetario-Fuente-Nikola-Smolenski-Wikimedia-Commons_Q320.jpg)
![Figura 3. Estrella HAT-P-11 [Fuente: Sloan Digital Sky Survey SDSS ] Se...](profile/Felipe-Meza-Obando/publication/311487362/figure/fig2/AS:436789677694976@1481150182005/Figura-3-Estrella-HAT-P-11-Fuente-Sloan-Digital-Sky-Survey-SDSS-Se-trata-de-una_Q320.jpg)
The work described below has been carried out for the subject Observational Practices corresponding to the Master of Astronomy and Astrophysics of the Valencian International University. The objective of this work is to calculate accurately the exoplanet radius and from there determinate the composition and type of exoplanet, physical characteristi...
