I'm currently doing my Ph.D. at the Institute of Radioastronomy and Astrophysics (IRyA) at the National Autonomous University of México (UNAM in Spanish).
Antigua Carretera a Pátzcuaro #8701
Ex-Hda. San José de la Huerta
Morelia, Michoacán. México. C.P.58089
+52 (443) 322 38 45 ext. 32845
f.tapia@irya.unam.mx
ftapia@igeofisica.unam.mx
Stellar Chromospheres, Radioastronomy, Sun, Flares, Stellar Flares, and Ultracool Dwarf stars.
Astronomy & Astrophysics • 8 August 2016
René Liseau, V. De la Luz, E. O'Gorman, E. Bertone, M. Chavez and F. Tapia.
arXiv:1608.02384
DOI:10.1051/0004-6361/201629135
The Astrophysical Journal• 16 April 2019
Jacob Aaron White, J. Aufdenberg, A. C. Boley, M. Devlin, S. Dicker, P. Hauschildt, A. G. Hughes,
A. M. Hughes, B. Mason, B. Matthews, A. Moór, T. Mroczkowski, C. Romero, J. Sievers, S. Stanchfield,
F. Tapia, and D. Wilner
arXiv:1903.03481
DOI:10.3847/1538-4357/ab0e7f
The Astrophysical Journal Supplement Series• 6 January 2020
F. Tapia-Vázquez and V. De la Luz
arXiv:1912.02593
DOI:10.3847/1538-4365/ab5f05
Accepted to The Astrophysical Journal • 27 March 2020
Jacob Aaron White, F. Tapia-Vázquez, A. G. Hughes, A. Moór, B. Matthews, D. Wilner, J. Aufdenberg, A. M. Hughes, V. De la Luz, and A. Boley
arXiv:2003.12284
DOI:10.3847/1538-4357/ab8467
Assistant professor/ENES-Morelia • 2017
Assistant professor/ENES-Morelia • 2018
Associate professor/ENES-Morelia • 2020
Onsala Space Observatory (OSO), the Swedish National Infrastructure for Radio Astronomy, provides scientists with equipment to study the Earth and the rest of the Universe. In Onsala, 45 km south of Göteborg, we operate several radio telescopes for astronomy and geodesy. We take part in international radio astronomical projects, e.g., EVN, ALMA and SKA. The observatory is a geodetic fundamental station. The equipment for Earth sciences includes navigation satellite receivers, a superconducting gravimeter, tide gauges, and radiometers.
Radiotelescope, AGB
The CRAAM originated in 1960 as the Mackenzie Radio Astronomy Group - GRAM of the then Faculty of Philosophy, Sciences and Letters of Mackenzie University, incorporating the experimental activities of a group of students of physics and engineering, technicians, and amateurs of the Association of Amateurs of Astronomy, São Paulo, started since 1958. CRAAM activities in research and post-graduation were pioneers in Brazil, in the areas of radio science, including radio-astronomy, solar physics, solar-terrestrial relations, ionosphere physics, astrophysics, radio instrumentation science and space sciences.
Radioastronomy, Sun, Flares
Located in Budapest (Hungary) was founded in 1899, when Miklós Konkoly Thege donated his private observatory (f. 1871) to the state. Together with the Heliophysical Observatory in Debrecen, it forms the Astrophysical Institute of the Hungarian Academy of Sciences. Research includes observations with our 0.5-1 m class optical telescopes in the Piszkéstető Mountain Station, theoretical works and involvement in space projects.
Debirs Disk, Radioastrnomy, Solar-like Stars
The Large Millimeter Telescope Alfonso Serrano (or Gran Telescopio Milimétrico Alfonso Serrano) is the world´s largest single-dish steerable millimetre-wavelength telescope designed specifically for astronomical observations in the wavelength range of 0.85 – 4mm. This binational project between México and the United States of America represents the largest and most complex scientific instrument constructed in México. Situated on the summit of Volcán Sierra Negra at an altitude of 4600 meters, the LMT has begun its exploration of the physical processes that lead to the formation and evolution of planetary systems, stars, black-holes and galaxies thoughout the 13.7 billion year history of the Universe.
Radioastronomy
Photospheric emission becomes much easier to observe at millimeter wavelengths owing to the Rayleigh-Jeans Law. ALMA can resolve the photospheres and chromospheres of giant and supergiant stars within a few hundred parsecs. Moreover, in addition to free-free emission, ALMA will allow (sub)millimeter imaging of thermal emission from dust in stellar envelopes. ALMA will detect the photospheres of stars across the HR diagram. ALMA images of the the star α Centauri (see Figure 5.1) indicate that the millimeter and submillimeter emission (measured at 0.44, 0.74, 0.87, 1.3, 2.1, and 3.1 mm) may be fit well by Solar chromospheric models, suitably modified. In the upper atmosphere of the Sun, nonradiative heating processes operate, which appear to be important in other stars.
Main squence, G Type
KINICH-PAKAL is a new methodology to fit the observed and synthetic spectrum of solar-like stars at millimeter, submillimeter, and infrared wavelengths through semiempirical models of the solar chromosphere.
Stellar atmospheres
The first millimeter flare detected by Meredith A. MacGregor.
Stellar Flares, Millimeter, ALMA
The new generation of radio telescopes such as ALMA allows characterize stellar emission at submillimeter and millimeter wavelengths. This work is the first effort to understand how the emission affects the debris studies.
Radioastronomy, Stellar Atmospheres