Alexandre Zabot

ORCID: 0000-0003-3727-0162
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About
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Research Areas
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Enhanced Oil Recovery Techniques
  • Gamma-ray bursts and supernovae
  • Lattice Boltzmann Simulation Studies
  • Cultural, Media, and Literary Studies
  • Galaxies: Formation, Evolution, Phenomena
  • Social and Economic Solidarity
  • Astrophysics and Star Formation Studies
  • Heat and Mass Transfer in Porous Media
  • Industrial Vision Systems and Defect Detection
  • Astrophysical Phenomena and Observations
  • Physical Education and Sports Studies
  • Physical Education and Gymnastics
  • GNSS positioning and interference
  • Adaptive optics and wavefront sensing
  • Hydraulic Fracturing and Reservoir Analysis
  • Media, Journalism, and Communication History
  • Social Sciences and Policies
  • Psychology and Mental Health
  • Brazilian cultural history and politics
  • Linguistics and Language Studies
  • Urban Development and Societal Issues
  • Cleft Lip and Palate Research
  • Education and Digital Technologies

Universidade Federal de Santa Catarina
2009-2024

Universidade Federal da Fronteira Sul
2010-2011

We describe the content and properties of UV source catalogs from GALEX’s All-Sky Imaging Survey (AIS, 5σ depth ≈19.9(FUV)/20.8(NUV) mag, in AB system) Medium-depth (MIS, ≈22.6(FUV)/22.7(NUV) mag), constructed by Bianchi L., et al.: Mon. Not. R. Astron. Soc. (2010, press). The contain 65.3/12.6 million (AIS/MIS) unique sources with photometric error NUV less than 0.5 over 21 435(AIS)/1579(MIS) square degrees. Matched optical data GSC-II provide additional B, R, I photometry for brightest...

10.1007/s10509-010-0581-x article EN cc-by-nc Astrophysics and Space Science 2011-01-17

We present comprehensive catalogs of hot star candidates in the Milky Way, selected from GALEX far-UV (FUV, 1344-1786 AA) and near-UV (NUV, 1771-2831 imaging. The FUV NUV photometry allows us to extract hottest stellar objects, particular white dwarfs (WD), which are elusive at other wavelengths because their high temperatures faint optical luminosities. generated UV sources two GALEX's surveys: AIS (All-Sky Imaging Survey, depth ABmag~19.9/20.8 FUV/NUV) MIS (Medium-depth ~22.6/22.7mag)....

10.1111/j.1365-2966.2010.17890.x article EN Monthly Notices of the Royal Astronomical Society 2010-12-15

A novel design technique for Rock-on-a-Chip microfluidic devices was developed allowing the creation of a macroporous system made up larger channels and vugs that can be filled with distinct microporosity types.

10.1039/d2lc00445c article EN Lab on a Chip 2022-01-01

Studies of debris disks around white dwarfs (WDs) have focused on infrared wavelengths because are much colder than the star and believed to contribute spectrum only at longer wavelengths. Nevertheless, these made dust grains which absorb scatter near-UV optical photons from WD, leaving a fingerprint that can be used further constrain disk properties. Our goal is show it possible detect effects in + integrated spectrum. We make theoretical calculations discuss necessary observational...

10.1088/0004-637x/704/2/l93 article EN The Astrophysical Journal 2009-09-30

Apresentamos neste artigo a transcrição francesa e tradução para o português da recémdescoberta entrevista de Georges Lemaître sobre Teoria do Big Bang, efetuada pela emissora belga Vlaamse Radio-en Televisieomroeporganisatie (VRT), em 1964 que, desde então, considerava-se como desaparecida. Para uma melhor contextualização, apresentamos também visão panorâmica as contribuições motivações Lemaître, bem outros vários aspectos históricos, talvez não tão conhecidos público menos especializado.

10.47976/rbhm2023v23n46440-461 article PT cc-by-nc-nd Revista Brasileira de História da Matemática 2023-07-19

10.26678/abcm.cobem2019.cob2019-0308 article EN Proceedings of the 26th International Congress of Mechanical Engineering 2019-01-01
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