University of Porto
Portugal
2022 - Research.com Physics in Portugal Leader Award
His primary areas of study are Astrophysics, Astronomy, Stars, Asteroseismology and Exoplanet. His work on Light curve, Metallicity, Effective temperature and Red clump is typically connected to Scaling as part of general Astrophysics study, connecting several disciplines of science. Tiago L. Campante works mostly in the field of Stars, limiting it down to concerns involving Radius and, occasionally, Photometry.
His Asteroseismology study integrates concerns from other disciplines, such as Spectral line, Red giant and Photometry. His Exoplanet study frequently draws parallels with other fields, such as Planetary system. His study explores the link between Subgiant and topics such as Mode that cross with problems in Likelihood-ratio test.
His main research concerns Astrophysics, Stars, Asteroseismology, Astronomy and Exoplanet. His Astrophysics research is multidisciplinary, incorporating elements of Radius and Mode. His Radius study combines topics in areas such as Spitzer Space Telescope and Frequency separation.
His Stars research includes themes of Amplitude and Spectral line. His Asteroseismology study combines topics from a wide range of disciplines, such as Stellar evolution, Red giant, Galaxy and Spectral density. His biological study spans a wide range of topics, including Stellar mass loss, Astrobiology and Transit.
Tiago L. Campante spends much of his time researching Stars, Astrophysics, Asteroseismology, Exoplanet and Planet. His Stars research is multidisciplinary, incorporating perspectives in Spectral line and Sample. His research in the fields of Star, Metallicity and Sky overlaps with other disciplines such as Benchmark and Espresso.
His Asteroseismology research incorporates elements of Milky Way, Red giant, Effective temperature and Kepler. Exoplanet is a subfield of Astronomy that Tiago L. Campante tackles. His research in Planet focuses on subjects like Radius, which are connected to Spectral density, Stellar mass and Giant planet.
His primary areas of investigation include Asteroseismology, Stars, Exoplanet, Astrophysics and Planet. In his research, Astrometry is intimately related to Galaxy, which falls under the overarching field of Asteroseismology. Stars is a subfield of Astronomy that Tiago L. Campante studies.
His Exoplanet research is multidisciplinary, relying on both Subgiant and Transit. Tiago L. Campante is interested in Red giant, which is a field of Astrophysics. The study incorporates disciplines such as Light curve, Radius and Spectral density in addition to Red giant.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets
Geoffrey W. Marcy;Howard Isaacson;Andrew W. Howard;Jason F. Rowe.
arXiv: Earth and Planetary Astrophysics (2014)
Masses, Radii, and Orbits of Small Kepler Planets: The Transition From Gaseous to Rocky Planets
Geoffrey W. Marcy;Howard Isaacson;Andrew W. Howard;Jason F. Rowe.
Astrophysical Journal Supplement Series (2014)
Testing Scaling Relations for Solar-Like Oscillations from the Main Sequence to Red Giants using Kepler Data
D. Huber;T. R. Bedding;D. Stello;S. Hekker.
arXiv: Solar and Stellar Astrophysics (2011)
Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission
W. J. Chaplin;H. Kjeldsen;J. Christensen-Dalsgaard;S. Basu.
Science (2011)
ASTEROSEISMIC FUNDAMENTAL PROPERTIES OF SOLAR-TYPE STARS OBSERVED BY THE NASA KEPLER MISSION
W. J. Chaplin;W. J. Chaplin;S. Basu;D. Huber;A. Serenelli.
Astrophysical Journal Supplement Series (2013)
Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology
Silva Aguirre;G.R. Davies;G.R. Davies;S Basu;J Christensen-Dalsgaard.
Monthly Notices of the Royal Astronomical Society (2015)
TESTING SCALING RELATIONS FOR SOLAR-LIKE OSCILLATIONS FROM THE MAIN SEQUENCE TO RED GIANTS USING KEPLER DATA
D. Huber;T. R. Bedding;D. Stello;S. Hekker;S. Hekker.
The Astrophysical Journal (2011)
Accurate parameters of 93 solar-type Kepler targets
H. Bruntt;S. Basu;B. Smalley;W. J. Chaplin.
arXiv: Solar and Stellar Astrophysics (2012)
Stellar Spin-Orbit Misalignment in a Multiplanet System
Daniel Huber;Joshua A. Carter;Mauro Barbieri;Andrea Miglio;Andrea Miglio.
Science (2013)
Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants
S. Deheuvels;S. Deheuvels;G. Doğan;G. Doğan;M. J. Goupil;T. Appourchaux.
Astronomy and Astrophysics (2014)
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