D-Index & Metrics Best Publications
Tiago L. Campante

Tiago L. Campante

University of Porto
Portugal

Physics
Portugal
2022

Research.com Recognitions

Awards & Achievements

2022 - Research.com Physics in Portugal Leader Award

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Statistics
  • Astrophysics

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 most cited work include:

  • Masses, Radii, and Orbits of Small Kepler Planets: The Transition From Gaseous to Rocky Planets (488 citations)
  • Masses, Radii, and Orbits of Small Kepler Planets: The Transition From Gaseous to Rocky Planets (488 citations)
  • Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets (478 citations)

What are the main themes of his work throughout his whole career to date?

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.

He most often published in these fields:

  • Astrophysics (132.25%)
  • Stars (119.82%)
  • Asteroseismology (107.69%)

What were the highlights of his more recent work (between 2018-2021)?

  • Stars (119.82%)
  • Astrophysics (132.25%)
  • Asteroseismology (107.69%)

In recent papers he was focusing on the following fields of study:

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.

Between 2018 and 2021, his most popular works were:

  • A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS (59 citations)
  • A Hot Saturn Orbiting an Oscillating Late Subgiant Discovered by TESS (57 citations)
  • AIMS - A new tool for stellar parameter determinations using asteroseismic constraints (45 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Statistics
  • Solar System

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.

Best Publications

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)

759 Citations

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)

536 Citations

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)

494 Citations

Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission

W. J. Chaplin;H. Kjeldsen;J. Christensen-Dalsgaard;S. Basu.
Science (2011)

362 Citations

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)

360 Citations

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)

353 Citations

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)

339 Citations

Accurate parameters of 93 solar-type Kepler targets

H. Bruntt;S. Basu;B. Smalley;W. J. Chaplin.
arXiv: Solar and Stellar Astrophysics (2012)

337 Citations

Stellar Spin-Orbit Misalignment in a Multiplanet System

Daniel Huber;Joshua A. Carter;Mauro Barbieri;Andrea Miglio;Andrea Miglio.
Science (2013)

312 Citations

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)

299 Citations

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