Matteo Cantiello
Astronomy and Astrophysics · 2007–2022
A researcher in the Science corpus: 13 papers; trusts 50 researchers and is trusted by 49 researchers here, as inferred from the citation graph.
Subfields
- Astronomy and Astrophysics — 424 citations into it; #1,465 of 10,964 by trust here, #1,874 by citations
- Instrumentation — 208 citations into it; #1,454 of 3,502 by trust here, #1,533 by citations
- Statistical and Nonlinear Physics — 41 citations into it
- Atomic and Molecular Physics, and Optics — 27 citations into it
- Education — 20 citations into it
- Computational Mechanics — 16 citations into it
- Ocean Engineering — 5 citations into it
Whom Matteo Cantiello trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
- Alexander Heger
- Sung-Chul Yoon
- N. Langer
- H. Spruit
- J. Christensen-Dalsgaard
- Stan Woosley
- Andre Maeder
- I. Hunter
- B. Paxton
- P. Eggenberger
Who trusts Matteo Cantiello overall
- J. Fuller
- Selma de Mink
- Ilya Mandel
- N. Langer
- J. Eldridge
- N. Smith
- Aaron Dotter
- Y. Qin
- J. Owen
- Sung-Chul Yoon
Papers from Matteo Cantiello's perspective
Ordered by how strongly the researchers Matteo Cantiello trusts endorse each paper. Same corpus, a different order for every researcher.
- Presupernova Evolution of Rotating Massive Stars. II. Evolution of the Surface Properties
- The Progenitor Stars of Gamma-Ray Bursts
- The chemical composition of the Sun
- Grids of stellar models with rotation - I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)
- Stellar evolution with rotation. VII. - Low metallicity models and the blue to red supergiant ratio in the SMC
- Stellar evolution with rotation XI. Wolf-Rayet star populations at different metallicities
- Dynamo action by differential rotation in a stably stratified stellar interior
- Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts
- On the variation of the initial mass function
- Dynamical Simulations of Magnetically Channeled Line-driven Stellar Winds. I. Isothermal, Nonrotating, Radially Driven Flow
Their papers
- Modules for Experiments in Stellar Astrophysics (MESA): Time-dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure (2022) — 333 citations
- Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation (2019) — 1,042 citations
- MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS (2016) — 948 citations
- MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS (2015) — 2,174 citations
- ANGULAR MOMENTUM TRANSPORT WITHIN EVOLVED LOW-MASS STARS (2014) — 168 citations
- MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARS (2013) — 2,495 citations
- Rotating massive main-sequence stars - I. Grids of evolutionary models and isochrones (2011) — 245 citations
- Rotating massive main-sequence stars: II. Simulating a population of LMC early B-type stars as a test of rotational mixing (2011) — 428 citations
- EVOLUTION OF MASSIVE STARS WITH PULSATION-DRIVEN SUPERWINDS DURING THE RED SUPERGIANT PHASE (2010) — 144 citations
- The VLT-FLAMES Tarantula survey (2009) — 457 citations
- Sub-surface convection zones in hot massive stars and their observable consequences (2009) — 258 citations
- Rotational mixing in massive binaries - Detached short-period systems (2009) — 197 citations
- Binary star progenitors of long gamma-ray bursts (2007) — 190 citations