Aldo M. Serenelli
Identifiers
- name variant Aldo M. Serenelli 0.60 · backfill
Papers (19)
- A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS astro-ph.EP · 2019 · author #25
- Two chemically similar stellar overdensities on opposite sides of the plane of the Galaxy astro-ph.GA · 2018 · author #4
- A new Generation of Standard Solar Models astro-ph.SR · 2016 · author #2
- Asteroseismology of the Hyades with K2: first detection of main-sequence solar-like oscillations in an open cluster astro-ph.SR · 2016 · author #5
- The effect of $^{22}$Ne diffusion in the evolution and pulsational properties of white dwarfs with solar metallicity progenitors astro-ph.SR · 2016 · author #5
- Updated determination of the solar neutrino fluxes from solar neutrino data hep-ph · 2016 · author #5
- The Apache Point Observatory Galactic Evolution Experiment (APOGEE) astro-ph.IM · 2015 · author #71
- Revised Stellar Properties of Kepler Targets for the Quarter 1-16 Transit Detection Run astro-ph.EP · 2013 · author #20
- Multi-periodic pulsations of a stripped red giant star in an eclipsing binary astro-ph.SR · 2013 · author #2
- Solar Neutrinos: Status and Prospects astro-ph.SR · 2012 · author #3
- Solar models with accretion. I. Application to the solar abundance problem astro-ph.SR · 2011 · author #1
- Detection of solar-like oscillations from Kepler photometry of the open cluster NGC 6819 astro-ph.SR · 2009 · author #44
- New Results on Standard Solar Models astro-ph.SR · 2009 · author #1
- Solar heavy element abundance: constraints from frequency separation ratios of low-degree p modes astro-ph · 2007 · author #2
- What Is The Neon Abundance Of The Sun? astro-ph · 2005 · author #3
- New solar opacities, abundances, helioseismology, and neutrino fluxes astro-ph · 2004 · author #2
- How do Uncertainties in the Surface Chemical Abundances of the Sun Affect the Predicted Solar Neutrino Fluxes? astro-ph · 2004 · author #2
- Helioseismological Implications of Recent Solar Abundance Determinations astro-ph · 2004 · author #4
- How Accurately Can We Calculate the Depth of the Solar Convective Zone? astro-ph · 2004 · author #2
Mentions
- 1509.05420 #71 · backfill · confidence 0.70 Aldo M. Serenelli
- 1312.0662 #20 · backfill · confidence 0.70 Aldo M. Serenelli
- 1307.1654 #2 · backfill · confidence 0.70 Aldo M. Serenelli
- 1208.5723 #3 · backfill · confidence 0.70 Aldo M. Serenelli
- 1104.1639 #1 · backfill · confidence 0.70 Aldo M. Serenelli
- 1001.0026 #44 · backfill · confidence 0.70 Aldo M. Serenelli
- 0910.3690 #1 · backfill · confidence 0.70 Aldo M. Serenelli
- 0705.3154 #2 · backfill · confidence 0.70 Aldo M. Serenelli
Frequent Coauthors
- Sarbani Basu 10 shared papers
- John N. Bahcall 5 shared papers
- William J. Chaplin 5 shared papers
- Andrea Miglio 4 shared papers
- Saskia Hekker 4 shared papers
- Savita Mathur 4 shared papers
- Victor Silva Aguirre 4 shared papers
- Benoit Mosser 3 shared papers
- Daniel Huber 3 shared papers
- Dennis Stello 3 shared papers
- Marc Pinsonneault 3 shared papers
- Rafael A. Garcia 3 shared papers
- Timothy R. Bedding 3 shared papers
- Andrew W. Mann 2 shared papers
- Barry Smalley 2 shared papers
- Carlos Pena-Garay 2 shared papers
- David R. Soderblom 2 shared papers
- David W. Latham 2 shared papers
- Eric Gaidos 2 shared papers
- Guy R. Davies 2 shared papers