The available data on nuclear fusion cross sections important to energy generation in the
Sun and other hydrogen-burning stars and to solar neutrino production are summarized and …

In this article we review the current state of the field of solar neutrinos, including flavor
oscillations, nonstandard effects, solar models, cross section measurements, and the broad …

We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar
model and isochrone library for a solar-scaled heavy element distribution. The main input …

We present a study of 33 Kepler planet-candidate host stars for which asteroseismic
observations have sufficiently high signal-to-noise ratio to allow extraction of individual …

We use asteroseismic data from the Kepler satellite to determine fundamental stellar
properties of the 66 main-sequence targets observed for at least one full year by the mission …

An update of the NACRE compilation [3] is presented. This new compilation, referred to as
NACRE II, reports thermonuclear reaction rates for 34 charged-particle induced, two-body …

In the solar system, the planets' compositions vary with orbital distance, with rocky planets in
close orbits and lower-density gas giants in wider orbits. The detection of close-in giant …

We construct solar models with the newly calculated radiative opacities from the Opacity
Project (OP) and with recently determined (lower) heavy-element abundances. We compare …

We report the complete GNO solar neutrino results for the measuring periods GNO III, GNO
II, and GNO I. The result for GNO III (last 15 solar runs) is [54.3− 9.3+ 9.9 (stat)±2.3 (syst)] …

The paper describes a multilevel, multichannel R-matrix code, azure, for applications in
nuclear astrophysics. The code allows simultaneous analysis and extrapolation of low …