B. Caccin

Solar granulation properties derived from three different time series

WASP-64 b and WASP-72 b: two new transiting highly irradiated giant planets

An absolutely calibratedT_effscale from the infrared flux method

The Confrontation between General Relativity and Experiment

An Earth-mass planet orbiting α Centauri B

Semiempirical Models of the Solar Atmosphere. I. The Quiet‐ and Active Sun Photosphere at Moderate Resolution

parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code

Accurate spectroscopic parameters of WASP planet host stars★

THE MOUNT WILSON OBSERVATORY S-INDEX OF THE SUN

Some comments on the limb shift of solar lines

History of solar oblateness measurements and interpretation

Solar Cycle Variation in Solar Irradiance

The Chemical Composition of the Sun

Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES‐2

Comparison of model calculations and photometric observations of bright “magnetic” regions

2-D multiline spectroscopy of the solar photosphere

Spectral line ratios as ${\vec T}_{\bf \sf eff}$ indicators in solar-like stars

Modeling solar irradiance variations through full-disk images and semi-empirical atmospheric models

High-Precision Measurements of the Solar Diameter and Oblateness by the Solar Disk Sextant (SDS) Experiment

Temperature variations in the solar photosphere

The Prototype RISE-PSPT Instrument Operating in Rome