▪ Abstract Standard star photometry dominated the latter half of the twentieth century
reaching its zenith in the 1980s. It was introduced to take advantage of the high sensitivity …

The relations between colors of the JHKL systems of SAAO (Glass et al.), ESO (Engels et al.;
Wamsteker), CIT/CTIO (Elias et al.), MSO (Jones and Hylund; Hylund andMcGregor), AAO …

Transformation equations are presented to convert colors and magnitudes measured in the
AAO, ARNICA, CIT, DENIS, ESO, LCO (Persson standards), MSSSO, SAAO, and UKIRT …

The determination of stellar temperatures and surface gravities by means of the Stromgren
uvby beta photometric system is examined in the region of main sequence stars. We used a …

The availability of a number of new interferometric measurements of Main Sequence and
subgiant stars makes it possible to calibrate the surface brightness relations of these stars …

The author continues the description of his unification and reparametrization of results of
various authors on near-infrared photometry, by deriving intrinsic colours and absolute …

Based on CHARA Array measurements, we present the angular diameters of 23 nearby,
main-sequence stars, ranging from spectral types A7 to K0, 5 of which are exoplanet host …

Far-red spectra and VRIJHK photometry have been obtained for a sample of late-M dwarfs
selected on the basis of large reduced red magnitudes from the LHS Catalog. Half of the …

We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the
CHARA Array, successfully measuring the angular diameters of forty-four stars with an …

We have observed nearly 200 FGK stars at 24 and 70 μm with the Spitzer Space Telescope.
We identify excess infrared emission, including a number of cases where the observed flux …