The measurement of precise absolute fluxes for stellar sources has been pursued with
increased vigor since the discovery of dark energy and the realization that its detailed …

This paper presents a table with estimates of the absolute magnitude of the Sun and the
conversions from vegamag to the AB and ST systems for several wide-band filters used in …

We present an analysis of the intrinsic colors and temperatures of 5–30 Myr old pre-main-
sequence (pre-MS) stars using the F0-through M9-type members of nearby, negligibly …

Optical interferometry provides us with a unique opportunity to improve our understanding of
stellar structure and evolution. Through direct observation of rotationally distorted …

It is critical for James Webb Space Telescope (JWST) science that instrumental units are
converted to physical units. We detail the design of the JWST absolute flux calibration …

Principles of Adaptive Optics describes the foundations, principles, and applications of
adaptive optics (AO) and its enabling technologies. This leading textbook addresses the …

Various effective temperature scales have been proposed over the years. Despite much
work and the high internal precision usually achieved, systematic differences of order 100 K …

After a pedagogical introduction to the main concepts of synthetic photometry, colours and
bolometric corrections in the Johnson–Cousins, 2MASS, and HST-ACS/WFC3 photometric …

We present the first results obtained from the identification of∼ 30,000 sources in the
Spitzer/24 μm observations of the COSMOS field at S 24 μm≳ 80 μJy. Using accurate …

In order to accurately determine stellar properties, knowledge of the effective temperature of
stars is vital. We implement Gaia and 2MASS photometry in the InfraRed Flux Method and …