A study is made for stellar and galaxy colours using a synthetic method. We show that a use of good colour response functions and a modern determination of the spectroscopic energy distribution for ff Lyr gives synthetic stellar colours in a good agreement with the observation to about 0.05mag. The synthetic method then applies to a study of galaxy colours using a spectrophotometric atlas of Kennicutt (1992), and a comparison is made with observed galaxy colours. The K-correction is calculated and compared with that of Coleman, Wu and Weedman (1980). We then study colours of galaxies in various colour band systems and obtain colour transformation laws, which enable us to find an offset among different observations for brightness of galaxies...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
We investigate the [3.6]-[4.5]Spitzer-IRAC colour behaviour of the early-type galaxies of the SAURON...
International audienceWe present empirical colour transformations between Sloan Digital Sky Survey u...
57 galaxies and 52 stars have been observed in four colors using a blue sensitive phototube. The re...
Abstract. Colours distributions have been studied in 12 S0 galaxies, most of these nearly edge-on, f...
Colours distributions have been studied in 12 S0 galaxies, most of these nearly edge-on, from high r...
We utilize color information for an H I-selected sample of 195 galaxies to explore the star formatio...
We discuss the colours of 99088 galaxies selected from the Sloan Digital Sky Survey (SDSS) Data Rele...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
International audienceWe use empirical techniques to interpret the near-infrared (near-IR) colours o...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
We have obtained integrated and nuclear spectra as well as U, B, R surface photometry for a represen...
The colours of the galaxy class known as Extremely Red Objects (EROs; R-K>5) are considered to be co...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
We have obtained integrated and nuclear spectra as well as U, B, R surface photometry for a represen...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
We investigate the [3.6]-[4.5]Spitzer-IRAC colour behaviour of the early-type galaxies of the SAURON...
International audienceWe present empirical colour transformations between Sloan Digital Sky Survey u...
57 galaxies and 52 stars have been observed in four colors using a blue sensitive phototube. The re...
Abstract. Colours distributions have been studied in 12 S0 galaxies, most of these nearly edge-on, f...
Colours distributions have been studied in 12 S0 galaxies, most of these nearly edge-on, from high r...
We utilize color information for an H I-selected sample of 195 galaxies to explore the star formatio...
We discuss the colours of 99088 galaxies selected from the Sloan Digital Sky Survey (SDSS) Data Rele...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
International audienceWe use empirical techniques to interpret the near-infrared (near-IR) colours o...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
We have obtained integrated and nuclear spectra as well as U, B, R surface photometry for a represen...
The colours of the galaxy class known as Extremely Red Objects (EROs; R-K>5) are considered to be co...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
We have obtained integrated and nuclear spectra as well as U, B, R surface photometry for a represen...
We have obtained integrated spectra and multifilter photometry for a representative sample of simila...
We investigate the [3.6]-[4.5]Spitzer-IRAC colour behaviour of the early-type galaxies of the SAURON...
International audienceWe present empirical colour transformations between Sloan Digital Sky Survey u...