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R. Buser

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author1
  • last author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • R. Buser — 13 papers, h 13

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982006
most citedColour Evolution of Disk Galaxy Models from z=4 to z=0

24 citations · 43 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2006★ 4 cited

On the geometrical evolution of the ionized gas in HII galaxies

F. Cuisinier, P. Westera, E. Telles +1

In this paper, we investigate the behaviour of the number of Lyman continuum ionizing photons as compared to the actual number of hydrogen recombinations in HII galaxies. We evalua…

astro-ph2002★ 24 cited

Colour Evolution of Disk Galaxy Models from z=4 to z=0

Pieter Westera, Markus Samland, Roland Buser +1

We calculate synthetic UBVRIJHKLM images, integrated spectra and colours for the disk galaxy formation models of Samland & Gerhard (2002), from redshift z=4 to z=0. Two models are…

astro-ph2001★ 15 cited

BaSeL: a library of synthetic spectra and colours for GAIA

E. Lastennet, T. Lejeune, E. Oblak +2

The BaseL Stellar Library (BaSeL) is a library of synthetic spectra which has already been used in various astrophysical applications (stellar clusters studies, characterization an…

astro-ph1998

Simultaneous solutions of stellar parameters (Teff, [Fe/H]) from synthetic uvby Stromgren photometry

E. Lastennet, T. Lejeune, P. Westera +1

The comprehensive knowledge of fundamental parameters of single stars is the basis of the modelling of star clusters and galaxies. Most fundamental stellar parameters of the indivi…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.