activity
20022004
most citedIntroducing adapted Nelder & Mead's downhill simplex method to a fully automated analysis of eclipsing binaries

4 citations · 7 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph2004

Extracting stellar parameters from observed spectra: the role of cross-correlation and minimum distance methods

Tomaz Zwitter, Ulisse Munari, Arnaud Siebert

One may consider cross-correlation routines applied to stellar spectra as a way to determine not only the radial velocities but also to assess the properties of stellar atmospheres…

astro-ph2004

Probing Galactic reddening with the 8620 A diffuse interstellar band

S. Vidrih, T. Zwitter

Using the correlation between the equivalent width of the diffuse interstellar band (DIB) at 8620 A and the interstellar reddening reported by Munari (2000) GAIA could directly tra…

astro-ph20044 cited

Introducing adapted Nelder & Mead's downhill simplex method to a fully automated analysis of eclipsing binaries

A. Prsa, T. Zwitter

Eclipsing binaries are extremely attractive objects because absolute physical parameters (masses, luminosities, radii) of both components may be determined from observations. Since…

astro-ph2004

SB2 and eclipsing binaries with GAIA and RAVE

U. Munari, T. Zwitter, E. F. Milone

The expected performance of GAIA satellite on eclipsing binaries is reviewed on the basis of (a) combined Hipparcos and ground-based observations mimicking GAIA data harvest, and (…

astro-ph2003

Spectroscopy, Photometry and Micro-arcsec Astrometry of Binaries with the GAIA Space Mission and with the RAVE Experiment

Tomaz Zwitter, Ulisse Munari

GAIA astrometric mission of ESA will be very efficient in discovering binary and multiple stars with any orbital period, from minutes to millions of years. Main parameters of the r…

astro-ph20033 cited

Observational tests of the GAIA expected harvest on eclipsing binaries

Tomaz Zwitter

GAIA observations of eclipsing binary stars will have a large impact on stellar astrophysics. Accurate parameters, including absolute masses and sizes will be derived for $\sim 10^…