Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-27T10:01:12.588Z Has data issue: false hasContentIssue false
  • English
  • Français

Exercise #2 Observability and UV coverage

Published online by Cambridge University Press:  31 January 2003

G. Perrin ,
F. Malbet  and
D. Ségransan
D. Ségransan*
Affiliation:
Observatoire de Genève, 51 chemin des Maillettes, 1290 Sauverny, Switzerland
Get access

Abstract

This exercize is divided into two main parts. The first one intends to give a clear idea about the UV coverage with baselines of different orientations and targets of different declinations. It also emphasizes on the delay lines constraints for a 2 and a 3-telescope array. In the second part, different array configurations have to be selected to efficiently measure the radius of 3 close M dwarfs and the parameters (ρ, Θ, Δmag) of a binary system.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 6: Observing with the VLTI , 2003 , pp. 79
Copyright
© EAS, EDP Sciences, 2003

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)