Slide 1VOScript | ESA-VO Team | INTEROP 2010, Nara | Pag. 1 VOScript: VO Spectral analysis scripting tool ESA-VO Team Juan González Deborah Baines Isa Barbarisi Andrea Laruelo…

Slide 1Data Acquisition & Distribution; and Archiving Plans Bill Boroski SDSS-II First Year Review National Science Foundation August 7, 2006 Slide 2 Data Acquisition…

Slide 1Stellar Rotation in the CoRoT Era Jose Dias do Nascimento Jr & José Renan de Medeiros and team DFTE- Natal Departamento de Física Teórica e Experimental, Brazil…

1. LETTER doi:10.1038/nature11878An eclipsing-binary distance to the Large MagellanicCloud accurate to two per centG. Pietrzynski1,2, D. Graczyk1, W. Gieren1, I. B. Thompson3,…

arX iv: 14 07 .22 45 v2 [a str o-p h.E P] 7 M ay 20 15 Draft version May 11, 2015 Preprint typeset using LATEX style emulateapj v. 5/2/11 CHANGING PHASES OF ALIEN WORLDS:…

Slide 1Chemical Cartography with SDSS/APOGEE Michael Hayden (NMSU), Jo Bovy (IAS), Steve Majewski (UVa), Jennifer Johnson (OSU), Gail Zasowski (JHU), Leo Girardi (Padova),…

Slide 1The Age-Metallicity-Velocity relation in the nearby disk Borja Anguiano Astrophysikalisches Institut Potsdam (AIP) K. Freeman (ANU), E. Wylie de Boer (ANU), M. Steinmetz…

Slide 1 Nuno C. Santos Cool Stars 13 - Hamburg, Germany - July2004 Spectroscopic characteristics of planet-host stars and their planets Nuno C. Santos (Observatory of Lisbon,…

Slide 1 The true orbits of visual binaries can be determined from their observed orbits as projected in the plane of the sky. Once the true orbit has been computed, determining…

Slide 1 The mass ratio of the stellar components of a spectroscopic binary can be directly computed from their ratio in radial velocities. To derive the total mass of the…