VOScript | ESA-VO Team | INTEROP 2010, Nara | Pag. 1 VOScript: VO Spectral analysis scripting tool ESA-VO Team Juan González Deborah Baines Isa Barbarisi.
Data Acquisition & Distribution; and Archiving Plans Bill Boroski SDSS-II First Year Review National Science Foundation August 7, 2006.
Stellar Rotation in the CoRoT Era Jose Dias do Nascimento Jr & José Renan de Medeiros and team DFTE- Natal Departamento de Física Teórica e Experimental,
An eclipsing binary_distance_to_the_large_magellanic_cloud_accurate_to_two_per_cent
Changing phases of_alien_worlds_probing_atmospheres_of_kepler_planets_with_high_precision_photometry
Skript Astrophysics
Chemical Cartography with SDSS/APOGEE Michael Hayden (NMSU), Jo Bovy (IAS), Steve Majewski (UVa), Jennifer Johnson (OSU), Gail Zasowski (JHU), Leo Girardi.
The Age-Metallicity-Velocity relation in the nearby disk Borja Anguiano Astrophysikalisches Institut Potsdam (AIP) K. Freeman (ANU), E. Wylie de Boer (ANU),
Nuno C. Santos Cool Stars 13 - Hamburg, Germany - July2004 Spectroscopic characteristics of planet-host stars and their planets Nuno C. Santos (Observatory.
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,
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.
Background information for users of STIS Charles R. Proffitt.