Atualizado: 27/11/2009

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SOAR - Distribuição de tempo
Semestre - 2010A

Projeto

Autor

Instituição

Título do Projeto

Horas

S-001 Diaz, M.P. IAG A Synoptic Spectroscopic Survey of Novae 41
S-015 Damineli, A. IAG Emission line stars and nebulae in the massive star cluster Westerlund1 13
S-021 Barbosa, C.L. UNIVAP Squished and Squashed: Probing GHII in the Presence of Massive Stars 16
S-002 Santiago, B.X. UFRGS The star clusters in the Magellanic Bridge: in situ star formation? 11
S-017 de Souza, T.R. UFSC Searching for the secondary star of HW Vir. 6,2
S-005 Damineli, A. IAG eta Carinae: high energy features along the orbital cycle 15
S-022 Oliveira, A.S. UNIVAP Search for the secondary stars in CBSS and V Sge binaries 8
S-011 Campos, F. UFRGS Deep photometry of the Globular Cluster NGC 6366 3,3
S-004 Kanaan, A. UFSC Mode identification in the pulsations of BPM37093 30
S-010 Telles, E. ON Characterizing the Evolutionary Stage of the Youngest Bursts in HII Galaxies 8
S-027 Tello, J. INPE Spectroscopy of Eclipsing Binaries in the OGLE Catalogue 23
S-009 Assafin, M. UFRJ 2010A Stellar Occultations by Pluto and its satellites plus by TNO Quaoar at SOAR 7,5
S-008 Moraes, O. C. IAG Planetary nebulae and the chemical evolution of the galactic bulge 16
S-018 Zabot, A. UFSC Near-Ultraviolet and Optical effects of Debris Disks around White Dwarfs 17
S-019 Moisés, A IAG K-band spectra of ionizing sources of Galactic HII regions 17
S-013 Kepler, S.O. UFRGS Spectroscopy of White Dwarf Stars 40
S-012 Kepler, S.O. UFRGS Searching for New White Dwarf Variables 80
S-023 Navarete, F. IAG Giant HII regions on the far side of the Galaxy 8
S-006 Emilio, M. UEPG Spectroscopic characterization of new CoRoT variable stars discovered in the exoplanet fields of the 20,5


Projetos que ganharam tempo no Telescópio Blanco (1 noite = 8,5h)

S-007 Balbinot, E. UFRGS Tidal tails around disrupting globular clusters 8,5
S-014 Proctor, R. IAG The Anatomy of the Compact Group HCG62 17
S-020 Cortes, C. UFRN The History of the Solar Angular Momentum: Pinning down Target Parameters in CoRoT Fields. 8,5