Atualizado: 23/06/2017

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SOAR - Classificação e Distribuição de tempo para o programa de Ciência Inicial
Semestre - 2017B

Projeto

Autor

Instituição

Título do Projeto

Horas

S-001 de Camargo, J.I.B. ON ToO - Stellar occultations of small distant solar system bodies in the Gaia era 12
S-014Kerber, L.UESCVIsible Soar star Clusters from tApii and Coxi HuguA (VISCACHA) survey: chemodynamical evolution and tidal history of the Magellanic Clouds60
S-013Fernades, B.IAGConspicuous features of molecular and ionized gas surrounding young star clusters19
S-004Galarza, J. Y.IAGFinding New Solar Twins for Planets, Stellar Evolution & Galactic Archaeology32
S-009Pelisoli, IngridUFRGSNeighbourhood watch: leave no white dwarf behind40
S-015De Pra, M.ON Compositional analysis of the outer belt Lixiahoua family II8
S-018Makler, M.CBPFEinstein Rings in the CFHT Stripe 82 Survey: from gravitational telescopes to probing Einstein's theory16
S-010Santiago, B.X.UFRGSDeep photometric follow-up of Milky-Way companions revealed by the Dark Energy Survey15
S-008Lopes, P.UFRJGalaxy Evolution within Interacting Galaxy Clusters10
S-007Pelisoli, IngridOutrosFollow-up spectroscopy of cool ELM candidates5
S-006Oliveira, A.S.UNIVAPSearch for new magnetic Cataclysmic Variables20
S-017Rimulo, L.IAGFundamental parameters of Be stars from Magellanic clusters: a census of Be stars and angular momentum loss rates10
S-003Reggiani, H MIAGFinding bright relics of the early Universe8
S-002Pelisoli, IngridUFRGSPhotometry of Extremely-Low Mass White Dwarf Candidates8
S-005da Costa, R.D.D.IAGGas and dust in comets from different dynamical groups5
S-012Romero, AUFRGSSearching for pulsating DA white dwarf stars near the blue edge of the instability strip8

Classificação e Distribuição de tempo para o programas de Longo Prazo -  Semestre - 2017A

Projeto

Autor

Instituição

Título do Projeto

Horas

S-104
(ID Original: SO2016A-014)
Brito, Alan, A UFRGS The UFRGS Open Cluster Survey (UOCS): searching for chemical anomalies in Galactic open clusters through CN and CH molecular band strengths 34