Distribuição de Tempo 2024A
Publicado em
16/12/2020 13h32
Atualizado em
12/12/2023 15h02
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Distribuição de tempo SOAR 2024A |
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| Projeto | Autor | Instituição | Titulo | Tempo Concedido | |||||
| SO2024A-001 | Felipe Navarete | SOAR | Confirming ultracool subdwarfs withTripeSpec | 24.0 | |||||
| SO2024A-002 | Hektor Monteiro | UNIFEI | Linking the morphology of SNRs with theirX-ray central emission | 20.0 | |||||
| SO2024A-003 | Julio Camargo | ON | Studying distant small Solar System bodies through stellar occultations | 6.0 | |||||
| SO2024A-004 | Rafael Miloni Santucci | UFG | Finding the brightest very metal-poor starcandidates of the Galaxy | 29.0 | |||||
| SO2024A-005 | Maiara Sampaio Carvalho | IAG/USP |
The local relation between supersonic velocity dispersion and star formation tracers in |
9.6 | |||||
| SO2024A-006 | Paulo Vitor Souza dos Santos | UFRJ | Fine Structure of the Age-Chromospheric Activity Relation in Solar Type Stars: H-alpha | 30.0 | |||||
| SO2024A-008 | Denise R. Gonçalves | UFRJ | Confirming the nature of the only dated nova remnant crossing the hibernation valley | 3.5 | |||||
| SO2024A-010 | Toni Santana-Ros | ICC/UB |
Multi-technique study of the extreme Atira 2021 PH27: Search for large-particle activity at aphelion |
12.0 | |||||
| SO2024A-011 | Martin Makler | CBPF | Searching for decaying axion-like particles in z > 1.1 galaxy clusters with SOAR/SIFS | 16.0 | |||||
| SO2024A-013 | Swayamtrupta Panda | LNA | Unveiling the interplay between continuum and CIV emitting regions in high-redshift AGNs | 8.59 | |||||
| SO2024A-014 | Kethelin Parra Ramos | IAG/USP | The presence of diffuse light in fossil and non-fossil systems | 18.5 | |||||
| SO2024A-015 | Swayamtrupta Panda | LNA | Radio-mode AGN feedback caught in the act | 9.0 | |||||
| SO2024A-016 | Marcelo Emilio | UEPG | A follow-up to TESS Cycle 6 observations of Be stars: searching for outbursts | 18.0 | |||||
| SO2024A-017 | Larissa Luciano Amorim | UFRGS | Rotational period of magnetic white dwarfs | 30.0 | |||||
| SO2024A-019 | Hektor Monteiro | UNIFEI | Integral Field Spectroscopy of Two Peculiar Planetary Nebulae with High Adf Values | 12.0 | |||||
| SO2024A-020 | Thaisa Storchi Bergmann | UFRGS | Monthly monitoring of Active Galactic Nuclei with double-peaked emission line profiles | 48.0 | |||||
| SO2024A-021 | Clecio Roque De Bom | CBPF | Using SOAR to Observe sGRB Afterglows | 10.0 | |||||
| SO2024A-022 | Clecio Roque De Bom | CBPF | Observing the Next Optical Counterpart ofGW using SOAR | 10.0 | |||||
| SO2024A-023 | Augusto Damineli | IAG/USP | An atlas in mid-resolution to classify OB starsin the near-infrared | 20.0 | |||||
| SO2024A-024 | Danilo Ferreira da Rocha | ON | Radial velocity measurement of Be Binaryobserved by TESS | 22.0 | |||||
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Projetos de Longo Prazo |
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| SO2024A-101 | Francisco Ferreira Maia | UFRJ | The VISCACHA survey: disentangling thehistory of the Magellanic Clouds usingstar clusters | ||||||
| SO2024A-102 | Rogerio Riffel | UFRGS | SO-SMARTY: SOar mileS Moderateresolution neAr infRared sTellar librarY | ||||||
| SO2024A-103 | Felipe Navarete | SOAR | Follow-up of O4 Kilonovae transientsusing SOAR. | ||||||