VISTA Variables in the Vía Láctea (VVV): halfway status and results (2014)
- Authors:
- USP affiliated authors: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG ; SODRE JUNIOR, LAERTE - IAG
- Unidade: IAG
- Subjects: INSTRUMENTAÇÃO (ASTRONOMIA); GALÁXIA (VIA LÁCTEA)
- Language: Inglês
- Imprenta:
- Publisher place: Garching bei München
- Date published: 2014
- Source:
- Título: The Messenger
- Volume/Número/Paginação/Ano: v. 155, p. 24-29, 2014
-
ABNT
HEMPEL, Maren et al. VISTA Variables in the Vía Láctea (VVV): halfway status and results. The Messenger, v. 155, p. 24-29, 2014Tradução . . Disponível em: http://www.eso.org/sci/publications/messenger/archive/no.155-mar14/messenger-no155.pdf. Acesso em: 25 jan. 2026. -
APA
Hempel, M., Minniti, D., Dékány, I., Barbuy, B. L. S., & Sodré Júnior, L. (2014). VISTA Variables in the Vía Láctea (VVV): halfway status and results. The Messenger, 155, 24-29. Recuperado de http://www.eso.org/sci/publications/messenger/archive/no.155-mar14/messenger-no155.pdf -
NLM
Hempel M, Minniti D, Dékány I, Barbuy BLS, Sodré Júnior L. VISTA Variables in the Vía Láctea (VVV): halfway status and results [Internet]. The Messenger. 2014 ; 155 24-29.[citado 2026 jan. 25 ] Available from: http://www.eso.org/sci/publications/messenger/archive/no.155-mar14/messenger-no155.pdf -
Vancouver
Hempel M, Minniti D, Dékány I, Barbuy BLS, Sodré Júnior L. VISTA Variables in the Vía Láctea (VVV): halfway status and results [Internet]. The Messenger. 2014 ; 155 24-29.[citado 2026 jan. 25 ] Available from: http://www.eso.org/sci/publications/messenger/archive/no.155-mar14/messenger-no155.pdf - VISTA variables in the Via Lactea (VVV): the public ES0 near-IR variability survey of the Milky Way
- Spectra of bulge stars with know abundance ratios for population synthesis
- VVV DR1: the first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea
- Stellar populations in superclusters of galaxies
- Técnica de lentes fracas para mapeamento da distribuição de massa em aglomerados de galáxias
- Projeto observatórios virtuais: segunda fase
- What drives the Balmer extinction sequence in spiral galaxies?: Clus from the sloan digital sky Survey
- Neural computation as a tool for galaxy classification: methods and examples
- Can retired galaxies mimic active galaxies? Clues from the Sloan Digital Sky Survey
- Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph
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