Recent Changes in GREATITNFC Web retrieved at 05:23 (GMT)
GREATITNFC Web Preferences The following settings are web preferences of the GREATITNFC web. These preferences overwrite the site level preferences in...
Proceedings The Milky Way Unravelled by Gaia Proceedings for the conference have been published in the `EAS Publications Series` They will be referenced...
Participants The Milky Way Unravelled by Gaia The list is being manually updated (as of 28 November) Participant Institution Abedi, Hoda Universitat...
The Milky Way Unravelled by Gaia GREAT Science from the Gaia Data Releases, Barcelona (Spain) 1 5 December 2014 NEWS: 20141109 the programme listing all speakers...
Outreach / Divulgaci...
Rationale Registration Important Dates Programme Participants Presenter Info Outreach/Divulgaci...
Programme The Milky Way Unravelled by Gaia Talks / Posters / Abstract Book When ID What Who Institute Slides Monday 1 December...
Important Dates The Milky Way Unravelled by Gaia First announcement: 15th August 2014 ( DONE ) Opening of registration and abstract submission: 15th September...
Local Organizing Committee The Milky Way Unravelled by Gaia Francesca Figueras (Chair) Carme Jordi Jordi Torra Xavier Luri Lola Balaguer...
The formation of the Milky Way bulge and its X shaped structure Juntai Shen Zhao Yu Li (SHAO, Shanghai, China) Bulges are commonly believed to form in the dynamical...
Baysian Inference of Kinematics and Memberships of Open Clusters Zhengyi Shao (SHAO, Shanghai, China) TBD
The M giants classication in the LAMOST DR1 Jing Zhong (SHAO, Shanghai, China) TBD
Pictures
PreciseSpectrosopicParametersForSolar-typeStarsWithModerate-to-highRotation
9 years ago - NEW
SusanaBascon
Precise spectroscopic parameters for solar type stars with moderate to high rotation Maria Tsantaki (CAUP, Porto, Portugal) One of the primary objectives of Gaia...
On the connection between the thick disk and the barred galactic bulge A. Spagna, A. Curir, M. G. Lattanzi, P. Re Fiorentin, A.Laura Serra (INAF, Torino, Italy...
VOSA: SED building and analysis of thousands of stars in the framework of Gaia E.Solano, C.Rodrigo, A.Bayo (CAB INTA CSIC, Spain) VOSA(VOSedAnalyzer, ttp://svo...
PeeningThorughTheDust:PreciseAstrometryOfTheGalacticMid-planeWithTheVVVSurvey
9 years ago - NEW
SusanaBascon
Peering through the dust: Precise astrometry of the Galactic mid plane with the VVV survey Leigh Smith, Philip Lucas, Hugh Jones (University of Herfordshire, UK...
Origin of the metallicity distribution in the thick disc Maider Sancho Miranda, Bradley Gibson, Kate Pilkington, Christopher Brook, Patricia Sanchez Blazquez (University...
EstimatingGaiaSPerformancesForOStarsInTheOuterGalacticPlaneUsingHerschelData
9 years ago - NEW
SusanaBascon
Estimating Gaia...
Characterisation of the Gaia Red Clump L. Ruiz Dern (Observatoire de Paris Meudon, France) The Red Clump is a compact group of stars located in the giant branch...
RSS feed, ATOM feed, WebNotify, site changes, site map 
Topic revision: r4 - 2006-11-15 - TWikiContributor
GREATITNFC
Copyright © 2008-2024 by the contributing authors. All material on this collaboration platform is the property of the contributing authors. Ideas, requests, problems regarding TWiki? Send feedback