At the end of the page you can find the instructions for the talk.
| Balbinot, Eduardo | University of Surrey | The devil is in the tails: the visibility of cold stellar streams |
| Dias, Bruno | ESO | The GOTHAM survey: homogeneous chemical evolution of Milky Way globular clusters |
| Ryde, Nils | Lund University | Detailed Abundances of Giants in the Inner Bulge and Galactic Centre |
| Kawata, Daisuke | University College London | Impacts of Radial Migration on the Galactic Thick and Thin Disks |
| Binney, James Jeffrey | University of Oxford | Tracking dark matter |
| Smith, Martin C. | Shanghai Astronomical Observatory | The Gaia-LAMOST Symbiosis – probing the chemodynamical evolution of the solar neighbourhood |
| Spitoni, Emanuele | University of Trieste, Department of Physics | The connection between the Galactic halo and ancient Dwarf Satellites |
| Bernard, Edouard | Lagrange – Observatoire de la Cote d’Azur | Reconstructing the star formation history of the solar neighborhood with Gaia |
| Sohn, Tony | Space Telescope Science Institute | Constraining the Formation and Mass of the Milky Way Halo using Globular Cluster Orbits from HST Proper Motions |
| Martell, Sarah L | University of New South Wales | Rediscovering the origins of the stellar halo with chemical tagging |
| Kallivayalil, Nitya Jacob | University of Virginia | Probing the Dark Halo of the Milky Way |
| Wetzel, Andrew | University of California, Davis | The Latte Project: Cosmological Simulations of Milky Way-like Galaxies and their Satellite Dwarf Galaxies |
| Nuza, Sebastián Ernesto | Instituto de Astronomía y Física del Espacio (IAFE) | Gas accretion onto MW-like galaxies and the Local Group |
| D’Onghia, Elena | University of Wisconsin, Madison | New Perspectives on the chemical tagging in GAIA and APOGEE-2 data |
| Ferguson, Annette | University of Edinburgh | Stellar Substructure in the Halos of the Milky Way and M31 |
| Gomez, Facundo Ariel | Max Planck Institute for Astrophysics | Warps and waves in the stellar discs of the Auriga cosmological simulations |
| Valentini, Marica | AIP | Using asteroseismology and spectroscopy for obtaining detailed abundances: CoRoT-GES and RAVE-K2 |
| Sheffield, Allyson | City University of New York | New Views From Galactoseismology: Rethinking the Galactic Disk-Halo Connection |
| Nissen, Poul Erik | Aarhus University | High-precision abundances of elements in stars with asteroseismic ages |
| Santiago, Basílio Xavier | UFRGS | Unravelling the structure and stellar populations of the outer Milky Way halo |
| Smiljanic, Rodolfo | Nicolaus Copernicus Astronomical Center | Chemical tagging experiment with the Gaia-ESO open clusters |
| Buck, Tobias | MPIA | NIHAO-UHD: Ultra High resolution cosmological simulations of Milky Way type galaxies and their surroundings |
| Melendez, Jorge | Universidade de Sao Paulo | Nucleosynthetic signatures unveiled by high precision abundances |
| Steinmetz, Matthias | AIP | The chemo-dynamical structure of the Milky Way with RAVE+TGAS |
| Li, Haining | National Astronomical Observatories, Chinese Academy of Sciences | LAMOST-Subaru exploration of chemical relics of first stars |
| Famaey, Benoit | CNRS Observatoire astronomique de Strasbourg | Distribution functions for resonantly trapped orbits in our Galaxy |
| Cescutti, Gabriele | I.N.A.F. Osservatorio Astronomico di Trieste | The oldest stars of the bulge: new information on the ancient Galaxy |
| Bensby, Thomas | Lund University | The age and abundance structure of the central kpc of the Milky Way – clues from microlensed dwarf stars |
| Casamiquela, Laia | Universitat de Barcelona | Chemical abundances of the Milky Way disk from OCCASO survey |
| Youakim, Kris | Leibniz Institute for Astrophysics Potsdam | The Pristine survey: Searching for metal poor stars with narrow-band photometry |
| Laporte, Chervin | Columbia | New views from galactoseismology: revised models of the impact of Sagittarius on the disc |
| Robin, Annie C. | Institut UTINAM | Kinematics of the local disc from RAVE survey and Gaia first data release |
| Buder, Sven | MPIA Heidelberg | Rediscovering our solar neighbourhood: Combining the GALAH survey and Gaia DR1 for a chemo-dynamic study in a melting pot of astrometry, photometry, and spectroscopy |
| Anders, Friedrich | Leibniz-Institut für Astrophysik Potsdam (AIP) | The APOGEE-TGAS red-giant sample: Precision chemo-dynamics in the extended solar vicinity |
| Wegg, Christopher | MPE | An Accurate Measurement of the IMF in the Inner Galaxy from Microlensing |
| Duong, Ly | The Australian National University | The GALAH survey: Properties of the Galactic thick disk and the inner galaxy |
| Chiti, Anirudh | MIT | Detection of a population of carbon-enhanced metal-poor stars in the Sculptor dwarf galaxy |
| Pasquini, Luca | ESO | A New Spectroscopic Facility |
| Weiss, Achim | Max-Planck-Institut für Astrophysik | Using low-mass stars as a tool: efforts towards precise models |
Instructions
To facilitate a smooth flow, we kindly ask you to prepare a presentation in pdf or powerpoint format and send it to iaus334-loc-at-aip.de the day before your talk, or hand it in via USB to one of the responsible persons during the coffee breaks (you can recognize them from the pink lanyard). We kindly ask Monday morning speakers to send their presentation in advance by Sunday, 9th July, 17:00 CEST.
Please send your final presentation to iaus334_loc@aip.de (please assure that its size does not exceed 20 MB. Alternatively, indicate some link (e.g. Dropbox) from which your presentation can be downloaded). The file name of your presentation should start with your surname.
Available presentation software will be Adobe Reader, MS PowerPoint 2010, and LibreOffice version 4, which will run under either Mac or Windows. Mac is also equipped with Keynote. Also available will be a current version of the VLC media-player as well as Windows Media Player. The screen format is 4:3. The computers will be connected to the internet for eventual on-line access during presentations; recent versions of Firefox and Chrome web-browsers are installed. Presentations prepared on other systems as well as presentations made with other software should be checked well in advance for compatibility. Speakers are encouraged to test their presentations before their session.
The room is equipped with a beamer, a computer, laser pointer and (sometimes slow!) wifi. There will be one person helping out in case technical support is needed.