When |
ID |
What |
Who |
Institute |
Slides |
|
|
|
|
|
|
09.00-09.15 |
C2.3 |
Measuring the Gaia basic angle variations: the BAM on-board laser interferometer |
Alcione Mora |
|
|
09.00-09.45 |
QA3 |
Scientific synergies of Gaia with ground based spectroscopic surveys |
Alejandra Recio-Blanco (I) |
Observatoire Cote d'Azur, Nice, France |
|
12.00-12.15 |
E4.4 |
Population seismology with large time-resolved astronomical surveys |
Alejandra Sans (E) |
KU Leuven, Belgium |
|
11.30-12.00 |
I3.2 |
Astrometric Discovery of Extrasolar Planets |
Alessandro Sozzetti (I) |
INAF-Torino, Italy |
|
12.00-12.30 |
I3.3 |
Planet formation with Gaia |
Anders Johansen (I) |
Lund University, Sweden |
|
17.30-17.45 |
E5.6 |
Towards a dynamically self-consistent evolutionary model of the Milky Way |
Andre Martins (E) |
UTINAM, Besançon, France |
|
12.15-12.30 |
C5.2 |
Constraints on thin and thick disc formation from new analysis of 2MASS and SDSS surveys |
Annie Robin |
UTINAM, Besançon, France |
|
12.15–12.45 |
I7.1 |
Astrometry Futures 2020 |
Anthony Brown (I) |
Leiden University, The Netherlands |
|
12.45-13.00 |
C4.2 |
The open clusters in the Gais ESO Surveys and beyond |
Antonella Vallenari (I) |
Osservatorio Astrofisico di Padova, Italy |
|
12.00-12.15 |
C6.4 |
Eclipsing binaries in the Gaia era: automated detection performance |
Berry Holl |
UNIGE, Switzerland |
|
12.30-12.45 |
C5.3 |
Orbit of the Ophiuchus Stream |
Branimir Sesar |
MPIA, Heidelberg, Germany |
|
17.15-17.30 |
E4.1 |
Open cluster evolution and the search for the Sun’s siblings |
Carmen Martinez (E) |
Leiden University, The Netherlands |
|
17.30-17.45 |
E4.2 |
Finding the lost siblings of the Sun |
Cheng Liu (E) |
ASTRO, Lund Observatory, Sweden |
|
17.30-17.45 |
C2.1 |
Gaia Validation Tasks |
Claus Fabricius |
ICC-UB / IEEC, Spain |
|
15.30-16.00 |
|
Coffee break and poster viewing |
10.30-11.00 |
|
Coffee break and poster viewing |
16.15-16.45 |
|
Coffee break and poster viewing |
11.00-11.30 |
|
Coffee break and poster viewing |
11:00-11:30 |
|
Coffee break and poster viewing |
16.15-16.45 |
|
Coffee break and poster viewing |
10.30-11.00 |
|
Coffee break and poster virwing |
16.30–17.00 |
I2.2 |
New observational constraints to chemodynamical models of the Milky Way |
Cristina Chiappini (I) |
AIP, Postsdam, Germany |
|
17.45-18.00 |
C5.6 |
Stellar motion around co-rotating spiral arm: Gaia Mock data |
Daisuke Kawata |
MSSL/UCL, UK |
|
18.00-18.15 |
C5.7 |
Hypervelocity stars in the Gaia era |
Elena Rossi |
Leiden University, The Netherlands |
|
12.00-12.15 |
E5.4 |
Assessing the impact of astronomical phenomena on the Earth |
Fabo Feng (E) |
MPIA, Heidelberg, Germany |
|
Friday 5 December 2014 |
14.30-15.00 |
I5.4 |
Dynamical models of the Galactic Disk |
Hans-Walter Rix (I) |
MPIA, Heidelberg, Germany |
|
17.15-17.35 |
E5.5 |
On the characterization of the Galactic warp in the Gaia era |
Hoda Abedi (E) |
ICC-UB / IEEC, Spain |
|
11.00–11.30 |
I3.1 |
The Gaia mission in the rapidly-evolving context of exoplanet science |
Ignasi Ribas (I) |
ICE - IEEC, Spain |
|
10.00-10.15 |
E5.1 |
Large-scale structure of the inner Milky Way |
Iulia Simion (E) |
IoA, Univ. Cambridge, UK |
|
14.45-15.30 |
QA1 |
Galactic Archaeology |
Ivan Minchev (I) |
Leibniz-Institut für Astrophysik Potsdam AIP |
|
10.00-10.15 |
C2.7 |
A PRIMAL view of the Milky Way, made possible by Gaia and M2M modelling |
Jason Hunt |
MSSL/UCL, UK |
|
15.30-16.15 |
QA2 |
What drives the evolution of the Milky Way’s disk? |
Jo Bovy (I) |
Institute for Advanced Studies, Princeton, USA |
|
10.15-10.30 |
E5.2 |
Galactic assembly history. The halo–satellite connection |
John Vickers (E) |
ARI, Heidelberg, Germany |
|
17.45-18.00 |
C2.2 |
From telemetry to science |
Jordi Portell |
ICC-UB / IEEC, Spain |
|
17.00–17.30 |
I2.3 |
Gaia Science Performance |
Jos de Bruijne (I) |
ESTEC, ESA, The Netherlands |
|
11.30-12.00 |
I4.3 |
Asteroseismology |
Josefina Montalban (I) |
University of Leige, Belgium |
|
15.30-16.00 |
I5.6 |
Scientific synergies of Gaia with ground based spectroscopic surveys |
Joss Bland-Hawthorn (I) |
University of Sidney, Australia |
|
11.30–12.00 |
I5.3 |
Clusters, Disks and Galaxy Structure |
Justin Read (I) |
University of Surrey, UK |
|
16.45-17.15 |
I4.1 |
The evolution of the Galactic disk with open clusters |
Laura Magrini (I) |
INAF-Acetri, Italy |
|
09.30-09.45 |
C2.5 |
The variability Analysis and Processing of Gaia data |
Laurent Eyer |
UNIGE, Switzerland |
|
10.30-11.00 |
|
!PhD focus: discussion session |
Led by Alejandra Sans & Sergi Blanco-Cuaresma |
LAB, Bourdeaux, CNRS, France |
|
12.30-12.45 |
E3.1 |
Exoplanets: Gaia and the importance of ground based spectroscopy follow-up |
Lisa Benamati (E) |
IA, University of Porto, Portugal |
|
12.15-12.30 |
E4.5 |
Highlights of the LINEAR survey |
Lovro Palaversa (E) |
UNIGE, Geneve, Switzerland |
|
16.45–17.15 |
I5.7 |
A multi-scale approach to simulate the Galaxy |
Luis Aguilar (I) |
UNAM, Ensenada, Mexico |
|
11.45-12.00 |
C6.3 |
Gaia Science Alerts |
Lukasz Wyrzykowski |
OAUW, Warsaw University, Poland |
|
13.15-14.30 |
|
Lunch and Conference Close |
13.15-14.45 |
|
Lunch and poster viewing |
13.15-14.45 |
|
Lunch and poster viewing |
13.00-14.30 |
|
Lunch and poster viewing |
16.00-16.15 |
C5.5 |
Radial velocities and chemical tagging with WEAVE at the WHT |
Marc Balcells |
ING, La Palma, Spain |
|
12.45-13.00 |
C5.4 |
The Perseus arm stellar overdensity at 1.6 kpc |
Maria Monguió, |
Universidad de Alicante, Spain |
|
09.15-09.30 |
C2.4 |
Gaia Radial Velocity Spectrograph Performance |
Mark Cropper |
MSSL/UCL, UK |
|
18.00-18.15 |
C4.1 |
Stellar relics from the cosmic dawn in the Milky Way bulge |
Martin Asplund |
Australian National University, Camberra, Australia |
|
18.15-18.30 |
C5.8 |
Cool runaways - Nearby Hills ejecta as a probe of the gravitational potential of the Milky Way |
Martin Smith |
SHAO, Shanghai, Xina |
|
10.30-10.45 |
E5.3 |
Substructure in galaxy discs: Identifying secularly evolved populations |
Matthew Molloy (E) |
KIAA/PKU, Beijing, Xina |
|
09.00–09.30 |
I5.1 |
RAVE as a Gaia precursor, what to expect from the Gaia RVS? |
Matthias Steinmetz (I) |
AIP, Potsdam, Germany |
|
09.30-09.45 |
E6.1 |
Towards an absolute stellar luminosity atlas |
Max Palmer (E) |
ICC-UB / IEEC, Spain |
|
10.15-10.30 |
C2.8 |
Analysing the disc Red Clump stars of the Galactic bar in the Gaia space of observables |
Mercè Romero-Gómez |
ICC-UB / IEEC, Spain |
|
16.00-16.30 |
I2.1 |
Galactic evolution and chemical evolution |
Misha Haywood (I) |
Observatoire de Paris, France |
|
Monday 1 December 2014 |
11.30-11.45 |
E6.3 |
Classification of Supernova from Gaia Alerts |
Nadejda Blagoródnova (E) |
IoA, Cambridge University, UK |
|
14.10–14.30 |
I1.1 |
GREAT-ITN and Gaia: Preparing for Science |
Nicholas Walton |
IoA, Univ. Cambridge, UK |
|
12.45–13.05 |
I7.2 |
GREAT2Net - Networking in the Era of Gaia |
Nicholas Walton (I) |
IoA, Univ. Cambridge, UK |
|
10.00-10.15 |
C6.1 |
Infrared survey of variable stars toward the bulge and beyond |
Noriyuki Matsunaga |
University of Tokyo, Japan |
|
09.00-09.30 |
I6.2 |
Gaia, Variable Stars and the Distance Scale |
Patricia Whitelock (I) |
SAAO, Cape Town, South Africa |
|
09.45-10.00 |
C2.6 |
Making action-angle disc models for Gaia |
Paul McMillan |
ASTRO, Lund Observatory, Sweden |
|
09.45-10.30 |
QA4 |
Galactic Dynamics |
Ralph Schönrich (I) |
Oxford University, UK |
|
12.30-14.00 |
|
Registration |
11.00-11.30 |
I6.3 |
Supernovae |
Rubina Kotak (I) |
Queen's University Belfast, UK |
|
15.00-15.30 |
I1.3 |
Astrometry - Gaia, Techniques and Limitations |
Sergei Klioner (I) |
Lohrmann Observatory, Dresden, Germany |
|
17.45-18.00 |
E4.3 |
Testing the chemical tagging technique with Open Clusters |
Sergi Blanco-Cuaresma |
LAB, Bourdeaux, CNRS, France |
|
14.00-15.30 |
|
Session 1: The GREAT ITN and Gaia: Context and Status |
Chair: |
09.00-10.30 |
|
Session 2 (cont): The Physics and Science Promise of Gaia |
Chair: |
16.00-18.00 |
|
Session 2: The Physics and Science Promise of Gaia |
Chair: |
11.00-13.15 |
|
Session 3: Planetary Systems: Worlds Near and Far |
Chair: |
|
|
Session 4: The Stellar Constituents of the Milky Way |
16.45-18.15 |
|
Session 4A: Star Cluster Evolution |
Chair: |
11.30-13.00 |
|
Session 4B: Stellar Astrophysics |
Chair: |
|
|
Session 5: The Origin and History of the Milky Way |
Chair: |
09.30-11.00 |
|
Session 5A: Archaeology of the Milky Way |
Chair: |
11.30-13.00 |
|
Session 5B: Galactic Structure and Evolution |
Chair: |
14.30-16.15 |
|
Session 5C: Gaia, Galactic Surveys, Modelling, Synergies |
Chair: |
16.45-18.30 |
|
Session 5D: Galactic Dynamics |
Chair: |
09.00-11.00 |
|
Session 6: Grand Challenges from Gaia |
09.00-10.30 |
|
Session 6A: The Distance Scale |
Chair: |
11.00-12.30 |
|
Session 6B: The Transient Sky |
Chair: |
12.15-13.15 |
|
Session 7: Beyond Gaia, Beyond GREAT |
Chair: |
14.45-16.15 |
|
Session QA1: Gaia Science - Extended Q+A session |
09.00-11.00 |
|
Session QA2: Gaia Science - Extended Q+A session |
Chair: |
10.45-11.00 |
C5.1 |
What can Gaia proper motions tell us about Milky Way dwarf galaxies? |
Shoko Jin |
RUG, Groningen, The Netherlands |
|
19.45 |
|
Social Dinner |
14.45-18.00 |
|
Social excursion programme |
13.00-13.15 |
C4.3 |
Galactocentric variation of the abundance structure in the Milky Way stellar disk - results from the Gaia-ESO survey |
Sofia Feltzing |
ASTRO Lund University, Sweden |
|
10.15-10.30 |
C6.2 |
Three-dimensional extinction mapping using Gaussian random fields |
Stuart Sale |
OX Physics, University of Oxford, UK |
|
09.45-10.00 |
E6.2 |
Improving the cosmic distance ladder: distance and structure of the Large Magellanic Cloud |
Tatiana Muraveva (E) |
INAF-Bologna, Italy |
|
14.00–14.10 |
I1.0 |
Welcome |
TBC (University Barcelona), Nicholas Walton (SOC) & Francesca Figueras (LOC) |
|
|
Thursday 4 December 2014 |
14.30–15.00 |
I1.2 |
Gaia Mission Status |
Timo Prusti (I) |
ESTEC, ESA, The Netherlands |
|
13.05–13.15 |
I7.3 |
Closing Words and Final Discussion |
Timo Prusti (I) |
ESTEC, ESA, The Netherlands |
|
13.00-13.15 |
E3.2 |
Physicals models of asteroids from photometric surveys: preparation of Gaia data exploitation |
Toni Santana i Ros (E) |
AMU, Poznam, Poland |
|
12.30-12.45 |
E4.6 |
Open Clusters as Tracers of the Galactic Disk |
Tristan Cantat-Gaudin (E) |
Osservatorio Astrofisico di Padova, Italy |
|
Tuesday 2 December 2014 |
12.45-13.00 |
C3.1 |
Stars with and without planets: Where do they come from? |
Vardan Adibekyan |
CAUP, Porto, Portugal |
|
Wednesday 3 December 2014 |
09.30-10.00 |
I5.2 |
Tick, tock, tick, tock ... |
Wyn Evans (I) |
IoA, Univ. Cambridge, UK |
|
15.00-15.30 |
I5.5 |
From SDSS to Gaia and LSST |
Zeljko Ivezic (I) |
Univesity of Washington, Seattle, USA |
|
Poster ID |
Title |
Author |
Institute |
pdf |
|
|
Carbon stars within the Gaia-ESO survey |
Abia, Carlos |
Universidad de Granada, Spain |
|
|
Stars with and without planets: where do they come from? |
Adibekyan, Vardan |
CAUP, Universidade do Porto, Portugal |
|
|
On the detection of satellite galaxies of the Milky Way with Gaia photometry |
Alzate-Trujillo, Jairo A. |
CRyA, UNAM, Mexico |
|
|
Exploring the orbits of the stars via chemical tagging techniques |
Angiano , Borja |
Macquarie University, Australia |
|
|
Will Gaia see TP-AGB stars in the galactic halo? |
Bruzual, Gustavo |
CRyA, UNAM, Mexico |
|
|
The response of streams to the time-evolution of the galaxy |
Buist, Hans J.T. |
Kapteyn Astronomical Institute, The Netherlands |
|
|
Characterization of the Gaia Photometry |
Carrasco, Josep M. |
ICC-UB / IEEC, Spain |
|
|
The OCCASO survey |
Casamiquela, Laia |
ICC-UB / IEEC, Spain |
|
|
The nearest high-velocity stars revealed by LAMOST data release 1 |
Chen, Li |
SHAO, Shanghai, Xina |
|
|
The TOROS and TORITOS projects |
Diaz, Mario C. |
CGWA, Texas University, USA |
|
|
Optical Cartography of the Northern Galactic Plane with IPHAS |
Farnhill, Hywel |
University of Herfordshire, UK |
|
|
Potential of the Galaxy from the Besançon Galaxy Model including the triaxial bar |
Fernández-Trincado, Jose G. |
UTINAM, Besançon, France |
|
|
The Gaia hybrid catalog: a leverage to find Galactic structures |
Fouesneau, Morgan |
MPIA, Heidelberg, Germany |
|
|
Benchmark stars for cross-calibration of galactic stellar surveys |
Heiter, Ulrike |
Upsala University, Sweden |
|
|
LAMOST Open Clusters survey: current status and perspective |
Hou, Jinliang |
SHAO, Shanghai, Xina |
|
|
Tracing the Sagittarius Tidal Streams in Carbon Long Period Variables |
Huxor, Avon |
ARI, Heidelberg, Germany |
|
|
Time variation of differential reddening towards NGC 4833 |
Itam-Pasquet, Johanna |
LUPM, Montpellier, France |
|
|
Mapping the 'X-shaped Structure' in the Galactic Bulge |
Li, Shao-Yu |
SHAO, Shanghai, Xina |
|
|
Tomography of star-forming regions with VLBI radio interferometers |
Loinard, Laurent |
CRyA, UNAM, Mexico |
|
|
New solar twins and siblings in the ELODIE and SOPHIE archives |
Mahdi, Dhiaa K. |
LAB, Bordeaux, France |
|
|
Metallicity Gradients through Disk Instabilities |
Martínez-Valpuesta, I. |
IAC, Spain |
|
|
The role of the magnetic field in the galactic evolution |
Martos, Marco A. |
UNAM, Mexico |
|
|
Gaia Mission App: developing a mobile application for science outreach |
Masana, Eduard |
ICC-UB / IEEC, Spain |
|
|
The Gaia Object Simulator |
Masana, Eduard |
ICC-UB / IEEC, Spain |
|
|
Detectability of Ultra Faint Dwarf Galaxies with Gaia |
Mateu, Cecilia |
CIDA, Venezuela |
|
|
Constraining the Milky Way IMF using Galactic Cepheids and placing it in the galaxy's zoo |
Mor, Roger |
ICC-UB / IEEC |
|
|
The Milky Way: facts and fiction |
Moreno, Manuel |
UPC, Spain |
|
|
Radial migration and teh properties of the MW disk |
Prantzos, Nikos |
AIP, Paris, France |
|
|
Halo streamers in the Era of Gaia |
Re Fiorentin, Paola |
INAF - Torino, Italy |
|
|
Novel kinematic methods to trace the Spiral Arms nature using Gaia data |
Roca-Fàbrega, Santi |
ICC-UB / IEEC |
|
|
Characterization of the Gaia Red Clump |
Ruiz-Dern, Laura |
Observatoire de Paris-Meudon, France |
|
|
Estimating Gaia's performances for O stars in the Outer Galactic Plane using Herschel data |
Rygl, Kazi |
ESTEC, ESA, The Netherlands |
|
|
Origin of the metallicity distribution in the thick disk |
Sancho-Miranda, Maider |
University of Central Lancashire, UK |
|
|
Bayesian inference of Kinematics and Memberships of Open Clusters |
Shao, Zhengyi |
SHAO, Shanghai, Xina |
|
|
The formation of the Milky Way bulge and its X-shaped structure |
Shen, Juntai |
SHAO, Shanghai, Xina |
|
|
Peening thorugh the dust: Precise astrometry of the Galactic mid-plane with the VVV survey |
Smith, Leigh |
University of Herfordshire, UK |
|
|
VOSA: SED buliding and analysis of thousands of sttars in the framework of Gaia |
Solano, Enrique |
CAB-INTA-CSIC, Spain |
|
|
On the connection between the thick disk and the barred galactic bulge |
Spagna, Alessandro |
INAF - OATo, Italy |
|
|
A stringent limit on the variation in the fine-structure constant from analysis of absorption line multiplets in the early universe |
Thong, Le Duc |
Department of Physics, Vietnam |
|
|
Precise spectrosopic parameters for solar-type stars with moderate-to-high rotation |
Tsantaki, Maria |
CAUP, Porto, Portugal |
|
|
The M giants classification in the LAMOST DR1 |
Zhong, Jing |
SHAO, Shanghai, Xina |
|
|