2017 Heidelberg Gaia Sprint
This page preserves the history from the 2017 Heidelberg Gaia Sprint,
which took place 2017 July 17 through 21 at the
Internationales
Wissenschaftsforum Heidelberg.
Results
Before and during the meeting, we kept jointly edited
2017 HD Gaia Sprint Running Notes
that gathered information about homework solutions, intended projects,
and breakouts.
On the first day, all participants
presented a slide from the jointly edited
2017 HD Gaia Sprint Pitch Slides to introduce themselves, their skills, expertise,
and their ideas for the week.
On the last day, the wrap up was given from a jointly edited set of
2017 HD Gaia Sprint Wrap-up Slides,
which summarize the accomplishments made throughout the week.
The 2017 HD Gaia Sprint has in part resulted in the following publications:
- Mapping young stellar populations toward Orion with Gaia DR1, Zari, E., Brown, A. G. A., de Bruijne, J., Manara, C. F. and de Zeeuw, P. T.
- The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS, Buder, S. et al.
- Dynamical heating across the Milky Way disc using APOGEE and $\it{Gaia}$, Mackereth, J. Ted et al.
- Metallicity dependence of the Hercules stream in Gaia/RAVE data - explanation by non-closed orbits, Kohei Hattori, Naoteru Gouda, Taihei Yano, Nobuyuki Sakai, Hiromichi Tagawa, Junichi Baba, Jun Kumamoto
- Synthetic Gaia surveys from the FIRE cosmological simulations of Milky Way-mass galaxies, Robyn E. Sanderson, Andrew Wetzel, Sarah Loebman, Sanjib Sharma, Philip F. Hopkins, Shea Garrison-Kimmel, Claude-Andre Faucher-Giguere, Dusan Keres, Eliot Quataert
- Chemo-dynamical clustering applied to APOGEE data: Re-discovering globular clusters, Boquan Chen, Elena D'Onghia, Stephen A. Pardy, Anna Pasquali, Clio Bertelli Motta, Bret Hanlon, Eva K. Grebel
- Spectroscopic confirmation of very-wide stellar binaries and large-separation comoving pairs from Gaia DR1, Adrian M. Price-Whelan, Semyeong Oh, David N. Spergel
- New and Known Moving Groups And Clusters Identified in a Gaia Co-Moving Catalog, Jacqueline K. Faherty, John J. Bochanski, Johnathan Gagne, Olivia Nelson, Kristina Coker, Iliya Smithka, Deion Desir, Chelsea Vasquez
- Photospheric Diagnostics of core helium burning in giant stars, Keith Hawkins, Yuan-Sen Ting, Hans-Walter Rix
- A large and pristine sample of standard candles across the Milky Way: ~100,000 red clump stars with 3% contamination, Y. S. Ting, K. Hawkins, H.-W. Rix
- Searching for the fastest stars in the Galaxy, T. Marchetti, E. M. Rossi, A. G. A. Brown
- Unbiased TGASxLAMOST distances and the role of binarity, J. Coronado, H.-W. Rix, W. H. Trick
- New members of nearby young associations from Gaia-Tycho data, J. Gagne, O. Roy-Loubier, J. Faherty, R. Doyon, L. Malo
- A Gaia DR2 Mock Stellar Catalog, J. Rybizki, M. Delmeitner, M. Fouesneau, C. Bailer-Jones, H.-W. Rix, R. Andrae
- The BANYAN multivariate Bayesian algorithm to identify members of young associations within 150 pc, J. Gagne, E. Mamajek, L. Malo, A. Riedel, D. Rodriguez, D. Lafreniere, J. Faherty, O. Roy-Loubier, L. Pueyo, A. Robin, R. Doyon
- Mapping young stellar populations towards Orion with Gaia DR1, E. Zari, A. G. A. Brown, J. de Bruijne, C. F. Manara, P. T. de Zeeuw
- Discovery and Characterization of 3000+ Main-Sequence Binaries from APOGEE Spectra, K. El-Badry, Y.-S. Ting, H.-W. Rix, E. Quataert, D. R. Weisz, P. Cargile, C. Conroy, D. W. Hogg, M. Bergemann, C. Liu
- Precise ages of field stars from white dwarf companions, M. Fouesneau, H.-W. Rix, T. von Hippel, D. W. Hogg, H. Tian
Scientific Organizing Committee
- Ana Bonaca (Harvard)
- Andy Casey (Monash)
- David W. Hogg (NYU) (MPIA) (Flatiron), Organizing Committee Chair
- Adrian Price-Whelan (Princeton)
- Hans-Walter Rix (MPIA)
- David Spergel (Flatiron) (Princeton)
- Wilma Trick (MPIA)
Local Organizing Committee
- Sven Buder (MPIA)
- Johanna Coronado (MPIA)
- Carola Jordan (MPIA)
Acknowledgements
We ask that any publications that were started or worked on
during this Gaia Sprint include the following acknowledgements:
This project was developed in part
at the 2017 Heidelberg Gaia Sprint,
hosted by the Max-Planck-Institut für Astronomie,
Heidelberg.
This work has made use of data from
the European Space Agency (ESA) mission Gaia
(http://www.cosmos.esa.int/gaia), processed by the Gaia Data
Processing and Analysis Consortium (DPAC,
http://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for
the DPAC has been provided by national institutions, in particular
the institutions participating in the Gaia Multilateral Agreement.
Previous events: