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Synthetic Gaia surveys from the FIRE cosmological simulations of Milky-Way-mass galaxies

Sanderson, Robyn E. and Wetzel, Andrew and Loebman, Sarah and Sharma, Sanjib and Hopkins, Philip F. and Garrison-Kimmel, Shea and Faucher-Giguère, Claude-André and Kereš, Dušan and Quataert, Eliot (2018) Synthetic Gaia surveys from the FIRE cosmological simulations of Milky-Way-mass galaxies. . (Unpublished) http://resolver.caltech.edu/CaltechAUTHORS:20190206-105555952

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Abstract

With Gaia Data Release 2, the astronomical community is entering a new era of multidimensional surveys of the Milky Way. This new phase-space view of our Galaxy demands new tools for comparing observations to simulations of Milky-Way-mass galaxies in a cosmological context, to test the physics of both dark matter and galaxy formation. We present ananke, a framework for generating synthetic phase-space surveys from high-resolution baryonic simulations, and we use ananke to generate a suite of synthetic surveys designed to resemble Gaia DR2 in data structure, magnitude limits, and observational errors. We use three cosmological simulations of Milky-Way-mass galaxies from the Latte suite of the Feedback In Realistic Environments (FIRE) project, which offer many advantages for generating synthetic stellar surveys: self-consistent clustering of star formation in dense molecular clouds, thin stellar and gaseous disks, cosmological accretion and enrichment histories, all in live cosmological halos with satellite dwarf galaxies and stellar halos. We select three solar viewpoints from each simulation to generate nine synthetic Gaia-like surveys. We generate synthetic stars assuming that each simulation’s star particles (of mass 7070 M_⊙ ) represent a single stellar population, and we use a kernel density representation to distribute synthetic stars accurately in position and velocity. At each viewpoint, we compute a self-consistent dust extinction map, using the gas metallicity distribution in each simulation. Finally, we apply a simple error model to produce a synthetic Gaia-like survey at each solar viewpoint, though we also provide quantities without error convolution. This results in a catalog of synthetic stars, as if measured by Gaia, that includes both observational properties and a pointer to each generating star particle in the simulation. We also provide the complete snapshot–including star, gas, and dark matter particles–at z = 0 for each simulated galaxy. We describe data access points, the data model, and plans for future upgrades to ananke. These synthetic surveys provide a tool for the scientific community to test analysis methods and interpret Gaia data.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1806.10564arXivDiscussion Paper
http://ananke.hub.yt/Related ItemData
http://fire.northwestern.edu/anankeRelated ItemMore information and updates
ORCID:
AuthorORCID
Sanderson, Robyn E.0000-0003-3939-3297
Wetzel, Andrew0000-0003-0603-8942
Sharma, Sanjib0000-0002-0920-809X
Hopkins, Philip F.0000-0003-3729-1684
Garrison-Kimmel, Shea0000-0002-4655-8128
Kereš, Dušan0000-0002-1666-7067
Quataert, Eliot0000-0001-9185-5044
Additional Information:The authors thank Justin Howell and Vandana Desai of IPAC, Kacper Kowalik and Matt Turk of yt, and Mark Bartelt at Caltech for their crucial assistance with the public data releases. We thank Anthony Brown for discussions on the characteristics of Gaia DR2 and Julianne Dalcanton for advice on models of dust extinction. This work grew out of two series of Gaia preparatory meetings focused on data analysis challenges. First, the Gaia Challenge Workshops (held 2011–2015), which were organized through the Gaia Research for European Astronomy Training Initial Training Network programme supported by the European Commission through its FP7 Marie Curie programme under grant agreement 264895. Second, the Gaia Sprints (held 2016–present). Code for 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. RES was supported by an NSF Astronomy & Astrophysics Postdoctoral Fellowship under grant AST-1400989, and by NASA through grant JPL 1589742. AW was supported by NASA through ATP grant 80NSSC18K1097 and grants HST-GO-14734 and HST-AR-15057 via STScI. Support for SL was provided by NASA through Hubble Fellowship grant HST-JF2-51395.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. Support for PFH was provided by an Alfred P. Sloan Research Fellowship, NSF Collaborative Research Grant #1715847 and CAREER grant #1455342, and NASA grants NNX15AT06G, and JPL 1589742. Support for SGK was provided by NASA through Einstein Postdoctoral Fellowship grant number PF5-160136 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060. CAFG was supported by NSF through grants AST-1412836, AST-1517491, AST-1715216, and CAREER award AST-1652522, by NASA through grant NNX15AB22G, and by a Cottrell Scholar Award from the Research Corporation for Science Advancement. DK was supported by NSF grant AST-1715101 and the Cottrell Scholar Award from the Research Corporation for Science Advancement. EQ was supported by a Simons Investigator Award from the Simons Foundation and by NSF grant AST-1715070. Numerical calculations were run on the Caltech compute cluster “Wheeler,” allocations from XSEDE TG-AST130039 and PRAC NSF.1713353 supported by the NSF, NASA HEC SMD-16-7592, and the High Performance Computing at Los Alamos National Lab. Software: matplotlib (Hunter 2007), scipy (Jones et al. 2001), astropy (The Astropy Collaboration et al. 2018), qhull (Barber et al. 1996), galaxia (Sharma et al. 2011), enlink (Sharma & Johnston 2009).
Group:TAPIR
Funders:
Funding AgencyGrant Number
Marie Curie Fellowship264895
Gaia Multilateral AgreementUNSPECIFIED
NSF Astronomy and Astrophysics FellowshipAST-1400989
JPL1589742
NASA80NSSC18K1097
NASAHST-GO-14734
NASAHST-AR-15057
NASA Hubble FellowshipHST-JF2-51395.001-A
NASANAS5-26555
Alfred P. Sloan FoundationUNSPECIFIED
NSFAST-1715847
NSFAST-1455342
NASANNX15AT06G
NASA Einstein FellowshipPF5-160136
NASANAS8-03060
NSFAST-1412836
NSFAST-1517491
NSFAST-1715216
NSFAST-1652522
NASANNX15AB22G
Cottrell Scholar of Research CorporationUNSPECIFIED
NSFAST-1715101
Simons FoundationUNSPECIFIED
NSFAST-1715070
NSFTG-AST130039
NSFOAC-1713353
NASASMD-16-7592
Record Number:CaltechAUTHORS:20190206-105555952
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190206-105555952
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92718
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:08 Feb 2019 18:44
Last Modified:22 Mar 2019 20:53

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