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Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations

Authors :
Azadeh Fattahi
Alis J. Deason
Shaun Cole
Dandan Xu
Christine M. Simpson
Facundo A. Gómez
John C. Helly
Marius Cautun
Andrew Cooper
Volker Springel
Jason A. S. Hunt
Federico Marinacci
Rüdiger Pakmor
Carlos S. Frenk
Robert J. J. Grand
Grand, Robert J.J.
Helly, John
Fattahi, Azadeh
Cautun, Mariu
Cole, Shaun
Cooper, Andrew P.
Deason, Alis J.
Frenk, Carlo
Gómez, Facundo A.
Hunt, Jason A.S.
Marinacci, Federico
Pakmor, Rüdiger
Simpson, Christine M.
Springel, Volker
Xu, Dandan
Source :
Monthly Notices of the Royal Astronomical Society, Monthly notices of the Royal Astronomical Society, 2018, Vol.481(2), pp.1726-1743 [Peer Reviewed Journal]
Publication Year :
2018

Abstract

We present and analyse mock stellar catalogues that match the selection criteria and observables (including uncertainties) of the Gaia satellite data release 2 (DR2). The source are six cosmological high-resolution magneto-hydrodynamic $\Lambda$CDM zoom simulations of the formation of Milky Way analogues from the AURIGA project. Mock data are provided for stars with $V < 16$ mag, and $V < 20$ mag at $|b|>20$ degrees. The mock catalogues are made using two different methods: the public SNAPDRAGONS code, and a method based on that of Lowing et al. that preserves the phase-space distribution of the model stars. These publicly available catalogues contain 5-parameter astrometry, radial velocities, multi-band photometry, stellar parameters, dust extinction values, and uncertainties in all these quantities. In addition, we provide the gravitational potential and information on the origin of each star. By way of demonstration, we apply the mock catalogues to analyses of the young stellar disc and the stellar halo. We show that: i) the young outer stellar disc exhibits a flared distribution that is detectable in the height and vertical velocity distribution of A- and B-dwarf stars up to radii of ~15 kpc; and ii) the spin of the stellar halo out to 100 kpc can be accurately measured with Gaia DR2 RR Lyrae stars. These catalogues are well suited for comparisons with observations and should help to: i) develop and test analysis methods for the Gaia DR2 data; ii) gauge the limitations and biases of the data and iii) interpret the data in the light of theoretical predictions from realistic $ab$ $initio$ simulations of galaxy formation in the $\Lambda$CDM cosmological model.<br />Comment: Accepted for publication in MNRAS (1st of September, 2018) after improvements to several figures and some discussion. The mock data are available for access and download at http://icc.dur.ac.uk/data and documentation and supplementary material is available at http://auriga.h-its.org/gaiamock.html

Details

Language :
English
Database :
OpenAIRE
Journal :
Monthly Notices of the Royal Astronomical Society, Monthly notices of the Royal Astronomical Society, 2018, Vol.481(2), pp.1726-1743 [Peer Reviewed Journal]
Accession number :
edsair.doi.dedup.....4c93d9826ba3c4281b474103e5d3d913