Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
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Author(s)
Safarzadeh, Mohammadtaher
Ji, Alexander P
Dooley, Gregory Alan
Frebel, Anna L.
Scannapieco, Evan
Gómez, Facundo A
O'Shea, Brian W
Date Issued
June 2018
Journal
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP)
Citation
Safarzadeh, Mohammadtaher et al. “Selecting Ultra-Faint Dwarf Candidate Progenitors in Cosmological N-Body Simulations at High Redshifts.” Monthly Notices of the Royal Astronomical Society 476, 4 (March 2018): 5006–5015 © The Author(s)
Version
Author's final manuscript
Abstract
The smallest satellites of the Milky Way ceased forming stars during the epoch of reionization and thus provide archaeological access to galaxy formation at z > 6. Numerical studies of these ultrafaint dwarf galaxies (UFDs) require expensive cosmological simulations with high mass resolution that are carried out down to z = 0. However, if we are able to statistically identify UFD host progenitors at high redshifts with relatively high probabilities, we can avoid this high computational cost. To find such candidates, we analyse the merger trees of Milky Way type haloes from the high-resolution Caterpillar suite of dark matter only simulations. Satellite UFD hosts at z = 0 are identified based on four different abundance matching (AM) techniques. All the haloes at high redshifts are traced forward in time in order to compute the probability of surviving as satellite UFDs today. Our results show that selecting potential UFD progenitors based solely on their mass at z = 12 (8) results in a 10 per cent (20 per cent) chance of obtaining a surviving UFD at z = 0 in three of the AM techniques we adopted. We find that the progenitors of surviving satellite UFDs have lower virial ratios (η), and are preferentially located at large distances from the main MW progenitor, while they show no correlation with concentration parameter. Haloes with favorable locations and virial ratios are ≈3 times more likely to survive as satellite UFD candidates at z = 0. Keywords: galaxies: dwarf, Local Group, galaxies: statistics
MIT Department
Massachusetts Institute of Technology. Department of Physics
MIT Kavli Institute for Astrophysics and Space Research
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DOI of Published Version
https://doi.org/10.1093/MNRAS/STY595
