Published April 10, 2020
| Version
v1
Dataset
Open
MUGS Initial Conditions
Creators
Description
The McMaster Unbiased Galaxy Simulations (MUGS) are a series of cosmological zoom-in simulations of L* galaxies (such as the Milky Way), chosen randomly to allow an unbiased sample in spin parameter and merger history. They were first presented in Bailin et al. 2010 "Consequences of Cosmic Microwave Background-Regulated Star Formation" and Stinson et al. 2014 "Cosmological Galaxy Formation Simulations Using SPH". These are the initial conditions for those simulations, in the Tipsy format used by the ChaNGa and gasoline codes.
The units for the IC are as follows:
Length: 68493.2 kpc
Mass: 4.7526e16 kpc
The periodic box size should be set to 1 in code units.
Files
Files
(5.0 GB)
| Name | Size | Download all |
|---|---|---|
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Checksum: md5:a793e79bda1bf78a7b2bce0c545f57ae
PID: http://hdl.handle.net/11304/cbb44ec1-fc9c-4927-a934-e25f24e112b2 |
265.2 MB | Download |
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Checksum: md5:cf9740c9df02e8a4da9c16dc892170f9
PID: http://hdl.handle.net/11304/39108fdb-3462-415c-af74-b9f3c9296b45 |
374.5 MB | Download |
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Checksum: md5:e22ad148e39925cb7cb91ce109520fd9
PID: http://hdl.handle.net/11304/ab8be895-f6e8-4e67-a014-dff97985db30 |
267.4 MB | Download |
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Checksum: md5:1ec8c51d467810a1d226a8064154440d
PID: http://hdl.handle.net/11304/999842b3-f202-466a-9dbd-0c7522758297 |
210.1 MB | Download |
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Checksum: md5:c3de6bd80f73872b5845b80b18079f9b
PID: http://hdl.handle.net/11304/cb0ea9d8-fb04-4017-aa25-09b265fa9074 |
239.9 MB | Download |
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Checksum: md5:c22af2900fc91296bc94bc91bb639751
PID: http://hdl.handle.net/11304/f412836a-2bdb-4f64-8e4c-4e587996efe3 |
207.6 MB | Download |
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Checksum: md5:1df6ce70b9bf573667e24a98add6ad84
PID: http://hdl.handle.net/11304/33001e49-0ea0-426d-ad02-7a181b8e2e3b |
365.3 MB | Download |
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Checksum: md5:318accddb6c0366f12d9a96a628b2b04
PID: http://hdl.handle.net/11304/9eae0d2e-3b3a-44c4-b620-1286ce68f656 |
260.0 MB | Download |
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Checksum: md5:481abebd04307bdc44a575191dae3b4d
PID: http://hdl.handle.net/11304/3ba104c3-9f2a-4189-9247-c6e6f7b87161 |
460.2 MB | Download |
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Checksum: md5:b95280b2a95b0187a56bb04ad7f84ae8
PID: http://hdl.handle.net/11304/2a7d8360-193c-42b7-97da-ae54b42ad6e8 |
226.3 MB | Download |
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Checksum: md5:08c0a9b15a8b0ea09322b4cf1a4b51c8
PID: http://hdl.handle.net/11304/63365ad1-5ff9-4b63-84c9-30633dce92a4 |
168.2 MB | Download |
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Checksum: md5:448e1fce63042cd9bee4cd0c9df65f0b
PID: http://hdl.handle.net/11304/8065b713-50e2-48c3-a8b8-7563a152dbd6 |
337.1 MB | Download |
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Checksum: md5:9bbce76bcba556944e56ad24993311f9
PID: http://hdl.handle.net/11304/506208d0-0449-4345-8f7e-f9e74b2828a0 |
324.7 MB | Download |
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Checksum: md5:2c4fd18fcc5219bba6634461ebe01e75
PID: http://hdl.handle.net/11304/03899f50-1801-427c-91bb-a8488cb84759 |
445.8 MB | Download |
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Checksum: md5:9132efd5670f8f5a55c7f3759e02a4f8
PID: http://hdl.handle.net/11304/ea106bc4-1dca-428f-b492-de16e7b05fda |
248.2 MB | Download |
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Checksum: md5:d01f2ab923a65aa4f2c47d45eba74324
PID: http://hdl.handle.net/11304/c7dc966b-4948-43b4-94f7-919ef27f6ec9 |
203.1 MB | Download |
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Checksum: md5:43468c68b2a72a560a7179f08e130bb2
PID: http://hdl.handle.net/11304/583047b3-7cb1-47ab-a540-5653424c28e6 |
362.2 MB | Download |
Additional details
Identifiers
- b2rec
- 479e2cc6b33340f1ad9a771763000beb
- b2rec
- 8caf186b92d34cd2bcce37e6f73c6efc