Reference Information ===================== Provenance for this README -------------------------- * File name: README_astro-tigress.txt * Author: Munan Gong * Date created: 2022-08-11 * Date modified: 2022-09-06 Dataset Version and Release History ----------------------------------- * Current Version: * Number: 1.0 * Date: 2022-09-06 * Persistent identifier: * Prior Versions: * Pre-release version was available at (link not persistent; superseded by version 1.0 above) Dataset Attribution and Usage ----------------------------- * Dataset Title: TIGRESS simulation data * Persistent Identifier: * Dataset Creators: * Chang-Goo Kim * Eve Ostriker * Munan Gong * Jeong-Gyu Kim * Date of Issue: 2022-09-06 * Publisher: Princeton University * License: * Title: Creative Commons Attribution 4.0 International (CC BY 4.0) * Specification: * Suggested Citations: * Dataset citation: > Chang-Goo Kim, Eve Ostriker, Munan Gong, and Jeong-Gyu Kim. 2022. "TIGRESS simulation data." [Dataset] Version 1.0. Princeton University. * Related publications: * If you make use of only the MHD data, please cite: Chang-Goo Kim and Eve C. Ostriker 2017 ApJ 846 133 . * If you make use of chem and/or CO_lines data, please also cite: Munan Gong et al 2018 ApJ 858 16 and Munan Gong et al 2020 ApJ 903 142 . * If you make use of MHD_PI data, please also cite: Erin Kado-Fong et al 2020 ApJ 897 143 . Contact Information ------------------- * Primary Contact: * Name: Chang-Goo Kim * Affiliation: Princeton University * ORCID ID: * Email: changgoo@princeton.edu * Alternative Contact: * Name: Munan Gong * Affiliations: Max Planck Institute for Extraterrestrial Physics; Princeton University * ORCID ID: * Email: munan@princeton.edu - - - Additional Dataset Metadata =========================== Description ----------- > We present the public data release of the TIGRESS (Three-phase Interstellar Medium in > Galaxies Resolving Evolution with Star Formation and Supernova Feedback) simulations. > This release includes simulations representing the solar neighborhood environment at > spatial resolutions of 2 and 4 pc. The original magneto-hydrodynamic simulation data > is published along with data products from post-processing, including chemistry, CO > emission line, and photoionization (HII regions). Acknowledgements ---------------- * Funding sources: * Grants AST-1312006 and AST-1713949 from the National Science Foundation * Grants NNX14AB49G and NNX17AG26G from NASA * Grant CCA528307 from the Simons Foundation * Lyman Spitzer Jr. Postdoctoral Fellowship at Princeton University * The EACOA Fellowship awarded by the East Asia Core Observatories Association * Institutional sponsors: * Princeton University * Flatiron Institute * The Max Planck Institute for Extraterrestrial Physics * Other sources of support: > Simulations were performed on the computational resources supported by the PICSciE > TIGRESS High Performance Computing Center at Princeton University, the NASA > High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) > Division at Ames Research Center, and the National Energy Research Scientific > Computing Center, which is supported by the Office of Science of the U.S. > Department of Energy under Contract No. DE-AC02-05CH11231. Relations to Other Datasets and/or Publications ----------------------------------------------- * Other publicly accessible locations of the same data: * (link not maintained as of 2022-09-06) * Further documentation and usage examples: * * * Corresponding publications: * Chang-Goo Kim and Eve C. Ostriker 2017 ApJ 846 133 * Munan Gong et al 2018 ApJ 858 16 * Munan Gong et al 2020 ApJ 903 142 * Erin Kado-Fong et al 2020 ApJ 897 143 - - - Data and File Overview ====================== Summary Metrics --------------- * File count: 206 files (262 directories) * Total file size: 1.07 TB * Range of individual file sizes: 81 B to 33.8 GB * File formats: [no extension] (3), .athdf (33), .bout (66), .chem (1), .hst (2), .par (2), .py (3), .vtk (64), .xdmf (33) Data Types ---------- * MHD: Small box (z=+-512 pc) original TIGRESS output for MHD variables including density, pressure, velocity (vector), and magnetic field (vector). Athena VTK format. * MHD_PI: Full box (z=+-3072 pc) MHD data plus electron abundance as a result of UV radiation post-processing. Athena VTK format. * chem: The chemistry post-processing small box output for molecular hydrogen and CO abundnaces. Athena++ HDF5 format. * CO_lines: The CO lines, J(1-0) and J(2-1). RADMC-3D binary format. Note that the chemistry post-processing data is only available for R8-2pc. Table of Contents ----------------- R8_2pc R8_2pc\0290 R8_2pc\0290\chem R8_2pc\0290\chem\Z05 R8_2pc\0290\chem\Z1 R8_2pc\0290\chem\Z2 R8_2pc\0290\CO_lines R8_2pc\0290\CO_lines\Z05 R8_2pc\0290\CO_lines\Z05\il1 R8_2pc\0290\CO_lines\Z05\il2 R8_2pc\0290\CO_lines\Z1 R8_2pc\0290\CO_lines\Z1\il1 R8_2pc\0290\CO_lines\Z1\il2 R8_2pc\0290\CO_lines\Z2 R8_2pc\0290\CO_lines\Z2\il1 R8_2pc\0290\CO_lines\Z2\il2 R8_2pc\0290\MHD R8_2pc\0290\MHD_PI R8_2pc\0300 R8_2pc\0300\chem R8_2pc\0300\chem\Z05 R8_2pc\0300\chem\Z1 R8_2pc\0300\chem\Z2 R8_2pc\0300\CO_lines R8_2pc\0300\CO_lines\Z05 R8_2pc\0300\CO_lines\Z05\il1 R8_2pc\0300\CO_lines\Z05\il2 R8_2pc\0300\CO_lines\Z1 R8_2pc\0300\CO_lines\Z1\il1 R8_2pc\0300\CO_lines\Z1\il2 R8_2pc\0300\CO_lines\Z2 R8_2pc\0300\CO_lines\Z2\il1 R8_2pc\0300\CO_lines\Z2\il2 R8_2pc\0300\MHD R8_2pc\0300\MHD_PI R8_2pc\0310 R8_2pc\0310\chem R8_2pc\0310\chem\Z05 R8_2pc\0310\chem\Z1 R8_2pc\0310\chem\Z2 R8_2pc\0310\CO_lines R8_2pc\0310\CO_lines\Z05 R8_2pc\0310\CO_lines\Z05\il1 R8_2pc\0310\CO_lines\Z05\il2 R8_2pc\0310\CO_lines\Z1 R8_2pc\0310\CO_lines\Z1\il1 R8_2pc\0310\CO_lines\Z1\il2 R8_2pc\0310\CO_lines\Z2 R8_2pc\0310\CO_lines\Z2\il1 R8_2pc\0310\CO_lines\Z2\il2 R8_2pc\0310\MHD R8_2pc\0310\MHD_PI R8_2pc\0320 R8_2pc\0320\chem R8_2pc\0320\chem\Z05 R8_2pc\0320\chem\Z1 R8_2pc\0320\chem\Z2 R8_2pc\0320\CO_lines R8_2pc\0320\CO_lines\Z05 R8_2pc\0320\CO_lines\Z05\il1 R8_2pc\0320\CO_lines\Z05\il2 R8_2pc\0320\CO_lines\Z1 R8_2pc\0320\CO_lines\Z1\il1 R8_2pc\0320\CO_lines\Z1\il2 R8_2pc\0320\CO_lines\Z2 R8_2pc\0320\CO_lines\Z2\il1 R8_2pc\0320\CO_lines\Z2\il2 R8_2pc\0320\MHD R8_2pc\0320\MHD_PI R8_2pc\0330 R8_2pc\0330\chem R8_2pc\0330\chem\Z05 R8_2pc\0330\chem\Z1 R8_2pc\0330\chem\Z2 R8_2pc\0330\CO_lines R8_2pc\0330\CO_lines\Z05 R8_2pc\0330\CO_lines\Z05\il1 R8_2pc\0330\CO_lines\Z05\il2 R8_2pc\0330\CO_lines\Z1 R8_2pc\0330\CO_lines\Z1\il1 R8_2pc\0330\CO_lines\Z1\il2 R8_2pc\0330\CO_lines\Z2 R8_2pc\0330\CO_lines\Z2\il1 R8_2pc\0330\CO_lines\Z2\il2 R8_2pc\0330\MHD R8_2pc\0330\MHD_PI R8_2pc\0340 R8_2pc\0340\chem R8_2pc\0340\chem\Z05 R8_2pc\0340\chem\Z1 R8_2pc\0340\chem\Z2 R8_2pc\0340\CO_lines R8_2pc\0340\CO_lines\Z05 R8_2pc\0340\CO_lines\Z05\il1 R8_2pc\0340\CO_lines\Z05\il2 R8_2pc\0340\CO_lines\Z1 R8_2pc\0340\CO_lines\Z1\il1 R8_2pc\0340\CO_lines\Z1\il2 R8_2pc\0340\CO_lines\Z2 R8_2pc\0340\CO_lines\Z2\il1 R8_2pc\0340\CO_lines\Z2\il2 R8_2pc\0340\MHD R8_2pc\0340\MHD_PI R8_2pc\0350 R8_2pc\0350\chem R8_2pc\0350\chem\Z05 R8_2pc\0350\chem\Z1 R8_2pc\0350\chem\Z2 R8_2pc\0350\CO_lines R8_2pc\0350\CO_lines\Z05 R8_2pc\0350\CO_lines\Z05\il1 R8_2pc\0350\CO_lines\Z05\il2 R8_2pc\0350\CO_lines\Z1 R8_2pc\0350\CO_lines\Z1\il1 R8_2pc\0350\CO_lines\Z1\il2 R8_2pc\0350\CO_lines\Z2 R8_2pc\0350\CO_lines\Z2\il1 R8_2pc\0350\CO_lines\Z2\il2 R8_2pc\0350\MHD R8_2pc\0350\MHD_PI R8_2pc\0360 R8_2pc\0360\chem R8_2pc\0360\chem\Z05 R8_2pc\0360\chem\Z1 R8_2pc\0360\chem\Z2 R8_2pc\0360\CO_lines R8_2pc\0360\CO_lines\Z05 R8_2pc\0360\CO_lines\Z05\il1 R8_2pc\0360\CO_lines\Z05\il2 R8_2pc\0360\CO_lines\Z1 R8_2pc\0360\CO_lines\Z1\il1 R8_2pc\0360\CO_lines\Z1\il2 R8_2pc\0360\CO_lines\Z2 R8_2pc\0360\CO_lines\Z2\il1 R8_2pc\0360\CO_lines\Z2\il2 R8_2pc\0360\MHD R8_2pc\0360\MHD_PI R8_2pc\0370 R8_2pc\0370\chem R8_2pc\0370\chem\Z05 R8_2pc\0370\chem\Z1 R8_2pc\0370\chem\Z2 R8_2pc\0370\CO_lines R8_2pc\0370\CO_lines\Z05 R8_2pc\0370\CO_lines\Z05\il1 R8_2pc\0370\CO_lines\Z05\il2 R8_2pc\0370\CO_lines\Z1 R8_2pc\0370\CO_lines\Z1\il1 R8_2pc\0370\CO_lines\Z1\il2 R8_2pc\0370\CO_lines\Z2 R8_2pc\0370\CO_lines\Z2\il1 R8_2pc\0370\CO_lines\Z2\il2 R8_2pc\0370\MHD R8_2pc\0370\MHD_PI R8_2pc\0380 R8_2pc\0380\chem R8_2pc\0380\chem\Z05 R8_2pc\0380\chem\Z1 R8_2pc\0380\chem\Z2 R8_2pc\0380\CO_lines R8_2pc\0380\CO_lines\Z05 R8_2pc\0380\CO_lines\Z05\il1 R8_2pc\0380\CO_lines\Z05\il2 R8_2pc\0380\CO_lines\Z1 R8_2pc\0380\CO_lines\Z1\il1 R8_2pc\0380\CO_lines\Z1\il2 R8_2pc\0380\CO_lines\Z2 R8_2pc\0380\CO_lines\Z2\il1 R8_2pc\0380\CO_lines\Z2\il2 R8_2pc\0380\MHD R8_2pc\0380\MHD_PI R8_2pc\0390 R8_2pc\0390\chem R8_2pc\0390\chem\Z05 R8_2pc\0390\chem\Z1 R8_2pc\0390\chem\Z2 R8_2pc\0390\CO_lines R8_2pc\0390\CO_lines\Z05 R8_2pc\0390\CO_lines\Z05\il1 R8_2pc\0390\CO_lines\Z05\il2 R8_2pc\0390\CO_lines\Z1 R8_2pc\0390\CO_lines\Z1\il1 R8_2pc\0390\CO_lines\Z1\il2 R8_2pc\0390\CO_lines\Z2 R8_2pc\0390\CO_lines\Z2\il1 R8_2pc\0390\CO_lines\Z2\il2 R8_2pc\0390\MHD R8_2pc\0390\MHD_PI R8_2pc\history R8_2pc\history\MHD R8_2pc\input R8_2pc\input\chem R8_2pc\input\CO_lines R8_2pc\input\MHD R8_4pc R8_4pc\0200 R8_4pc\0200\MHD R8_4pc\0200\MHD_PI R8_4pc\0210 R8_4pc\0210\MHD R8_4pc\0210\MHD_PI R8_4pc\0220 R8_4pc\0220\MHD R8_4pc\0220\MHD_PI R8_4pc\0230 R8_4pc\0230\MHD R8_4pc\0230\MHD_PI R8_4pc\0240 R8_4pc\0240\MHD R8_4pc\0240\MHD_PI R8_4pc\0250 R8_4pc\0250\MHD R8_4pc\0250\MHD_PI R8_4pc\0260 R8_4pc\0260\MHD R8_4pc\0260\MHD_PI R8_4pc\0270 R8_4pc\0270\MHD R8_4pc\0270\MHD_PI R8_4pc\0280 R8_4pc\0280\MHD R8_4pc\0280\MHD_PI R8_4pc\0290 R8_4pc\0290\MHD R8_4pc\0290\MHD_PI R8_4pc\0300 R8_4pc\0300\MHD R8_4pc\0300\MHD_PI R8_4pc\0310 R8_4pc\0310\MHD R8_4pc\0310\MHD_PI R8_4pc\0320 R8_4pc\0320\MHD R8_4pc\0320\MHD_PI R8_4pc\0330 R8_4pc\0330\MHD R8_4pc\0330\MHD_PI R8_4pc\0340 R8_4pc\0340\MHD R8_4pc\0340\MHD_PI R8_4pc\0350 R8_4pc\0350\MHD R8_4pc\0350\MHD_PI R8_4pc\0360 R8_4pc\0360\MHD R8_4pc\0360\MHD_PI R8_4pc\0370 R8_4pc\0370\MHD R8_4pc\0370\MHD_PI R8_4pc\0380 R8_4pc\0380\MHD R8_4pc\0380\MHD_PI R8_4pc\0390 R8_4pc\0390\MHD R8_4pc\0390\MHD_PI R8_4pc\0400 R8_4pc\0400\MHD R8_4pc\0400\MHD_PI R8_4pc\history R8_4pc\history\MHD R8_4pc\input R8_4pc\input\MHD Setup ----- See instructions at - - - END OF README