Data from : The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations

• Other Authors: Claudia Lagos Urbina (Creator), Intl Centre for Radio Astronomy Research (ICRAR) (isManagedBy), Luca Cortese (Creator)
• Format: Dataset
• Language: unknown
• Published: The University of Western Australia
• Subjects: galaxies: evolution; galaxies: formation; galaxies: kinematics and dynamics; galaxies: stellar content; galaxies: structure; cosmology: observations; Astrophysics - Astrophysics of Galaxies; Astrophysics - Cosmology and Nongalactic Astrophysics; Bryant; DuBois; Goodwin; Sande; sami
• Online Access: https://researchdata.edu.au/data-the-sami-hydrodynamical-simulations/1711788

Associated Persons Charlotte Welker (Creator)Jesse Van De Sande (Creator); Joss Bland-Hawthorn (Creator); Felix Schulze (Creator); R.S. Remus (Creator); Yannick M. Bahé (Creator); Sarah Brough (Creator); Julia J. Bryant (Creator); Scott M. Croom (Creator); Julien E. Devriendt (Creator); Y. Dubois (Creator); Michael Goodwin (Creator); Iraklis S. Konstantopoulos (Creator); Jon S. Lawrence (Creator); Anne M. Medling (Creator); Christophe Pichon (Creator); Samuel N. Richards (Creator); Sebastian F. Sanchez (Creator) Cosmological hydrodynamical simulations are rich tools to understand the build-up of stellar mass and angular momentum in galaxies, but require some level of calibration to observations. We compare predictions at z ˜ 0 from the EAGLE, HYDRANGEA, HORIZON-AGN, and MAGNETICUM simulations with integral field spectroscopic (IFS) data from the SAMI (Sydney-AAO Multi-object Integral field spectrograph) Galaxy Survey, ATLAS3D, CALIFA (Calar Alto Legacy Integral Field Area), and MASSIVE surveys. The main goal of this work is to simultaneously compare structural, dynamical, and stellar population measurements in order to identify key areas of success and tension. We have taken great care to ensure that our simulated measurement methods match the observational methods as closely as possible, and we construct samples that match the observed stellar mass distribution for the combined IFS sample. We find that the EAGLE and HYDRANGEA simulations reproduce many galaxy relations but with some offsets at high stellar masses. There are moderate mismatches in Re (+), ɛ (-), σe (-), and mean stellar age (+), where a plus sign indicates that quantities are too high on average, and minus sign too low. The HORIZON-AGN simulations qualitatively reproduce several galaxy relations, but there are a number of properties where we find a quantitative offset to observations. Massive galaxies are better matched to observations than galaxies at low and intermediate masses. Overall, we find mismatches in Re (+), ɛ (-), σe (-), and ...