SimSpin v2.6.0 - Constructing synthetic spectral IFU cubes for comparison with observational surveys

• Published in: Publications of the Astronomical Society of Australia
• Main Authors: Harborne, K. E., Serene, A., Davies, E. J. A., Derkenne, C., Vaughan, S., Burdon, A. I., Lagos, C. del P., McDermid, R., O'Toole, S., Power, C., Robotham, A. S. G., Santucci, G., Tobar, R.
• Format: Article in Journal/Newspaper
• Language: English
• Published: 2023
• Subjects: Virtual observatory tools; galaxies: evolution; galaxy: kinematics; methods: numerical; sami
• Online Access: https://researchers.mq.edu.au/en/publications/30cc9795-4797-4927-b966-7b8328286eed; https://doi.org/10.1017/pasa.2023.47; https://research-management.mq.edu.au/ws/files/303897789/298359452.pdf; http://www.scopus.com/inward/record.url?scp=85171276003&partnerID=8YFLogxK; http://purl.org/au-research/grants/arc/DP210101945

In this work, we present a methodology and a corresponding code-base for constructing mock integral field spectrograph (IFS) observations of simulated galaxies in a consistent and reproducible way. Such methods are necessary to improve the collaboration and comparison of observation and theory results, and accelerate our understanding of how the kinematics of galaxies evolve over time. This code, SimSpin, is an open-source package written in R, but also with an API interface such that the code can be interacted with in any coding language. Documentation and individual examples can be found at the open-source website connected to the online repository. SimSpin is already being utilised by international IFS collaborations, including SAMI and MAGPI, for generating comparable data sets from a diverse suite of cosmological hydrodynamical simulations.