People & Credits#

Contributors#

  • Susmita Adhikari (India Institute of Science and Research)

  • Arka Banerjee (India Institute of Science and Research)

  • Andrew Benson (Carnegie Observatories)

  • Elise Darragh-Ford (KIPAC, Stanford University & SLAC National Accelerator Laboratory)

  • Xiaolong Du (Carnegie Observatories)

  • BrynĂ© Hadnott (KIPAC, Stanford University & SLAC National Accelerator Laboratory)

  • Philip Mansfield (KIPAC, Stanford University & SLAC National Accelerator Laboratory)

  • Yao-Yuan Mao (University of Utah & Rutgers)

  • Ethan O. Nadler (Carnegie Observatories, & USC)

  • Sebastian Wagner-Carena (KIPAC, Stanford University & SLAC National Accelerator Laboratory)

  • Yunchong Wang (KIPAC, Stanford University & SLAC National Accelerator Laboratory)

  • Risa Wechsler (KIPAC, Stanford University & SLAC National Accelerator Laboratory)

  • Hao-Yi Wu (Boise State Univeristy)

Citing Symphony#

Symphony and its data products have been collected from a number of distinct research efforts, some of which predate Symphony. Because of this, appropriate citation depends on which data is used. We ask that all works which use Symphony data cite Nadler et al. (in press) and add the following to to their acknowledgements:

This work used data from the Symphony suite of simulations (http://web.stanford.edu/group/gfc/symphony/), which was supported by the Kavli Institute for Particle Astrophysics and Cosmology at Stanford University and SLAC National Accelerator Laboratory, and by the U.S. Department of Energy under contract number DE-AC02-76SF00515 to SLAC National Accelerator Laboratory.

Three of the simulations in Symphony are adapted or partially rerun from earlier research works. We ask that works which use these simulations cite the original sources as well. SymphonyMilkyWay is a partial rerun of the simulations in Mao et al. (2015), SymphonyLCluster was originally run by Bhattacharyya et al. (2022), and SymphonyCluster was originally run by Wu et al. (2013).

Acknowledgements#

This research was supported in part by the Kavli Institute for Particle Astrophysics and Cosmology at Stanford University and SLAC National Accelerator Laboratory, and from the U.S. Department of Energy under contract number DE-AC02-76SF00515 to SLAC National Accelerator Laboratory. This research made use of computational resources at SLAC National Accelerator Laboratory, a U.S. Department of Energy Office, and the Sherlock cluster at the Stanford Research Computing Center (SRCC); the authors are thankful for the support of the SLAC and SRCC computing teams. Additional computing resources used in this work were made available by a generous grant from the Ahmanson Foundation.