Synthetic galaxy clusters and observations based on Dark Energy Survey Year 3 Data

@article{Varga2021SyntheticGC,
  title={Synthetic galaxy clusters and observations based on Dark Energy Survey Year 3 Data},
  author={T. N. Varga and Daniel Gruen and Stella Seitz and Niall MacCrann and Erin S. Sheldon and William G. Hartley and A. Amon and Ami Choi and Antonella Palmese and Y. Zhang and Matthew R. Becker and J. Mccullough and Eduardo Rozo and Eli S. Rykoff and C. To and Sebastian Grandis and Gary M. Bernstein and Scott Dodelson and Kathleen D. Eckert and S. Everett and Robert A. Gruendl and Ian Harrison and Ken Herner and Richard Rollins and Ignacio Sevilla-Noarbe and Michael Troxel and Brian Yanny and Joe Zuntz and H. Thomas Diehl and Michael Jarvis and Michel Aguena and Sahar Allam and James T. Annis and Emmanuel Bertin and S. Bhargava and David Brooks and Aurelio Carnero Rosell and Matias Carrasco Kind and Jorge Carretero and Matteo Costanzi and Luiz Nicolaci da Costa and M. E. S. Pereira and Juan de Vicente and Shantanu Desai and J. P. Dietrich and I. Ferrero and Brenna L. Flaugher and Juan Garc{\'i}a-Bellido and Enrique Gazta{\~n}aga and David W. Gerdes and Julia Gschwend and Gaston R. Guti{\'e}rrez and Samuel R. Hinton and Klaus Honscheid and Tesla E. Jeltema and Kyler W. Kuehn and Nikolay Kuropatkin and Marcio A. G. Maia and M March and Peter Melchior and Felipe Menanteau and Ramon Miquel and Robert Morgan and Justin Myles and Francisco Paz-Chinch{\'o}n and Andreas Alejandro Plazas and A. K. Romer and Eusebio S{\'a}nchez and Victor E. Scarpine and Michael S. Schubnell and Santiago Serrano and M. Smith and Marcelle Soares-Santos and Eric Suchyta and Mollye E. C. Swanson and Gregory G. Tarl{\'e} and D. Thomas and Jochen Weller},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2021}
}
We develop a novel data-driven method for generating synthetic optical observations of galaxy clusters. In cluster weak lensing, the interplay between analysis choices and systematic effects related to source galaxy selection, shape measurement and photometric redshift estimation can be best characterized in end-to-end tests going from mock observations to recovered cluster masses. To create such test scenarios, we measure and model the photometric properties of galaxy clusters and their sky… 
Halo Mass-concentration Relation at the High-mass End
The concentration–mass (c–M) relation encodes key information about the assembly history of dark matter halos. However, its behavior at the high mass end has not been measured precisely in

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