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Metadata
Description
A simulation of the extragalactic sky including clustering based on
empirical prescriptions.
Creator
Béthermin, M.
Created
2022-04-14T13:06:57Z
Data updated
2022-04-25T12:32:11Z
Metadata updated
2023-05-05T08:34:12Z
Simulated Infrared Dusty Extragalactic Sky (SIDES) is a simulation of the extragalactic sky in the far-infrared and the millimetre domain, including clustering, based on dark-matter simulations and empirical prescriptions.
The initial paper presenting the method used to build the initial 2 deg² simulated catalogue and its application to continuum observables is Béthermin, Wu, Lagache, et al. (2017A&A...607A..89B). Please refer to this paper to introduce SIDES.
The new python version of the code (pySIDES, https://gitlab.lam.fr/mbethermin/sides-public-release) is described in Béthermin, Gkogkou, Van Cuyck, et al. (submitted, 2022arXiv220412827B). This paper also introduces the modelling of the main emission lines observables in the millimetre ([CII], CO, [CI]) and discusses the implication for line intensity mapping. Please refer to this paper if you use the line-related observables.
This resource contains the pySIDES catalogue (2022) created using the Bolshoi simulation. To get the 2017 catalogue and other products (simulated CONCERTO cubes), please visit SIDES web site (https://cesamsi.lam.fr/instance/sides/home).