The AGORA High-resolution Galaxy Simulations Comparison Project. IV. Halo and Galaxy Mass Assembly in a Cosmological Zoom-in Simulation at z ≤ 2

In this fourth paper from the AGORA Collaboration, we study the evolution down to redshift z = 2 and below of a set of cosmological zoom-in simulations of a Milky Way mass galaxy by eight of the leading hydrodynamic simulation codes. We also compare this CosmoRun suite of simulations with dark matte...

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Ngā kaituhi matua:	Santi Roca-Fàbrega, Ji-hoon Kim, Joel R. Primack, Minyong Jung, Anna Genina, Loic Hausammann, Hyeonyong Kim, Alessandro Lupi, Kentaro Nagamine, Johnny W. Powell, Yves Revaz, Ikkoh Shimizu, Clayton Strawn, Héctor Velázquez, Tom Abel, Daniel Ceverino, Bili Dong, Thomas R. Quinn, Eun-jin Shin, Alvaro Segovia-Otero, Oscar Agertz, Kirk S. S. Barrow, Corentin Cadiou, Avishai Dekel, Cameron Hummels, Boon Kiat Oh, Romain Teyssier, The AGORA Collaboration
Hōputu:	Artigo
Reo:	Inglês
I whakaputaina:	IOP Publishing 2024-01-01
Rangatū:	The Astrophysical Journal
Ngā marau:	Hydrodynamical simulations Galaxy formation Galaxy evolution
Urunga tuihono:	https://doi.org/10.3847/1538-4357/ad43de
Ngā Tūtohu:	Tāpirihia he Tūtohu Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!