RT Journal Article
T1 Ovi traces photoionized streams with collisionally ionized boundaries in cosmological simulations of z similar to 1 massive galaxies
A1 Strawn, Clayton
A1 Roca Fábrega, Santi
A1 Mandelker, Nir
A1 Primack, Joel
A1 Stern, Jonathan
A1 Ceverino, Daniel
A1 Dekel, Avishai
A1 Wang, Bryan
A1 Dange, Rishi Dange
AB Partial support for CS was provided by grant HST-AR-14578 toJP from the STScI under NASA contract NAS5-26555. SRF ac-knowledges support from a Spanish postdoctoral fellowship, undergrant number 2017- T2/TIC-5592. SRF also acknowledges finan-cial support from the Spanish Ministry of Economy and Com-petitiveness (MINECO) under grant number AYA2016-75808-R,AYA2017-90589-REDT and S2018/NMT-429, and from the CAM-UCM under grant number PR65/19-22462. NM acknowledges sup-port from the Klauss Tschira Foundation through the HITS YaleProgram in Astrophysics (HYPA), and from the Gordon and BettyMoore Foundation through Grant GBMF7392. JS is supported bythe CIERA Postdoctoral Fellowship Program. The VELA simula-tions were performed at the National Energy Research ScientificComputing Center (NERSC) at Lawrence Berkeley National Lab-oratory, and at NASA Advanced Supercomputing (NAS) at NASAAmes Research Center. DC is a Ramon-Cajal Researcher and issupported by the Ministerio de Ciencia, Innovación y Universidades(MICIU/FEDER) under research grant PGC2018-094975-C21. Par-tial support for AD comes from DIP STE1869/2-1 GE625/17-1 andISF 861/20. BW and RD carried out this research under the aus-pices of the Science Internship Program (SIP) at the University ofCalifornia Santa Cruz, which also provided partial funding to CS.Technical help was provided by Cameron Hummels, Britton Smith,Nathan Goldbaum, Matt Turk, and the rest of theytcommunity. Wealso benefitted from helpful discussions with Joe Burchett, SandraFaber, Yakov Faerman, Max Gronke, David Koo, Daisuke Nagai,S. Peng Oh, J. Xavier Prochaska, Rahul Sharma, and Sally Zhu.Finally, we thank the comments of an anonymous referee whichimproved several key points of the paper.
PB Oxford University Press.
SN 0035-8711
YR 2021
FD 2021-03
LK https://hdl.handle.net/20.500.14352/8466
UL https://hdl.handle.net/20.500.14352/8466
LA eng
NO © 2020 The Author(s). Artículo firmado por 9 autores. Partial support for CS was provided by grant HST-AR-14578 toJP from the STScI under NASA contract NAS5-26555. SRF ac-knowledges support from a Spanish postdoctoral fellowship, undergrant number 2017- T2/TIC-5592. SRF also acknowledges finan-cial support from the Spanish Ministry of Economy and Com-petitiveness (MINECO) under grant number AYA2016-75808-R,AYA2017-90589-REDT and S2018/NMT-429, and from the CAM-UCM under grant number PR65/19-22462. NM acknowledges sup-port from the Klauss Tschira Foundation through the HITS YaleProgram in Astrophysics (HYPA), and from the Gordon and BettyMoore Foundation through Grant GBMF7392. JS is supported bythe CIERA Postdoctoral Fellowship Program. The VELA simula-tions were performed at the National Energy Research ScientificComputing Center (NERSC) at Lawrence Berkeley National Lab-oratory, and at NASA Advanced Supercomputing (NAS) at NASAAmes Research Center. DC is a Ramon-Cajal Researcher and issupported by the Ministerio de Ciencia, Innovación y Universidades(MICIU/FEDER) under research grant PGC2018-094975-C21. Par-tial support for AD comes from DIP STE1869/2-1 GE625/17-1 andISF 861/20. BW and RD carried out this research under the aus-pices of the Science Internship Program (SIP) at the University ofCalifornia Santa Cruz, which also provided partial funding to CS.Technical help was provided by Cameron Hummels, Britton Smith,Nathan Goldbaum, Matt Turk, and the rest of theytcommunity. Wealso benefitted from helpful discussions with Joe Burchett, SandraFaber, Yakov Faerman, Max Gronke, David Koo, Daisuke Nagai,S. Peng Oh, J. Xavier Prochaska, Rahul Sharma, and Sally Zhu.Finally, we thank the comments of an anonymous referee whichimproved several key points of the paper.
NO Ministerio de Economía y Competitividad (MINECO)
NO Ministerio de Ciencia e Innovación (MICINN)/FEDER
NO Comunidad de Madrid
NO Universidad Complutense de Madrid/Comunidad de Madrid
NO STScI under NASA
NO Klauss Tschira Foundation through the HITS Yale Program in Astrophysics (HYPA)
NO Gordon and Betty Moore Foundation
NO CIERA Postdoctoral Fellowship Program
NO Science Internship Program (SIP) at the University of California Santa Cruz
DS Docta Complutense
RD 19 abr 2025