Star formation quenching in the infall region around galaxy clusters

Autor: Valeria Coenda, Andrés Nicolás Ruiz, Hernán Muriel, Sofía Alejandra Cora, Cristian Antonio Vega Martínez, Luis Pereyra, Juan Manuel Salerno

Publikováno v: Monthly Notices of the Royal Astronomical Society. 517:4515-4528

We analyse the connection between the star formation quenching of galaxies and their location in the outskirts of clusters in the redshift range z = [0, 2] by estimating the fraction of red galaxies. More specifically, we focus on galaxies that infal

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::7736b7419ab42e16966fcabd6e8a4c44
https://doi.org/10.1093/mnras/stac2980

Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations

Autor: Valeria Coenda, Martín de los Rios, Hernán Muriel, Sofía A Cora, Héctor J Martínez, Andrés N Ruiz, Cristian A Vega-Martínez

Publikováno v: Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP

We connect galaxy properties with their orbital classification by analysing a sample of galaxies with stellar mass $M_{\star} \geq 10^{8.5}h^{-1}M_\odot$ residing in and around massive and isolated galaxy clusters with mass $M_{200} > 10^{15}h^{-1}M_

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::93b4dbec817e7d05710cff858500cd2d
http://arxiv.org/abs/2112.01552

The Uchuu simulations: Data Release 1 and dark matter halo concentrations

Autor: Anatoly Klypin, David E. Millán-Calero, Francisco Prada, Darren J. Croton, Bruno Altieri, Cristian A. Vega-Martínez, Taira Oogi, Sofía A. Cora, Manodeep Sinha, Sylvain de la Torre, Eric Jullo, José Ruedas, R. Benton Metcalf, Tomoaki Ishiyama

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 506 (3), pp.4210-4231. ⟨10.1093/mnras/stab1755⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 506 (3), pp.4210-4231. ⟨10.1093/mnras/stab1755⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname

We introduce the Uchuu suite of large high-resolution cosmological N-body simulations. The largest simulation, named Uchuu, consists of 2.1 trillion (12 8003) dark matter particles in a box of side-length 2.0 h-1, Gpc$, with particle mass of 3.27 ×

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b90914e298262960a5582aa4ef8d5112
http://hdl.handle.net/10261/264963

Overdensity of VVV galaxies behind the Galactic bulge

Autor: Sol Alonso, Georgina Coldwell, Daniela Galdeano, Dante Minniti, Fernanda Duplancic, Andrés N. Ruiz, Sofía A. Cora, Cristian A Vega-Martínez, Noelia Perez, Luis Pereyra

Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP

Context. The extragalactic vision we have through the Milky Way is very unclear. There is significant extinction of the optical emission from objects located in the region called the zone of avoidance (ZOA). NIR wavelengths are less affected by extin

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7021903d55b7fbc404615629b2c5784f
http://arxiv.org/abs/2103.01865

Investigating the growing population of massive quiescent galaxies at cosmic noon

Autor: Sofía A. Cora, Isak Wold, Caryl Gronwall, Sydney Sherman, Robin Ciardullo, Casey Papovich, Jonathan Florez, Tomás Hough, Cristian A. Vega-Martínez, Matthew L. Stevans, Steven L. Finkelstein, Lalitwadee Kawinwanichakij, Shardha Jogee

Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET

We explore the buildup of quiescent galaxies using a sample of 28,469 massive (𝑀★ ≥ 1011M ) galaxies at redshifts 1.5 < 𝑧 < 3.0, drawn from a 17.5 deg2 area (0.33 Gpc3 comoving volume at these redshifts). This allows for a robust study of t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47526e42eaae6dc1165cf5c5d176050a
https://academic.oup.com/mnras/article/499/3/4239/5924472