The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web

Autores
Tissera, Patricia Beatriz; Bignone, Lucas Axel; Gonzalez Jara, Jenny; Muñoz Escobar, Ignacio; Cataldi, Pedro Anselmo; Miranda, Valentina P.; Barrientos Acevedo, Daniela; Tapia Contreras, Brian; Pedrosa, Susana Elizabeth; Padilla, Nelson David; Dominguez Tenreiro, Rosa; Casanueva Villarreal, Catalina; Sillero, Emanuel; Silva Mella, Benjamin; Shailesh, Isha; Jara Ferreira, Francisco
Año de publicación
2025
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Context. The CIELO project introduces a novel set of chemo-dynamical zoom-in simulations, designed to simultaneously resolve galaxies and their nearby environments. The initial conditions (ICs) encompass a diverse range of cosmic structures, including local groups, filaments, voids, and walls, enabling a detailed exploration of galaxies within their broader cosmic web context. Aims. This study aims to present the ICs and characterise the global properties of CIELO galaxies and their environments. Specifically, it focuses on galaxies with stellar masses ranging from 108 to 1011 M and investigates key scaling relations, such as the mass-size relation, the Tully-Fisher relation (TFR), and the mass-metallicity relation (MZR) for both stars and star-forming gas. Methods. We employed the DisPerSe algorithm to determine the positions of CIELO galaxies within the cosmic web, with a particular focus on the Pehuen haloes. The selection of Local Group (LG) type volumes was guided by criteria based on relative positions and velocities of the two primary galaxies. The Pehuen regions were selected to map walls, filaments and voids. Synthetic SDSS i, r, and g band images were generated using the SKIRT radiative transfer code. Furthermore, a dynamical decomposition was performed to classify galaxy morphologies into bulge, disc, and stellar halo components. Results. The CIELO galaxies exhibit stellar-to-dark matter fractions consistent with both observational data and other simulation results. These galaxies align with expected scaling relations, such as the mass-size relation and TFR, indicating effective regulation of star formation and feedback processes. The mass-size relation reveals the expected dependence on galaxy morphology. The gas and stellar MZRs also agree well with observational data, with the stellar MZR displaying strong correlations with galaxy size (Rhm) and star formation rate (SFR). This indicates that smaller, less star-forming galaxies tend to have higher metallicities. Future investigations will delve into the chemo-dynamical properties of bulges, discs, and stellar haloes, exploring their connections to assembly histories and positions within the cosmic web.
Fil: Tissera, Patricia Beatriz. Pontificia Universidad Católica de Chile; Chile
Fil: Bignone, Lucas Axel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Gonzalez Jara, Jenny. Pontificia Universidad Católica de Chile; Chile
Fil: Muñoz Escobar, Ignacio. Pontificia Universidad Católica de Chile; Chile
Fil: Cataldi, Pedro Anselmo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Miranda, Valentina P.. Pontificia Universidad Católica de Chile; Chile
Fil: Barrientos Acevedo, Daniela. Pontificia Universidad Católica de Chile; Chile
Fil: Tapia Contreras, Brian. Pontificia Universidad Católica de Chile; Chile
Fil: Pedrosa, Susana Elizabeth. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Padilla, Nelson David. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Dominguez Tenreiro, Rosa. Universidad Autónoma de Madrid; España
Fil: Casanueva Villarreal, Catalina. Pontificia Universidad Católica de Chile; Chile
Fil: Sillero, Emanuel. Pontificia Universidad Católica de Chile; Chile
Fil: Silva Mella, Benjamin. Pontificia Universidad Católica de Chile; Chile
Fil: Shailesh, Isha. Pontificia Universidad Católica de Chile; Chile
Fil: Jara Ferreira, Francisco. Pontificia Universidad Católica de Chile; Chile
Materia
galaxies: abundances
galaxies: evolution
galaxies: fundamental parameters
Astrophysics of Galaxies
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/278048
Acceder
id CONICETDig_8f8a9cd899eb7fee3641d529ab9168a7
oai_identifier_str oai:ri.conicet.gov.ar:11336/278048
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The CIELO project: The chemo-dynamical properties of galaxies and the cosmic webTissera, Patricia BeatrizBignone, Lucas AxelGonzalez Jara, JennyMuñoz Escobar, IgnacioCataldi, Pedro AnselmoMiranda, Valentina P.Barrientos Acevedo, DanielaTapia Contreras, BrianPedrosa, Susana ElizabethPadilla, Nelson DavidDominguez Tenreiro, RosaCasanueva Villarreal, CatalinaSillero, EmanuelSilva Mella, BenjaminShailesh, IshaJara Ferreira, Franciscogalaxies: abundancesgalaxies: evolutiongalaxies: fundamental parametersAstrophysics of Galaxieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. The CIELO project introduces a novel set of chemo-dynamical zoom-in simulations, designed to simultaneously resolve galaxies and their nearby environments. The initial conditions (ICs) encompass a diverse range of cosmic structures, including local groups, filaments, voids, and walls, enabling a detailed exploration of galaxies within their broader cosmic web context. Aims. This study aims to present the ICs and characterise the global properties of CIELO galaxies and their environments. Specifically, it focuses on galaxies with stellar masses ranging from 108 to 1011 M and investigates key scaling relations, such as the mass-size relation, the Tully-Fisher relation (TFR), and the mass-metallicity relation (MZR) for both stars and star-forming gas. Methods. We employed the DisPerSe algorithm to determine the positions of CIELO galaxies within the cosmic web, with a particular focus on the Pehuen haloes. The selection of Local Group (LG) type volumes was guided by criteria based on relative positions and velocities of the two primary galaxies. The Pehuen regions were selected to map walls, filaments and voids. Synthetic SDSS i, r, and g band images were generated using the SKIRT radiative transfer code. Furthermore, a dynamical decomposition was performed to classify galaxy morphologies into bulge, disc, and stellar halo components. Results. The CIELO galaxies exhibit stellar-to-dark matter fractions consistent with both observational data and other simulation results. These galaxies align with expected scaling relations, such as the mass-size relation and TFR, indicating effective regulation of star formation and feedback processes. The mass-size relation reveals the expected dependence on galaxy morphology. The gas and stellar MZRs also agree well with observational data, with the stellar MZR displaying strong correlations with galaxy size (Rhm) and star formation rate (SFR). This indicates that smaller, less star-forming galaxies tend to have higher metallicities. Future investigations will delve into the chemo-dynamical properties of bulges, discs, and stellar haloes, exploring their connections to assembly histories and positions within the cosmic web.Fil: Tissera, Patricia Beatriz. Pontificia Universidad Católica de Chile; ChileFil: Bignone, Lucas Axel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Gonzalez Jara, Jenny. Pontificia Universidad Católica de Chile; ChileFil: Muñoz Escobar, Ignacio. Pontificia Universidad Católica de Chile; ChileFil: Cataldi, Pedro Anselmo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Miranda, Valentina P.. Pontificia Universidad Católica de Chile; ChileFil: Barrientos Acevedo, Daniela. Pontificia Universidad Católica de Chile; ChileFil: Tapia Contreras, Brian. Pontificia Universidad Católica de Chile; ChileFil: Pedrosa, Susana Elizabeth. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Padilla, Nelson David. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Dominguez Tenreiro, Rosa. Universidad Autónoma de Madrid; EspañaFil: Casanueva Villarreal, Catalina. Pontificia Universidad Católica de Chile; ChileFil: Sillero, Emanuel. Pontificia Universidad Católica de Chile; ChileFil: Silva Mella, Benjamin. Pontificia Universidad Católica de Chile; ChileFil: Shailesh, Isha. Pontificia Universidad Católica de Chile; ChileFil: Jara Ferreira, Francisco. Pontificia Universidad Católica de Chile; ChileEDP Sciences2025-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/278048Tissera, Patricia Beatriz; Bignone, Lucas Axel; Gonzalez Jara, Jenny; Muñoz Escobar, Ignacio; Cataldi, Pedro Anselmo; et al.; The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web; EDP Sciences; Astronomy and Astrophysics; 697; A134; 5-2025; 1-120004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/10.1051/0004-6361/202453348info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202453348info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-12-23T14:22:22Zoai:ri.conicet.gov.ar:11336/278048instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-12-23 14:22:23.297CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
title The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
spellingShingle The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
Tissera, Patricia Beatriz
galaxies: abundances
galaxies: evolution
galaxies: fundamental parameters
Astrophysics of Galaxies
title_short The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
title_full The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
title_fullStr The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
title_full_unstemmed The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
title_sort The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web
dc.creator.none.fl_str_mv Tissera, Patricia Beatriz
Bignone, Lucas Axel
Gonzalez Jara, Jenny
Muñoz Escobar, Ignacio
Cataldi, Pedro Anselmo
Miranda, Valentina P.
Barrientos Acevedo, Daniela
Tapia Contreras, Brian
Pedrosa, Susana Elizabeth
Padilla, Nelson David
Dominguez Tenreiro, Rosa
Casanueva Villarreal, Catalina
Sillero, Emanuel
Silva Mella, Benjamin
Shailesh, Isha
Jara Ferreira, Francisco
author Tissera, Patricia Beatriz
author_facet Tissera, Patricia Beatriz
Bignone, Lucas Axel
Gonzalez Jara, Jenny
Muñoz Escobar, Ignacio
Cataldi, Pedro Anselmo
Miranda, Valentina P.
Barrientos Acevedo, Daniela
Tapia Contreras, Brian
Pedrosa, Susana Elizabeth
Padilla, Nelson David
Dominguez Tenreiro, Rosa
Casanueva Villarreal, Catalina
Sillero, Emanuel
Silva Mella, Benjamin
Shailesh, Isha
Jara Ferreira, Francisco
author_role author
author2 Bignone, Lucas Axel
Gonzalez Jara, Jenny
Muñoz Escobar, Ignacio
Cataldi, Pedro Anselmo
Miranda, Valentina P.
Barrientos Acevedo, Daniela
Tapia Contreras, Brian
Pedrosa, Susana Elizabeth
Padilla, Nelson David
Dominguez Tenreiro, Rosa
Casanueva Villarreal, Catalina
Sillero, Emanuel
Silva Mella, Benjamin
Shailesh, Isha
Jara Ferreira, Francisco
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv galaxies: abundances
galaxies: evolution
galaxies: fundamental parameters
Astrophysics of Galaxies
topic galaxies: abundances
galaxies: evolution
galaxies: fundamental parameters
Astrophysics of Galaxies
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Context. The CIELO project introduces a novel set of chemo-dynamical zoom-in simulations, designed to simultaneously resolve galaxies and their nearby environments. The initial conditions (ICs) encompass a diverse range of cosmic structures, including local groups, filaments, voids, and walls, enabling a detailed exploration of galaxies within their broader cosmic web context. Aims. This study aims to present the ICs and characterise the global properties of CIELO galaxies and their environments. Specifically, it focuses on galaxies with stellar masses ranging from 108 to 1011 M and investigates key scaling relations, such as the mass-size relation, the Tully-Fisher relation (TFR), and the mass-metallicity relation (MZR) for both stars and star-forming gas. Methods. We employed the DisPerSe algorithm to determine the positions of CIELO galaxies within the cosmic web, with a particular focus on the Pehuen haloes. The selection of Local Group (LG) type volumes was guided by criteria based on relative positions and velocities of the two primary galaxies. The Pehuen regions were selected to map walls, filaments and voids. Synthetic SDSS i, r, and g band images were generated using the SKIRT radiative transfer code. Furthermore, a dynamical decomposition was performed to classify galaxy morphologies into bulge, disc, and stellar halo components. Results. The CIELO galaxies exhibit stellar-to-dark matter fractions consistent with both observational data and other simulation results. These galaxies align with expected scaling relations, such as the mass-size relation and TFR, indicating effective regulation of star formation and feedback processes. The mass-size relation reveals the expected dependence on galaxy morphology. The gas and stellar MZRs also agree well with observational data, with the stellar MZR displaying strong correlations with galaxy size (Rhm) and star formation rate (SFR). This indicates that smaller, less star-forming galaxies tend to have higher metallicities. Future investigations will delve into the chemo-dynamical properties of bulges, discs, and stellar haloes, exploring their connections to assembly histories and positions within the cosmic web.
Fil: Tissera, Patricia Beatriz. Pontificia Universidad Católica de Chile; Chile
Fil: Bignone, Lucas Axel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Gonzalez Jara, Jenny. Pontificia Universidad Católica de Chile; Chile
Fil: Muñoz Escobar, Ignacio. Pontificia Universidad Católica de Chile; Chile
Fil: Cataldi, Pedro Anselmo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Miranda, Valentina P.. Pontificia Universidad Católica de Chile; Chile
Fil: Barrientos Acevedo, Daniela. Pontificia Universidad Católica de Chile; Chile
Fil: Tapia Contreras, Brian. Pontificia Universidad Católica de Chile; Chile
Fil: Pedrosa, Susana Elizabeth. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Padilla, Nelson David. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Dominguez Tenreiro, Rosa. Universidad Autónoma de Madrid; España
Fil: Casanueva Villarreal, Catalina. Pontificia Universidad Católica de Chile; Chile
Fil: Sillero, Emanuel. Pontificia Universidad Católica de Chile; Chile
Fil: Silva Mella, Benjamin. Pontificia Universidad Católica de Chile; Chile
Fil: Shailesh, Isha. Pontificia Universidad Católica de Chile; Chile
Fil: Jara Ferreira, Francisco. Pontificia Universidad Católica de Chile; Chile
description Context. The CIELO project introduces a novel set of chemo-dynamical zoom-in simulations, designed to simultaneously resolve galaxies and their nearby environments. The initial conditions (ICs) encompass a diverse range of cosmic structures, including local groups, filaments, voids, and walls, enabling a detailed exploration of galaxies within their broader cosmic web context. Aims. This study aims to present the ICs and characterise the global properties of CIELO galaxies and their environments. Specifically, it focuses on galaxies with stellar masses ranging from 108 to 1011 M and investigates key scaling relations, such as the mass-size relation, the Tully-Fisher relation (TFR), and the mass-metallicity relation (MZR) for both stars and star-forming gas. Methods. We employed the DisPerSe algorithm to determine the positions of CIELO galaxies within the cosmic web, with a particular focus on the Pehuen haloes. The selection of Local Group (LG) type volumes was guided by criteria based on relative positions and velocities of the two primary galaxies. The Pehuen regions were selected to map walls, filaments and voids. Synthetic SDSS i, r, and g band images were generated using the SKIRT radiative transfer code. Furthermore, a dynamical decomposition was performed to classify galaxy morphologies into bulge, disc, and stellar halo components. Results. The CIELO galaxies exhibit stellar-to-dark matter fractions consistent with both observational data and other simulation results. These galaxies align with expected scaling relations, such as the mass-size relation and TFR, indicating effective regulation of star formation and feedback processes. The mass-size relation reveals the expected dependence on galaxy morphology. The gas and stellar MZRs also agree well with observational data, with the stellar MZR displaying strong correlations with galaxy size (Rhm) and star formation rate (SFR). This indicates that smaller, less star-forming galaxies tend to have higher metallicities. Future investigations will delve into the chemo-dynamical properties of bulges, discs, and stellar haloes, exploring their connections to assembly histories and positions within the cosmic web.
publishDate 2025
dc.date.none.fl_str_mv 2025-05
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/278048
Tissera, Patricia Beatriz; Bignone, Lucas Axel; Gonzalez Jara, Jenny; Muñoz Escobar, Ignacio; Cataldi, Pedro Anselmo; et al.; The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web; EDP Sciences; Astronomy and Astrophysics; 697; A134; 5-2025; 1-12
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/278048
identifier_str_mv Tissera, Patricia Beatriz; Bignone, Lucas Axel; Gonzalez Jara, Jenny; Muñoz Escobar, Ignacio; Cataldi, Pedro Anselmo; et al.; The CIELO project: The chemo-dynamical properties of galaxies and the cosmic web; EDP Sciences; Astronomy and Astrophysics; 697; A134; 5-2025; 1-12
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/10.1051/0004-6361/202453348
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202453348
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1852335646335565824
score 12.952241

Publicaciones similares