The discovery space of ELT-ANDES. Stars and stellar populations

The ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is the optical and near-infrared high-resolution echelle spectrograph envisioned for the Extremely Large Telescope (ELT). We present a selection of science cases, supported by new calculations and simulations, where ANDES could enable major...

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Detalles Bibliográficos
Autores: Roederer, Ian U., Amado, Pedro J., Rodríguez-López, Cristina
Tipo de recurso: artículo
Estado:Versión aceptada para publicación
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/371615
Acceso en línea:http://hdl.handle.net/10261/371615
Access Level:acceso abierto
Palabra clave:Star clusters
Stellar atmospheres
Stellar evolution
Stellar physics
Stellar populations
High resolution spectroscopy
Galactic archaeology
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dc.title.none.fl_str_mv The discovery space of ELT-ANDES. Stars and stellar populations
title The discovery space of ELT-ANDES. Stars and stellar populations
spellingShingle The discovery space of ELT-ANDES. Stars and stellar populations
Roederer, Ian U.
Star clusters
Stellar atmospheres
Stellar evolution
Stellar physics
Stellar populations
High resolution spectroscopy
Galactic archaeology
title_short The discovery space of ELT-ANDES. Stars and stellar populations
title_full The discovery space of ELT-ANDES. Stars and stellar populations
title_fullStr The discovery space of ELT-ANDES. Stars and stellar populations
title_full_unstemmed The discovery space of ELT-ANDES. Stars and stellar populations
title_sort The discovery space of ELT-ANDES. Stars and stellar populations
dc.creator.none.fl_str_mv Roederer, Ian U.
Amado, Pedro J.
Rodríguez-López, Cristina
author Roederer, Ian U.
author_facet Roederer, Ian U.
Amado, Pedro J.
Rodríguez-López, Cristina
author_role author
author2 Amado, Pedro J.
Rodríguez-López, Cristina
author2_role author
author
dc.contributor.none.fl_str_mv National Science Foundation (US)
Ministerio de Ciencia e Innovación (España)
Swedish Research Council
Science and Technology Facilities Council (UK)
Swedish National Space Agency
Fundação para a Ciência e a Tecnologia (Portugal)
Agencia Estatal de Investigación (España)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Star clusters
Stellar atmospheres
Stellar evolution
Stellar physics
Stellar populations
High resolution spectroscopy
Galactic archaeology
topic Star clusters
Stellar atmospheres
Stellar evolution
Stellar physics
Stellar populations
High resolution spectroscopy
Galactic archaeology
description The ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is the optical and near-infrared high-resolution echelle spectrograph envisioned for the Extremely Large Telescope (ELT). We present a selection of science cases, supported by new calculations and simulations, where ANDES could enable major advances in the fields of stars and stellar populations. We focus on three key areas, including the physics of stellar atmospheres, structure, and evolution; stars of the Milky Way, Local Group, and beyond; and the star-planet connection. The key features of ANDES are its wide wavelength coverage at high spectral resolution and its access to the large collecting area of the ELT. These features position ANDES to address the most compelling questions and potentially transformative advances in stellar astrophysics of the decades ahead, including questions which cannot be anticipated today. © The Author(s) under exclusive licence to Springer Nature B.V. 2024
publishDate 2024
dc.date.none.fl_str_mv 2024
2024
2024
2024
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dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/371615
url http://hdl.handle.net/10261/371615
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spelling The discovery space of ELT-ANDES. Stars and stellar populationsRoederer, Ian U.Amado, Pedro J.Rodríguez-López, CristinaStar clustersStellar atmospheresStellar evolutionStellar physicsStellar populationsHigh resolution spectroscopyGalactic archaeologyThe ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is the optical and near-infrared high-resolution echelle spectrograph envisioned for the Extremely Large Telescope (ELT). We present a selection of science cases, supported by new calculations and simulations, where ANDES could enable major advances in the fields of stars and stellar populations. We focus on three key areas, including the physics of stellar atmospheres, structure, and evolution; stars of the Milky Way, Local Group, and beyond; and the star-planet connection. The key features of ANDES are its wide wavelength coverage at high spectral resolution and its access to the large collecting area of the ELT. These features position ANDES to address the most compelling questions and potentially transformative advances in stellar astrophysics of the decades ahead, including questions which cannot be anticipated today. © The Author(s) under exclusive licence to Springer Nature B.V. 2024IUR acknowledges support from United States National Science Foundation grants AST 1815403 and AST 2205847. CAP and JIGH are thankful to the Spanish Ministry of Science and Innovation (MICINN) for funding under the project PID2020-117493GB-I00. TB acknowledges support from project grant No. 2018- 04857 from the Swedish Research Council. E.M.A.G. acknowledges support from the German Leibniz-Gemeinschaft under project number P67/2018. RM acknowledges support from the Science and Technology Facilities Council (STFC), by the ERC Advanced Grant 695671 ‘QUENCH,’ and by the UKRI Frontier Research grant RISEandFALL. RM also acknowledges funding from a research professorship from the Royal Society. AC acknowledges support from the French National Research Agency (ANR) funded project PEPPER (ANR-20-CE31-0002). AJK acknowledges support by the Swedish National Space Agency (SNSA). VA is supported by FCT (Fundação para a Ciência e Tecnologia) through national funds by the following grants: UIDB/04434/2020, UIDP/04434/2020, and 2022.06962.PTDC. CRL and PJA acknowledge financial support from the Agencia Estatal de Investigación of the Ministerio de Ciencia e Innovación through projects PID2019-109522GB-C52, PID2022-137241NB-C43 and the Severo Ochoa grant CEX2021-001131-S all funded by MCIN/AEI/10.13039/501100011033. DR acknowledges support from the Italian National Institute for Astrophysics through Theory Grant 2022, Fu. Ob. 1.05.12.06.08. JRM acknowledges continuous support from the Universidade Federal do Rio Grande do Norte and Brazilian Agencies CNPq and CAPES.With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).Peer reviewedSpringer NatureNational Science Foundation (US)Ministerio de Ciencia e Innovación (España)Swedish Research CouncilScience and Technology Facilities Council (UK)Swedish National Space AgencyFundação para a Ciência e a Tecnologia (Portugal)Agencia Estatal de Investigación (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2024202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Postprintinfo:eu-repo/semantics/acceptedVersionhttp://hdl.handle.net/10261/371615reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-117493GB-I00info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-109522GB-C52info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2022-137241NB-C43info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2021-001131-Shttp://dx.doi.org/10.1007/s10686-024-09938-8Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3716152026-05-22T06:33:51Z
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