Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

Detalhes bibliográficos
Autores: Lusso, E., Akrami, Y., Euclid Collaboration, García-Bellido Capdevila, Juan
Formato: artículo
Fecha de publicación:2024
País:España
Recursos:Universidad Autónoma de Madrid
Repositorio:Biblos-e Archivo. Repositorio Institucional de la UAM
Idioma:inglés
OAI Identifier:oai:repositorio.uam.es:10486/716970
Acesso em linha:http://hdl.handle.net/10486/716970
https://dx.doi.org/10.1051/0004-6361/202348326
Access Level:acceso abierto
Palavra-chave:Galaxies: active
Quasars: general
Quasars: supermassive black holes
Física
id ES_b4c5ec7f9bdcba601023d2c5bc32b2d8
oai_identifier_str oai:repositorio.uam.es:10486/716970
network_acronym_str ES
network_name_str España
repository_id_str
dc.title.none.fl_str_mv Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
spellingShingle Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
Lusso, E.
Galaxies: active
Quasars: general
Quasars: supermassive black holes
Física
title_short Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_full Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_fullStr Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_full_unstemmed Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_sort Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
dc.creator.none.fl_str_mv Lusso, E.
Akrami, Y.
Euclid Collaboration
García-Bellido Capdevila, Juan
author Lusso, E.
author_facet Lusso, E.
Akrami, Y.
Euclid Collaboration
García-Bellido Capdevila, Juan
author_role author
author2 Akrami, Y.
Euclid Collaboration
García-Bellido Capdevila, Juan
author2_role author
author
author
dc.contributor.none.fl_str_mv Facultad de Ciencias
dc.subject.none.fl_str_mv Galaxies: active
Quasars: general
Quasars: supermassive black holes
Física
topic Galaxies: active
Quasars: general
Quasars: supermassive black holes
Física
description Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
publishDate 2024
dc.date.none.fl_str_mv 2024
2024-05-01
dc.type.none.fl_str_mv research article
http://purl.org/coar/resource_type/c_2df8fbb1
AM
http://purl.org/coar/version/c_ab4af688f83e57aa
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv http://hdl.handle.net/10486/716970
https://dx.doi.org/10.1051/0004-6361/202348326
url http://hdl.handle.net/10486/716970
https://dx.doi.org/10.1051/0004-6361/202348326
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:Biblos-e Archivo. Repositorio Institucional de la UAM
instname:Universidad Autónoma de Madrid
instname_str Universidad Autónoma de Madrid
reponame_str Biblos-e Archivo. Repositorio Institucional de la UAM
collection Biblos-e Archivo. Repositorio Institucional de la UAM
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869417288623456256
spelling Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISPLusso, E.Akrami, Y.Euclid CollaborationGarcía-Bellido Capdevila, JuanGalaxies: activeQuasars: generalQuasars: supermassive black holesFísicaArtículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAMThe statistical distribution and evolution of key properties of active galactic nuclei (AGN), such as their accretion rate, mass, and spin, remains a subject of open debate in astrophysics. The ESA Euclid space mission, launched on July 1 2023, promises a breakthrough in this field. We create detailed mock catalogues of AGN spectra from the rest-frame near-infrared down to the ultraviolet -including emission lines -to simulate what Euclid will observe for both obscured (type 2) and unobscured (type 1) AGN. We concentrate on the red grisms of the NISP instrument, which will be used for the wide-field survey, opening a new window for spectroscopic AGN studies in the near-infrared. We quantify the efficiency in the redshift determination as well as in retrieving the emission line flux of the Hα+[N II] complex, as Euclid is mainly focused on this emission line, given that it is expected to be the brightest one in the probed redshift range. Spectroscopic redshifts are measured for 83% of the simulated AGN in the interval where the Hα is visible (i.e. 0.89 < z < 1.83 at a line flux of > 2 × 10-16 erg s-1 cm-2, encompassing the peak of AGN activity at z ≃ 1 - 1.5) within the spectral coverage of the red grism. Outside this redshift range, the measurement efficiency decreases significantly. Overall, a spectroscopic redshift iscorrectly determined for about 90% of type 2 AGN down to an emission line flux of roughly 3 × 10-16 erg s-1 cm-2, and for type 1 AGN down to 8.5 × 10-16 erg s-1 cm-2. Recovered values for black hole mass show a small offset with respect to the input values by about 10%, but the agreement is good overall. With such a high spectroscopic coverage at z < 2, we will be able to measure AGN demography, scaling relations, and clustering from the epoch of the peak of AGN activity down to the present-day Universe for hundreds of thousands of AGN with homogeneous spectroscopic informationWe thank the anonymous reviewer for their thorough reading and for useful comments and suggestions that have improved the clarity of the paper. V. A. acknowledges support from INAF-PRIN 1.05.01.85.08. L. B. acknowledges financial support from grant PRIN2017. A. F. acknowledges the support from project \"VLT-MOONS\" CRAM 1.05.03.07, INAF Large Grant 2022 \"The metal circle: a new sharp view of the baryon cycle up to Cosmic Dawn with the latest generation IFU facilities\" and INAF Large Grant 2022 \"Dual and binary SMBH in the multi-messenger era\". F. S. acknowledges partial support from the European Union's Horizon 2020 research and innovation programme under the Marie Sk\u0142odowska-Curie grant agreement No. 860744. The Euclid Consortium acknowledges the European Space Agency and a number of agencies and institutes that have supported the development of Euclid, in particular the Academy of Finland, the Agenzia Spaziale Italiana, the Belgian Science Policy, the Canadian Euclid Consortium, the French Centre National d'\u00C9tudes Spatiales, the Deutsches Zentrum f\u00FCr Luft- und Raumfahrt, the Danish Space Research Institute, the Funda\u00E7\u00E3o para a Ci\u00EAncia e a Tecnologia, the Ministerio de Ciencia e Innovaci\u00F3n, the National Aeronautics and Space Administration, the National Astronomical Observatory of Japan, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Romanian Space Agency, the State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid web site (http://www.euclid-ec.org).EDP SciencesFacultad de Ciencias20242024-05-01research articlehttp://purl.org/coar/resource_type/c_2df8fbb1AMhttp://purl.org/coar/version/c_ab4af688f83e57aainfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10486/716970https://dx.doi.org/10.1051/0004-6361/202348326reponame:Biblos-e Archivo. Repositorio Institucional de la UAMinstname:Universidad Autónoma de MadridInglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttp://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:repositorio.uam.es:10486/7169702026-06-23T12:46:27Z
score 15,811543

Registos relacionados