Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT

We present preliminary results on the potential of HARMONI, the first light integral field spectrograph for the ELT, to explore the evolution of central super massive black holes (SMBH)—host galaxy relation in the range from z~0.7 to z~2.5. We simulated HARMONI observations of QSO+host galaxy at dif...

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Detalles Bibliográficos
Autores: García Lorenzo, B., Monreal Ibero, A., Mediavilla, E., Pereira Santaella, Miguel, Thatte, Niranjan
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:España
Institución:Instituto Nacional de Técnica Aeroespacial (INTA)
Repositorio:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
OAI Identifier:oai:digital.inta.es:20.500.12666/317
Acceso en línea:https://www.frontiersin.org/articles/10.3389/fspas.2019.00073
http://hdl.handle.net/20.500.12666/317
Access Level:acceso abierto
Palabra clave:Quasars
Cosmology
Extragalactic astronomy
Active galactic nuclei
Cosmological parameters
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spelling Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELTGarcía Lorenzo, B.Monreal Ibero, A.Mediavilla, E.Pereira Santaella, MiguelThatte, NiranjanQuasarsCosmologyExtragalactic astronomyActive galactic nucleiCosmological parametersWe present preliminary results on the potential of HARMONI, the first light integral field spectrograph for the ELT, to explore the evolution of central super massive black holes (SMBH)—host galaxy relation in the range from z~0.7 to z~2.5. We simulated HARMONI observations of QSO+host galaxy at different redshifts, assuming different morphologies for the host galaxy. As input, we combined MUSE observations of nearby galaxies and a theoretical QSO spectrum. These were dimmed and redshifted to the desired cosmic epoch. We scaled the total host galaxy luminosity to three different values, sampling three orders of magnitude. Likewise, we assumed two different luminosities for the central QSO. Simulations were performed for the 30×60 mas2 HARMONI spatial scale and LTAO working at 0.67 arcsec seeing. The selected wavelength range (i.e., 4,700–5,300 Å at rest-frame) was sampled at the lowest HARMONI spectral resolving power (i.e., R~3,200). This configuration included all the ingredients to estimate the host galaxy parameters and the SMBH mass, as well as for assessing the morphological type of the host galaxy.BG-L and AM-I acknowledge support from the State Research Agency (AEI) of the Spanish Ministry of Science, Innovation and Universities (MCIU) and the European Regional Development Fund (FEDER) under grant with reference AYA2105-68217-P. MP-S acknowledges support from the Comunidad de Madrid through Atraccion de Talento Investigador Grant 2018-T1/TIC-11035 and STFC through grant ST/N000919/1. MP-S and NT acknowledge support from STFC through grant ST/N002717/1; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737).Peer reviewExtragalactic AstronomyUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737Science and Technology Facilities Council (STFC)Comunidad de MadridMinisterio de Economía y Competitividad (MINECO)202120212019info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501application/pdfhttps://www.frontiersin.org/articles/10.3389/fspas.2019.00073http://hdl.handle.net/20.500.12666/317reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacialinstname:Instituto Nacional de Técnica Aeroespacial (INTA)Inglésinfo:eu-repo/grantAgreement/MINECO//AYA2015-68217-PAttribution-NonCommercial-NoDerivatives 4.0 InternationalCopyright © 2019 García-Lorenzo, Monreal-Ibero, Mediavilla, Pereira-Santaella and Thatte.https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessoai:digital.inta.es:20.500.12666/3172026-06-23T12:46:37Z
dc.title.none.fl_str_mv Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
title Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
spellingShingle Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
García Lorenzo, B.
Quasars
Cosmology
Extragalactic astronomy
Active galactic nuclei
Cosmological parameters
title_short Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
title_full Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
title_fullStr Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
title_full_unstemmed Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
title_sort Black Hole-Galaxy Scaling Relation Evolution From z~2.5: Simulated Observations With HARMONI on the ELT
dc.creator.none.fl_str_mv García Lorenzo, B.
Monreal Ibero, A.
Mediavilla, E.
Pereira Santaella, Miguel
Thatte, Niranjan
author García Lorenzo, B.
author_facet García Lorenzo, B.
Monreal Ibero, A.
Mediavilla, E.
Pereira Santaella, Miguel
Thatte, Niranjan
author_role author
author2 Monreal Ibero, A.
Mediavilla, E.
Pereira Santaella, Miguel
Thatte, Niranjan
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
Science and Technology Facilities Council (STFC)
Comunidad de Madrid
Ministerio de Economía y Competitividad (MINECO)
dc.subject.none.fl_str_mv Quasars
Cosmology
Extragalactic astronomy
Active galactic nuclei
Cosmological parameters
topic Quasars
Cosmology
Extragalactic astronomy
Active galactic nuclei
Cosmological parameters
description We present preliminary results on the potential of HARMONI, the first light integral field spectrograph for the ELT, to explore the evolution of central super massive black holes (SMBH)—host galaxy relation in the range from z~0.7 to z~2.5. We simulated HARMONI observations of QSO+host galaxy at different redshifts, assuming different morphologies for the host galaxy. As input, we combined MUSE observations of nearby galaxies and a theoretical QSO spectrum. These were dimmed and redshifted to the desired cosmic epoch. We scaled the total host galaxy luminosity to three different values, sampling three orders of magnitude. Likewise, we assumed two different luminosities for the central QSO. Simulations were performed for the 30×60 mas2 HARMONI spatial scale and LTAO working at 0.67 arcsec seeing. The selected wavelength range (i.e., 4,700–5,300 Å at rest-frame) was sampled at the lowest HARMONI spectral resolving power (i.e., R~3,200). This configuration included all the ingredients to estimate the host galaxy parameters and the SMBH mass, as well as for assessing the morphological type of the host galaxy.
publishDate 2019
dc.date.none.fl_str_mv 2019
2021
2021
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://www.frontiersin.org/articles/10.3389/fspas.2019.00073
http://hdl.handle.net/20.500.12666/317
url https://www.frontiersin.org/articles/10.3389/fspas.2019.00073
http://hdl.handle.net/20.500.12666/317
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv info:eu-repo/grantAgreement/MINECO//AYA2015-68217-P
dc.rights.none.fl_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
Copyright © 2019 García-Lorenzo, Monreal-Ibero, Mediavilla, Pereira-Santaella and Thatte.
https://creativecommons.org/licenses/by-nc-nd/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
Copyright © 2019 García-Lorenzo, Monreal-Ibero, Mediavilla, Pereira-Santaella and Thatte.
https://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Extragalactic Astronomy
publisher.none.fl_str_mv Extragalactic Astronomy
dc.source.none.fl_str_mv reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname:Instituto Nacional de Técnica Aeroespacial (INTA)
instname_str Instituto Nacional de Técnica Aeroespacial (INTA)
reponame_str DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
collection DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
repository.name.fl_str_mv
repository.mail.fl_str_mv
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