Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST
- Autores
- Saxena, Aayush; Overzier, Roderik A; Villar Martín, Montserrat; Heckman, Tim; Roy, Namrata; Duncan, Kenneth J; Röttgering, Huub; Miley, George; Aydar, Catarina; Best, Philip; Bosman, Sarah E. I.; Cameron, Alex J.; Gabányi, Krisztina Éva; Humphrey, Andrew; Morais, Sandy; Onoue, Masafusa; Pentericci, Laura; Reynaldi, María Victoria; Venemans, Bram
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present rest-frame optical JWST Near-infrared Spectrograph (NIRSpec) integral field unit (IFU) spectroscopy of TN J1338−1942 at z = 4.1, one of the most luminous galaxies in the early universe with powerful extended radio jets. Previous observations showed evidence for strong, large-scale outflows based on its large (∼150 kpc) halo detected in Ly α, and high-velocity [O ii] emission features detected in ground-based spectroscopy. Our NIRSpec/IFU observations spatially resolve the emission line properties across the host galaxy. We find at least five concentrations of strong line emission, coinciding with discrete continuum features previously detected in imaging from Hubble Space Telescope and JWST, over an extent of ∼2 arcsec (∼15 kpc). The spectral diagnostics unambiguously trace active galactic nuclei (AGN) activity plus interaction between the interstellar medium and the radio jet as the dominant mechanisms for the ionization state and kinematics of the gas in the system. A secondary region of very high ionization lies at roughly 5 kpc away from the nucleus, and within the context of an expanding cocoon enveloping the radio lobe, this may be explained by strong shock-ionization of the entrained gas. However, it could also signal the presence of a second obscured AGN, which may offer an explanation for an intriguing outflow feature seen perpendicular to the radio axis. The presence of a dual supermassive black holes system in this galaxy would support that large galaxies in the early Universe quickly accumulated their mass through the merging of smaller units, at the centres of large overdensities. The inferred black hole mass to stellar mass ratio of 0.01−0.1 for TNJ1338 points to a more rapid assembly of black holes compared to the stellar mass of galaxies at high redshifts, consistent with other recent observations.
Fil: Saxena, Aayush. University of Oxford. Department of Physics; Reino Unido. University College London; Estados Unidos
Fil: Overzier, Roderik A. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil. Tno; Países Bajos. Leiden University; Países Bajos
Fil: Villar Martín, Montserrat. Consejo Superior de Investigaciones Cientificas. Centro de Astrobiologia.; España
Fil: Heckman, Tim. University Johns Hopkins; Estados Unidos
Fil: Roy, Namrata. University Johns Hopkins; Estados Unidos
Fil: Duncan, Kenneth J. University of Edinburgh; Reino Unido
Fil: Röttgering, Huub. Leiden University; Países Bajos
Fil: Miley, George. Leiden University; Países Bajos
Fil: Aydar, Catarina. Institut Max Planck Fuer Gesellschaft. Max Planck Institute For Extraterrestrial Physics.; Alemania
Fil: Best, Philip. University of Edinburgh; Reino Unido
Fil: Bosman, Sarah E. I.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. Ruprecht Karls Universitat Heidelberg; Alemania
Fil: Cameron, Alex J.. University of Oxford. Department of Physics; Reino Unido
Fil: Gabányi, Krisztina Éva. ELTE Eoẗovös Loránd University; Hungría. Hungarian Academy Of Science; Hungría. Institute Of Physics And Astronomy; Hungría
Fil: Humphrey, Andrew. Universidad de Porto. Facultad de Ciências.; Portugal. Universidade do Minho; Portugal
Fil: Morais, Sandy. Universidad de Porto. Facultad de Ciências.; Portugal
Fil: Onoue, Masafusa. Peking University; China. The University of Tokyo; Japón
Fil: Pentericci, Laura. Istituto Nazionale di Astrofisica; Italia
Fil: Reynaldi, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Venemans, Bram. Leiden University; Países Bajos - Materia
-
GALAXIES: ACTIVE
GALAXIES: JETS
GALAXIES: HIGH REDSHIFT
GALAXIES: KINEMATICS AND DYNAMICS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/265959
Ver los metadatos del registro completo
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Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWSTSaxena, AayushOverzier, Roderik AVillar Martín, MontserratHeckman, TimRoy, NamrataDuncan, Kenneth JRöttgering, HuubMiley, GeorgeAydar, CatarinaBest, PhilipBosman, Sarah E. I.Cameron, Alex J.Gabányi, Krisztina ÉvaHumphrey, AndrewMorais, SandyOnoue, MasafusaPentericci, LauraReynaldi, María VictoriaVenemans, BramGALAXIES: ACTIVEGALAXIES: JETSGALAXIES: HIGH REDSHIFTGALAXIES: KINEMATICS AND DYNAMICShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present rest-frame optical JWST Near-infrared Spectrograph (NIRSpec) integral field unit (IFU) spectroscopy of TN J1338−1942 at z = 4.1, one of the most luminous galaxies in the early universe with powerful extended radio jets. Previous observations showed evidence for strong, large-scale outflows based on its large (∼150 kpc) halo detected in Ly α, and high-velocity [O ii] emission features detected in ground-based spectroscopy. Our NIRSpec/IFU observations spatially resolve the emission line properties across the host galaxy. We find at least five concentrations of strong line emission, coinciding with discrete continuum features previously detected in imaging from Hubble Space Telescope and JWST, over an extent of ∼2 arcsec (∼15 kpc). The spectral diagnostics unambiguously trace active galactic nuclei (AGN) activity plus interaction between the interstellar medium and the radio jet as the dominant mechanisms for the ionization state and kinematics of the gas in the system. A secondary region of very high ionization lies at roughly 5 kpc away from the nucleus, and within the context of an expanding cocoon enveloping the radio lobe, this may be explained by strong shock-ionization of the entrained gas. However, it could also signal the presence of a second obscured AGN, which may offer an explanation for an intriguing outflow feature seen perpendicular to the radio axis. The presence of a dual supermassive black holes system in this galaxy would support that large galaxies in the early Universe quickly accumulated their mass through the merging of smaller units, at the centres of large overdensities. The inferred black hole mass to stellar mass ratio of 0.01−0.1 for TNJ1338 points to a more rapid assembly of black holes compared to the stellar mass of galaxies at high redshifts, consistent with other recent observations.Fil: Saxena, Aayush. University of Oxford. Department of Physics; Reino Unido. University College London; Estados UnidosFil: Overzier, Roderik A. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil. Tno; Países Bajos. Leiden University; Países BajosFil: Villar Martín, Montserrat. Consejo Superior de Investigaciones Cientificas. Centro de Astrobiologia.; EspañaFil: Heckman, Tim. University Johns Hopkins; Estados UnidosFil: Roy, Namrata. University Johns Hopkins; Estados UnidosFil: Duncan, Kenneth J. University of Edinburgh; Reino UnidoFil: Röttgering, Huub. Leiden University; Países BajosFil: Miley, George. Leiden University; Países BajosFil: Aydar, Catarina. Institut Max Planck Fuer Gesellschaft. Max Planck Institute For Extraterrestrial Physics.; AlemaniaFil: Best, Philip. University of Edinburgh; Reino UnidoFil: Bosman, Sarah E. I.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. Ruprecht Karls Universitat Heidelberg; AlemaniaFil: Cameron, Alex J.. University of Oxford. Department of Physics; Reino UnidoFil: Gabányi, Krisztina Éva. ELTE Eoẗovös Loránd University; Hungría. Hungarian Academy Of Science; Hungría. Institute Of Physics And Astronomy; HungríaFil: Humphrey, Andrew. Universidad de Porto. Facultad de Ciências.; Portugal. Universidade do Minho; PortugalFil: Morais, Sandy. Universidad de Porto. Facultad de Ciências.; PortugalFil: Onoue, Masafusa. Peking University; China. The University of Tokyo; JapónFil: Pentericci, Laura. Istituto Nazionale di Astrofisica; ItaliaFil: Reynaldi, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Venemans, Bram. Leiden University; Países BajosWiley Blackwell Publishing, Inc2024-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/265959Saxena, Aayush; Overzier, Roderik A; Villar Martín, Montserrat; Heckman, Tim; Roy, Namrata; et al.; Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 531; 4; 7-2024; 4391-44070035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/531/4/4391/7688463info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stae1406info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:36:01Zoai:ri.conicet.gov.ar:11336/265959instacron: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:34982025-09-29 09:36:01.614CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST |
| title |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST |
| spellingShingle |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST Saxena, Aayush GALAXIES: ACTIVE GALAXIES: JETS GALAXIES: HIGH REDSHIFT GALAXIES: KINEMATICS AND DYNAMICS |
| title_short |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST |
| title_full |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST |
| title_fullStr |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST |
| title_full_unstemmed |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST |
| title_sort |
Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST |
| dc.creator.none.fl_str_mv |
Saxena, Aayush Overzier, Roderik A Villar Martín, Montserrat Heckman, Tim Roy, Namrata Duncan, Kenneth J Röttgering, Huub Miley, George Aydar, Catarina Best, Philip Bosman, Sarah E. I. Cameron, Alex J. Gabányi, Krisztina Éva Humphrey, Andrew Morais, Sandy Onoue, Masafusa Pentericci, Laura Reynaldi, María Victoria Venemans, Bram |
| author |
Saxena, Aayush |
| author_facet |
Saxena, Aayush Overzier, Roderik A Villar Martín, Montserrat Heckman, Tim Roy, Namrata Duncan, Kenneth J Röttgering, Huub Miley, George Aydar, Catarina Best, Philip Bosman, Sarah E. I. Cameron, Alex J. Gabányi, Krisztina Éva Humphrey, Andrew Morais, Sandy Onoue, Masafusa Pentericci, Laura Reynaldi, María Victoria Venemans, Bram |
| author_role |
author |
| author2 |
Overzier, Roderik A Villar Martín, Montserrat Heckman, Tim Roy, Namrata Duncan, Kenneth J Röttgering, Huub Miley, George Aydar, Catarina Best, Philip Bosman, Sarah E. I. Cameron, Alex J. Gabányi, Krisztina Éva Humphrey, Andrew Morais, Sandy Onoue, Masafusa Pentericci, Laura Reynaldi, María Victoria Venemans, Bram |
| author2_role |
author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
GALAXIES: ACTIVE GALAXIES: JETS GALAXIES: HIGH REDSHIFT GALAXIES: KINEMATICS AND DYNAMICS |
| topic |
GALAXIES: ACTIVE GALAXIES: JETS GALAXIES: HIGH REDSHIFT GALAXIES: KINEMATICS AND DYNAMICS |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
We present rest-frame optical JWST Near-infrared Spectrograph (NIRSpec) integral field unit (IFU) spectroscopy of TN J1338−1942 at z = 4.1, one of the most luminous galaxies in the early universe with powerful extended radio jets. Previous observations showed evidence for strong, large-scale outflows based on its large (∼150 kpc) halo detected in Ly α, and high-velocity [O ii] emission features detected in ground-based spectroscopy. Our NIRSpec/IFU observations spatially resolve the emission line properties across the host galaxy. We find at least five concentrations of strong line emission, coinciding with discrete continuum features previously detected in imaging from Hubble Space Telescope and JWST, over an extent of ∼2 arcsec (∼15 kpc). The spectral diagnostics unambiguously trace active galactic nuclei (AGN) activity plus interaction between the interstellar medium and the radio jet as the dominant mechanisms for the ionization state and kinematics of the gas in the system. A secondary region of very high ionization lies at roughly 5 kpc away from the nucleus, and within the context of an expanding cocoon enveloping the radio lobe, this may be explained by strong shock-ionization of the entrained gas. However, it could also signal the presence of a second obscured AGN, which may offer an explanation for an intriguing outflow feature seen perpendicular to the radio axis. The presence of a dual supermassive black holes system in this galaxy would support that large galaxies in the early Universe quickly accumulated their mass through the merging of smaller units, at the centres of large overdensities. The inferred black hole mass to stellar mass ratio of 0.01−0.1 for TNJ1338 points to a more rapid assembly of black holes compared to the stellar mass of galaxies at high redshifts, consistent with other recent observations. Fil: Saxena, Aayush. University of Oxford. Department of Physics; Reino Unido. University College London; Estados Unidos Fil: Overzier, Roderik A. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil. Tno; Países Bajos. Leiden University; Países Bajos Fil: Villar Martín, Montserrat. Consejo Superior de Investigaciones Cientificas. Centro de Astrobiologia.; España Fil: Heckman, Tim. University Johns Hopkins; Estados Unidos Fil: Roy, Namrata. University Johns Hopkins; Estados Unidos Fil: Duncan, Kenneth J. University of Edinburgh; Reino Unido Fil: Röttgering, Huub. Leiden University; Países Bajos Fil: Miley, George. Leiden University; Países Bajos Fil: Aydar, Catarina. Institut Max Planck Fuer Gesellschaft. Max Planck Institute For Extraterrestrial Physics.; Alemania Fil: Best, Philip. University of Edinburgh; Reino Unido Fil: Bosman, Sarah E. I.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. Ruprecht Karls Universitat Heidelberg; Alemania Fil: Cameron, Alex J.. University of Oxford. Department of Physics; Reino Unido Fil: Gabányi, Krisztina Éva. ELTE Eoẗovös Loránd University; Hungría. Hungarian Academy Of Science; Hungría. Institute Of Physics And Astronomy; Hungría Fil: Humphrey, Andrew. Universidad de Porto. Facultad de Ciências.; Portugal. Universidade do Minho; Portugal Fil: Morais, Sandy. Universidad de Porto. Facultad de Ciências.; Portugal Fil: Onoue, Masafusa. Peking University; China. The University of Tokyo; Japón Fil: Pentericci, Laura. Istituto Nazionale di Astrofisica; Italia Fil: Reynaldi, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Venemans, Bram. Leiden University; Países Bajos |
| description |
We present rest-frame optical JWST Near-infrared Spectrograph (NIRSpec) integral field unit (IFU) spectroscopy of TN J1338−1942 at z = 4.1, one of the most luminous galaxies in the early universe with powerful extended radio jets. Previous observations showed evidence for strong, large-scale outflows based on its large (∼150 kpc) halo detected in Ly α, and high-velocity [O ii] emission features detected in ground-based spectroscopy. Our NIRSpec/IFU observations spatially resolve the emission line properties across the host galaxy. We find at least five concentrations of strong line emission, coinciding with discrete continuum features previously detected in imaging from Hubble Space Telescope and JWST, over an extent of ∼2 arcsec (∼15 kpc). The spectral diagnostics unambiguously trace active galactic nuclei (AGN) activity plus interaction between the interstellar medium and the radio jet as the dominant mechanisms for the ionization state and kinematics of the gas in the system. A secondary region of very high ionization lies at roughly 5 kpc away from the nucleus, and within the context of an expanding cocoon enveloping the radio lobe, this may be explained by strong shock-ionization of the entrained gas. However, it could also signal the presence of a second obscured AGN, which may offer an explanation for an intriguing outflow feature seen perpendicular to the radio axis. The presence of a dual supermassive black holes system in this galaxy would support that large galaxies in the early Universe quickly accumulated their mass through the merging of smaller units, at the centres of large overdensities. The inferred black hole mass to stellar mass ratio of 0.01−0.1 for TNJ1338 points to a more rapid assembly of black holes compared to the stellar mass of galaxies at high redshifts, consistent with other recent observations. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024-07 |
| 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/11336/265959 Saxena, Aayush; Overzier, Roderik A; Villar Martín, Montserrat; Heckman, Tim; Roy, Namrata; et al.; Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 531; 4; 7-2024; 4391-4407 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/265959 |
| identifier_str_mv |
Saxena, Aayush; Overzier, Roderik A; Villar Martín, Montserrat; Heckman, Tim; Roy, Namrata; et al.; Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 531; 4; 7-2024; 4391-4407 0035-8711 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://academic.oup.com/mnras/article/531/4/4391/7688463 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stae1406 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by/2.5/ar/ |
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application/pdf application/pdf |
| dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
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Wiley Blackwell Publishing, Inc |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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