New hope for obscured AGN: the PRIMA-NewAthena alliance
The software POMPA was utilized to estimate the AGN density is available here. The NewAthena responses and background can be accessed in the link. The SEDs utilized in this work were obtained from Delvecchio et al. (2015)95 and can be provided upon request. The latest PRIMA capabilities can be found...
| Autores: | , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/406466 |
| Acceso en línea: | http://hdl.handle.net/10261/406466 |
| Access Level: | acceso abierto |
| Palabra clave: | Infrared space observatory Hyperspectral imaging Infrared imaging X-rays |
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New hope for obscured AGN: the PRIMA-NewAthena alliance |
| title |
New hope for obscured AGN: the PRIMA-NewAthena alliance |
| spellingShingle |
New hope for obscured AGN: the PRIMA-NewAthena alliance Barchiesi, Luigi Infrared space observatory Hyperspectral imaging Infrared imaging X-rays |
| title_short |
New hope for obscured AGN: the PRIMA-NewAthena alliance |
| title_full |
New hope for obscured AGN: the PRIMA-NewAthena alliance |
| title_fullStr |
New hope for obscured AGN: the PRIMA-NewAthena alliance |
| title_full_unstemmed |
New hope for obscured AGN: the PRIMA-NewAthena alliance |
| title_sort |
New hope for obscured AGN: the PRIMA-NewAthena alliance |
| dc.creator.none.fl_str_mv |
Barchiesi, Luigi Carrera, Francisco J. Vignali, Cristian Pozzi, Francesca Marchetti, Lucia Gruppioni, Carlotta Delvecchio, Ivan Bisigello, Laura Calura, Francesco Aird, James Vaccari, Mattia |
| author |
Barchiesi, Luigi |
| author_facet |
Barchiesi, Luigi Carrera, Francisco J. Vignali, Cristian Pozzi, Francesca Marchetti, Lucia Gruppioni, Carlotta Delvecchio, Ivan Bisigello, Laura Calura, Francesco Aird, James Vaccari, Mattia |
| author_role |
author |
| author2 |
Carrera, Francisco J. Vignali, Cristian Pozzi, Francesca Marchetti, Lucia Gruppioni, Carlotta Delvecchio, Ivan Bisigello, Laura Calura, Francesco Aird, James Vaccari, Mattia |
| author2_role |
author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Inter-University Centre for Astronomy and Astrophysics (India) University of Cape Town University of Pretoria University of Western Cape National Research Foundation (South Africa) Department of Science and Innovation (South Africa) Agencia Estatal de Investigación (España) Ministerio de Ciencia, Innovación y Universidades (España) European Commission Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Infrared space observatory Hyperspectral imaging Infrared imaging X-rays |
| topic |
Infrared space observatory Hyperspectral imaging Infrared imaging X-rays |
| description |
The software POMPA was utilized to estimate the AGN density is available here. The NewAthena responses and background can be accessed in the link. The SEDs utilized in this work were obtained from Delvecchio et al. (2015)95 and can be provided upon request. The latest PRIMA capabilities can be found here. |
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2025 |
| dc.date.none.fl_str_mv |
2025 2025 2025 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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http://hdl.handle.net/10261/406466 |
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Inglés |
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Inglés |
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info:eu-repo/semantics/openAccess |
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openAccess |
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SPIE digital library |
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SPIE digital library |
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New hope for obscured AGN: the PRIMA-NewAthena allianceBarchiesi, LuigiCarrera, Francisco J.Vignali, CristianPozzi, FrancescaMarchetti, LuciaGruppioni, CarlottaDelvecchio, IvanBisigello, LauraCalura, FrancescoAird, JamesVaccari, MattiaInfrared space observatoryHyperspectral imagingInfrared imagingX-raysThe software POMPA was utilized to estimate the AGN density is available here. The NewAthena responses and background can be accessed in the link. The SEDs utilized in this work were obtained from Delvecchio et al. (2015)95 and can be provided upon request. The latest PRIMA capabilities can be found here.Understanding the AGN-galaxy co-evolution, feedback processes, and the evolution of Black Hole Accretion rate Density (BHAD) requires accurately estimating the contribution of obscured Active Galactic Nuclei (AGN). However, detecting these sources is challenging due to significant extinction at the wavelengths typically used to trace their emission. We evaluate the capabilities of the proposed far-infrared observatory PRIMA and its synergies with the X-ray observatory NewAthena in detecting AGN and in measuring the BHAD. Starting from X-ray background synthesis models, we simulate the performance of NewAthena and of PRIMA in Deep and Wide surveys. Our results show that the combination of these facilities is a powerful tool for selecting and characterizing all types of AGN. Although NewAthena is particularly effective at detecting the most luminous, the unobscured, and the moderately obscured AGN, PRIMA excels at identifying heavily obscured sources, including Compton-thick AGN (of which we expect 7500 detections per deg2). We find that PRIMA will detect ∼60 times more sources than Herschel over the same area and will allow us to accurately measure the BHAD evolution up to z∼8, better than any current IR or X-ray survey, finally revealing the true contribution of Compton-thick AGN to the BHAD evolution.LB, LM, and MV acknowledge financial support from the Inter-University Institute for Data Intensive Astronomy (IDIA), a partnership of the University of Cape Town, the University of Pretoria and the University of the Western Cape, and from the South African Department of Science and Innovation’s National Research Foundation under the ISARP RADIOMAP Joint Research Scheme (DSI-NRF Grant No. 150551) and the Competitive Programme for Rated Researchers (CPRR) HELP-IDIA Panchromatic PrOject (HIPPO) Project (DSI-NRF Grant No. SRUG22031677). FJC acknowledges funding from grant PID2021-122955OB-C41 funded by MCIN/AEI/10.13039/501100011033 and by ERDF A way of making Europe. Part of the research activities described in this paper was carried out with the contribution of the NextGenerationEU funds within the National Recovery and Resilience Plan (PNRR), Mission 4 - Education and Research, Component 2 - from Research to Business (M4C2), Investment Line 3.1 - Strengthening and creation of Research Infrastructures, and Project IR0000034 - “STILES - Strengthening the Italian Leadership in ELT and SKA.” ID acknowledges funding by the European Union - NextGenerationEU, RRF M4C2 1.1, Project No. 2022JZJBHM: “AGN-sCAN: zooming-in on the AGN-galaxy connection since the cosmic noon” - CUP C53D23001120006.Peer reviewedSPIE digital libraryInter-University Centre for Astronomy and Astrophysics (India)University of Cape TownUniversity of PretoriaUniversity of Western CapeNational Research Foundation (South Africa)Department of Science and Innovation (South Africa)Agencia Estatal de Investigación (España)Ministerio de Ciencia, Innovación y Universidades (España)European CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/406466reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-122955OB-C41https://doi.org/10.1117/1.JATIS.11.3.031609Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/4064662026-05-22T06:33:51Z |
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