V. Mainieri, C. Circosta, D. Kakkad, Michele Perna, G. Vietri, A. Bongiorno, M. Brusa, S. Carniani, C. Cicone, F. Civano, A. Comastri, G. Cresci, C. Feruglio, F. Fiore, A. Georgakakis, C. Harrison, B. Husemann, A. Lamastra, I. Lamperti, G. Lanzuisi, F. Mannucci, A. Marconi, N. Menci, A. Merloni, H. Netzer, P. Padovani, E. Piconcelli, A. Puglisi, M. Salvato, J. Scholtz, M. Schramm, J. Silverman, C. Vignali, G. Zamorani, L. Zappacosta
{"title":"宇宙正午的超级AGN反馈:一个多阶段和多尺度的挑战","authors":"V. Mainieri, C. Circosta, D. Kakkad, Michele Perna, G. Vietri, A. Bongiorno, M. Brusa, S. Carniani, C. Cicone, F. Civano, A. Comastri, G. Cresci, C. Feruglio, F. Fiore, A. Georgakakis, C. Harrison, B. Husemann, A. Lamastra, I. Lamperti, G. Lanzuisi, F. Mannucci, A. Marconi, N. Menci, A. Merloni, H. Netzer, P. Padovani, E. Piconcelli, A. Puglisi, M. Salvato, J. Scholtz, M. Schramm, J. Silverman, C. Vignali, G. Zamorani, L. Zappacosta","doi":"10.18727/0722-6691/5222","DOIUrl":null,"url":null,"abstract":"Theoretical models of galaxy evolution suggest that galaxy-wide outflows driven by active galactic nuclei (AGN), one of the so-called AGN-feedback mechanisms, are a fundamental process affecting the bulk of the baryons in the Universe. While the presence of such outflows out to kpc scales is now undisputed, their impact on the star formation, gas content and kinematics of the host galaxy is hotly debated. Here we report on the results from our Large Programme SUPER, which used the Spectrograph for INtegral Field Observations in the Near INfrared (SINFONI) on the Very Large Telescope (VLT) to carry out the first statistically sound high-spatialresolution investigation of AGN outflows at z ~ 2, covering four orders of magnitude in AGN bolometric luminosity.","PeriodicalId":41738,"journal":{"name":"Jurnal The Messenger","volume":"231 1","pages":"45-49"},"PeriodicalIF":0.3000,"publicationDate":"2021-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"SUPER — AGN feedback at cosmic noon: a multi-phase and multi-scale challenge\",\"authors\":\"V. Mainieri, C. Circosta, D. Kakkad, Michele Perna, G. Vietri, A. Bongiorno, M. Brusa, S. Carniani, C. Cicone, F. Civano, A. Comastri, G. Cresci, C. Feruglio, F. Fiore, A. Georgakakis, C. Harrison, B. Husemann, A. Lamastra, I. Lamperti, G. Lanzuisi, F. Mannucci, A. Marconi, N. Menci, A. Merloni, H. Netzer, P. Padovani, E. Piconcelli, A. Puglisi, M. Salvato, J. Scholtz, M. Schramm, J. Silverman, C. Vignali, G. Zamorani, L. Zappacosta\",\"doi\":\"10.18727/0722-6691/5222\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Theoretical models of galaxy evolution suggest that galaxy-wide outflows driven by active galactic nuclei (AGN), one of the so-called AGN-feedback mechanisms, are a fundamental process affecting the bulk of the baryons in the Universe. While the presence of such outflows out to kpc scales is now undisputed, their impact on the star formation, gas content and kinematics of the host galaxy is hotly debated. Here we report on the results from our Large Programme SUPER, which used the Spectrograph for INtegral Field Observations in the Near INfrared (SINFONI) on the Very Large Telescope (VLT) to carry out the first statistically sound high-spatialresolution investigation of AGN outflows at z ~ 2, covering four orders of magnitude in AGN bolometric luminosity.\",\"PeriodicalId\":41738,\"journal\":{\"name\":\"Jurnal The Messenger\",\"volume\":\"231 1\",\"pages\":\"45-49\"},\"PeriodicalIF\":0.3000,\"publicationDate\":\"2021-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Jurnal The Messenger\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.18727/0722-6691/5222\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"COMMUNICATION\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Jurnal The Messenger","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.18727/0722-6691/5222","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"COMMUNICATION","Score":null,"Total":0}
SUPER — AGN feedback at cosmic noon: a multi-phase and multi-scale challenge
Theoretical models of galaxy evolution suggest that galaxy-wide outflows driven by active galactic nuclei (AGN), one of the so-called AGN-feedback mechanisms, are a fundamental process affecting the bulk of the baryons in the Universe. While the presence of such outflows out to kpc scales is now undisputed, their impact on the star formation, gas content and kinematics of the host galaxy is hotly debated. Here we report on the results from our Large Programme SUPER, which used the Spectrograph for INtegral Field Observations in the Near INfrared (SINFONI) on the Very Large Telescope (VLT) to carry out the first statistically sound high-spatialresolution investigation of AGN outflows at z ~ 2, covering four orders of magnitude in AGN bolometric luminosity.
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