{"status":"public","day":"04","main_file_link":[{"url":"https://doi.org/10.1007/s10686-021-09709-9","open_access":"1"}],"date_published":"2021-09-04T00:00:00Z","article_type":"original","issue":"3","language":[{"iso":"eng"}],"page":"1333-1383","author":[{"full_name":"Sesana, Alberto","first_name":"Alberto","last_name":"Sesana"},{"last_name":"Korsakova","first_name":"Natalia","full_name":"Korsakova, Natalia"},{"last_name":"Sedda","full_name":"Sedda, Manuel Arca","first_name":"Manuel Arca"},{"last_name":"Baibhav","full_name":"Baibhav, Vishal","first_name":"Vishal"},{"last_name":"Barausse","full_name":"Barausse, Enrico","first_name":"Enrico"},{"last_name":"Barke","full_name":"Barke, Simon","first_name":"Simon"},{"last_name":"Berti","first_name":"Emanuele","full_name":"Berti, Emanuele"},{"full_name":"Bonetti, Matteo","first_name":"Matteo","last_name":"Bonetti"},{"last_name":"Capelo","first_name":"Pedro R.","full_name":"Capelo, Pedro R."},{"last_name":"Caprini","first_name":"Chiara","full_name":"Caprini, Chiara"},{"last_name":"Garcia-Bellido","first_name":"Juan","full_name":"Garcia-Bellido, Juan"},{"first_name":"Zoltán","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"first_name":"Karan","full_name":"Jani, Karan","last_name":"Jani"},{"first_name":"Oliver","full_name":"Jennrich, Oliver","last_name":"Jennrich"},{"first_name":"Peter H.","full_name":"Johansson, Peter H.","last_name":"Johansson"},{"first_name":"Fazeel Mahmood","full_name":"Khan, Fazeel Mahmood","last_name":"Khan"},{"full_name":"Korol, Valeriya","first_name":"Valeriya","last_name":"Korol"},{"last_name":"Lamberts","full_name":"Lamberts, Astrid","first_name":"Astrid"},{"last_name":"Lupi","first_name":"Alessandro","full_name":"Lupi, Alessandro"},{"last_name":"Mangiagli","first_name":"Alberto","full_name":"Mangiagli, Alberto"},{"last_name":"Mayer","first_name":"Lucio","full_name":"Mayer, Lucio"},{"first_name":"Germano","full_name":"Nardini, Germano","last_name":"Nardini"},{"last_name":"Pacucci","full_name":"Pacucci, Fabio","first_name":"Fabio"},{"full_name":"Petiteau, Antoine","first_name":"Antoine","last_name":"Petiteau"},{"last_name":"Raccanelli","full_name":"Raccanelli, Alvise","first_name":"Alvise"},{"last_name":"Rajendran","full_name":"Rajendran, Surjeet","first_name":"Surjeet"},{"last_name":"Regan","full_name":"Regan, John","first_name":"John"},{"last_name":"Shao","full_name":"Shao, Lijing","first_name":"Lijing"},{"last_name":"Spallicci","full_name":"Spallicci, Alessandro","first_name":"Alessandro"},{"last_name":"Tamanini","full_name":"Tamanini, Nicola","first_name":"Nicola"},{"first_name":"Marta","full_name":"Volonteri, Marta","last_name":"Volonteri"},{"first_name":"Niels","full_name":"Warburton, Niels","last_name":"Warburton"},{"last_name":"Wong","first_name":"Kaze","full_name":"Wong, Kaze"},{"last_name":"Zumalacarregui","first_name":"Miguel","full_name":"Zumalacarregui, Miguel"}],"date_created":"2024-09-05T09:42:29Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publisher":"Springer Science and Business Media LLC","type":"journal_article","oa_version":"Published Version","citation":{"mla":"Sesana, Alberto, et al. “Unveiling the Gravitational Universe at μ-Hz Frequencies.” <i>Experimental Astronomy</i>, vol. 51, no. 3, Springer Science and Business Media LLC, 2021, pp. 1333–83, doi:<a href=\"https://doi.org/10.1007/s10686-021-09709-9\">10.1007/s10686-021-09709-9</a>.","ieee":"A. Sesana <i>et al.</i>, “Unveiling the gravitational universe at μ-Hz frequencies,” <i>Experimental Astronomy</i>, vol. 51, no. 3. Springer Science and Business Media LLC, pp. 1333–1383, 2021.","ista":"Sesana A, Korsakova N, Sedda MA, Baibhav V, Barausse E, Barke S, Berti E, Bonetti M, Capelo PR, Caprini C, Garcia-Bellido J, Haiman Z, Jani K, Jennrich O, Johansson PH, Khan FM, Korol V, Lamberts A, Lupi A, Mangiagli A, Mayer L, Nardini G, Pacucci F, Petiteau A, Raccanelli A, Rajendran S, Regan J, Shao L, Spallicci A, Tamanini N, Volonteri M, Warburton N, Wong K, Zumalacarregui M. 2021. Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy. 51(3), 1333–1383.","apa":"Sesana, A., Korsakova, N., Sedda, M. A., Baibhav, V., Barausse, E., Barke, S., … Zumalacarregui, M. (2021). Unveiling the gravitational universe at μ-Hz frequencies. <i>Experimental Astronomy</i>. Springer Science and Business Media LLC. <a href=\"https://doi.org/10.1007/s10686-021-09709-9\">https://doi.org/10.1007/s10686-021-09709-9</a>","ama":"Sesana A, Korsakova N, Sedda MA, et al. Unveiling the gravitational universe at μ-Hz frequencies. <i>Experimental Astronomy</i>. 2021;51(3):1333-1383. doi:<a href=\"https://doi.org/10.1007/s10686-021-09709-9\">10.1007/s10686-021-09709-9</a>","short":"A. Sesana, N. Korsakova, M.A. Sedda, V. Baibhav, E. Barausse, S. Barke, E. Berti, M. Bonetti, P.R. Capelo, C. Caprini, J. Garcia-Bellido, Z. Haiman, K. Jani, O. Jennrich, P.H. Johansson, F.M. Khan, V. Korol, A. Lamberts, A. Lupi, A. Mangiagli, L. Mayer, G. Nardini, F. Pacucci, A. Petiteau, A. Raccanelli, S. Rajendran, J. Regan, L. Shao, A. Spallicci, N. Tamanini, M. Volonteri, N. Warburton, K. Wong, M. Zumalacarregui, Experimental Astronomy 51 (2021) 1333–1383.","chicago":"Sesana, Alberto, Natalia Korsakova, Manuel Arca Sedda, Vishal Baibhav, Enrico Barausse, Simon Barke, Emanuele Berti, et al. “Unveiling the Gravitational Universe at μ-Hz Frequencies.” <i>Experimental Astronomy</i>. Springer Science and Business Media LLC, 2021. <a href=\"https://doi.org/10.1007/s10686-021-09709-9\">https://doi.org/10.1007/s10686-021-09709-9</a>."},"date_updated":"2024-09-11T14:53:17Z","quality_controlled":"1","scopus_import":"1","month":"09","publication":"Experimental Astronomy","year":"2021","publication_identifier":{"issn":["0922-6435","1572-9508"]},"doi":"10.1007/s10686-021-09709-9","oa":1,"volume":51,"extern":"1","_id":"17534","title":"Unveiling the gravitational universe at μ-Hz frequencies","publication_status":"published","abstract":[{"text":"We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a μ-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe.","lang":"eng"}],"intvolume":"        51","article_processing_charge":"No"}