[{"publication_status":"published","article_type":"original","author":[{"full_name":"Su, Kung-Yi","first_name":"Kung-Yi","last_name":"Su"},{"last_name":"Bryan","full_name":"Bryan, Greg L","first_name":"Greg L"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"first_name":"Rachel S","full_name":"Somerville, Rachel S","last_name":"Somerville"},{"last_name":"Hayward","first_name":"Christopher C","full_name":"Hayward, Christopher C"},{"last_name":"Faucher-Giguère","first_name":"Claude-André","full_name":"Faucher-Giguère, Claude-André"}],"oa_version":"Published Version","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad252"}],"issue":"3","intvolume":"       520","month":"01","article_processing_charge":"No","oa":1,"year":"2023","publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","date_created":"2024-09-05T09:22:35Z","extern":"1","citation":{"mla":"Su, Kung-Yi, et al. “Self-Regulation of Black Hole Accretion via Jets in Early Protogalaxies.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 520, no. 3, Oxford University Press, 2023, pp. 4258–75, doi:<a href=\"https://doi.org/10.1093/mnras/stad252\">10.1093/mnras/stad252</a>.","ama":"Su K-Y, Bryan GL, Haiman Z, Somerville RS, Hayward CC, Faucher-Giguère C-A. Self-regulation of black hole accretion via jets in early protogalaxies. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;520(3):4258-4275. doi:<a href=\"https://doi.org/10.1093/mnras/stad252\">10.1093/mnras/stad252</a>","ista":"Su K-Y, Bryan GL, Haiman Z, Somerville RS, Hayward CC, Faucher-Giguère C-A. 2023. Self-regulation of black hole accretion via jets in early protogalaxies. Monthly Notices of the Royal Astronomical Society. 520(3), 4258–4275.","chicago":"Su, Kung-Yi, Greg L Bryan, Zoltán Haiman, Rachel S Somerville, Christopher C Hayward, and Claude-André Faucher-Giguère. “Self-Regulation of Black Hole Accretion via Jets in Early Protogalaxies.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnras/stad252\">https://doi.org/10.1093/mnras/stad252</a>.","apa":"Su, K.-Y., Bryan, G. L., Haiman, Z., Somerville, R. S., Hayward, C. C., &#38; Faucher-Giguère, C.-A. (2023). Self-regulation of black hole accretion via jets in early protogalaxies. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stad252\">https://doi.org/10.1093/mnras/stad252</a>","ieee":"K.-Y. Su, G. L. Bryan, Z. Haiman, R. S. Somerville, C. C. Hayward, and C.-A. Faucher-Giguère, “Self-regulation of black hole accretion via jets in early protogalaxies,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 520, no. 3. Oxford University Press, pp. 4258–4275, 2023.","short":"K.-Y. Su, G.L. Bryan, Z. Haiman, R.S. Somerville, C.C. Hayward, C.-A. Faucher-Giguère, Monthly Notices of the Royal Astronomical Society 520 (2023) 4258–4275."},"quality_controlled":"1","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":520,"day":"27","date_published":"2023-01-27T00:00:00Z","fulldoi":"https://doi.org/10.1093/mnras/stad252","language":[{"iso":"eng"}],"abstract":[{"text":"The early growth of black holes (BHs) in high-redshift galaxies is likely feedback regulated. While radiative feedback has been extensively studied, the role of mechanical feedback has received less scrutiny to date. Here, we use high-resolution parsec-scale hydrodynamical simulations to study jet propagation and its effect on 100 M⊙ BH accretion in the dense, low-metallicity gas expected in early protogalaxies. As the jet propagates, it shocks the surrounding gas forming a jet cocoon. The cocoon consists of a rapidly cooling cold phase at the interface with the background gas and an overpressured subsonic phase of reverse shock-heated gas filling the interior. We vary the background gas density and temperature, BH feedback efficiency, and the jet model. We found that the width of the jet cocoon roughly follows a scaling derived by assuming momentum conservation in the jet-propagation direction and energy conservation in the lateral directions. Depending on the assumed gas and jet properties, the cocoon either stays elongated to large radii or isotropizes before reaching the Bondi radius, forming a nearly spherical bubble. Lower jet velocities and higher background gas densities result in self-regulation to higher momentum fluxes and elongated cocoons. In all cases, the outward cocoon momentum flux balances the inward inflowing gas momentum flux near the Bondi radius, which ultimately regulates BH accretion. The time-averaged accretion rate always remains below the Bondi rate, and exceeds the Eddington rate only if the ambient medium is dense and cold, and/or the jet is weak (low velocity and mass loading).","lang":"eng"}],"title":"Self-regulation of black hole accretion via jets in early protogalaxies","date_updated":"2024-09-11T07:39:21Z","page":"4258-4275","type":"journal_article","_id":"17522","status":"public","doi":"10.1093/mnras/stad252","publisher":"Oxford University Press","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345"},{"day":"05","date_published":"2023-09-05T00:00:00Z","fulldoi":"https://doi.org/10.1093/mnras/stad2616","language":[{"iso":"eng"}],"type":"journal_article","_id":"17527","status":"public","doi":"10.1093/mnras/stad2616","publisher":"Oxford University Press","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"text":"The origin of the recently discovered new class of transients, X-ray quasi-periodic eruptions (QPEs), remains a puzzle. Due to their periodicity and association with active galactic nuclei (AGNs), it is natural to relate these eruptions to stars or compact objects in tight orbits around supermassive black holes (SMBHs). In this paper, we predict the properties of emission from bow shocks produced by stars crossing AGN discs, and compare them to the observed properties of QPEs. We find that when a star’s orbit is retrograde and has a low inclination (≲40°) with respect to the AGN disc and the star is massive (≳10 M⊙), the breakout emission from the bow shock can explain the observed duration (∼hours) and X-ray luminosity (∼few × 1042 erg s−1) of QPEs. This model can further explain various observed features of QPEs, such as their complex luminosity evolution, the gradual decline of luminosity of the flares over several years, the evolution of the hardness ratio, the modulation of the luminosity during quiescent phases, and the preference of the central SMBHs to have low masses.","lang":"eng"}],"title":"Flares from stars crossing active galactic nucleus discs on low-inclination orbits","page":"69-79","date_updated":"2024-09-11T08:52:17Z","intvolume":"       526","issue":"1","oa_version":"Published Version","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stad2616","open_access":"1"}],"month":"09","article_processing_charge":"No","oa":1,"year":"2023","publication_status":"published","article_type":"original","author":[{"first_name":"Hiromichi","full_name":"Tagawa, Hiromichi","last_name":"Tagawa"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"}],"quality_controlled":"1","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":526,"publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","date_created":"2024-09-05T09:30:18Z","extern":"1","citation":{"ista":"Tagawa H, Haiman Z. 2023. Flares from stars crossing active galactic nucleus discs on low-inclination orbits. Monthly Notices of the Royal Astronomical Society. 526(1), 69–79.","ama":"Tagawa H, Haiman Z. Flares from stars crossing active galactic nucleus discs on low-inclination orbits. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;526(1):69-79. doi:<a href=\"https://doi.org/10.1093/mnras/stad2616\">10.1093/mnras/stad2616</a>","mla":"Tagawa, Hiromichi, and Zoltán Haiman. “Flares from Stars Crossing Active Galactic Nucleus Discs on Low-Inclination Orbits.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 526, no. 1, Oxford University Press, 2023, pp. 69–79, doi:<a href=\"https://doi.org/10.1093/mnras/stad2616\">10.1093/mnras/stad2616</a>.","short":"H. Tagawa, Z. Haiman, Monthly Notices of the Royal Astronomical Society 526 (2023) 69–79.","apa":"Tagawa, H., &#38; Haiman, Z. (2023). Flares from stars crossing active galactic nucleus discs on low-inclination orbits. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stad2616\">https://doi.org/10.1093/mnras/stad2616</a>","ieee":"H. Tagawa and Z. Haiman, “Flares from stars crossing active galactic nucleus discs on low-inclination orbits,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 526, no. 1. Oxford University Press, pp. 69–79, 2023.","chicago":"Tagawa, Hiromichi, and Zoltán Haiman. “Flares from Stars Crossing Active Galactic Nucleus Discs on Low-Inclination Orbits.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnras/stad2616\">https://doi.org/10.1093/mnras/stad2616</a>."}},{"day":"10","date_published":"2023-05-10T00:00:00Z","fulldoi":"https://doi.org/10.1093/mnras/stad1412","language":[{"iso":"eng"}],"type":"journal_article","_id":"17539","status":"public","doi":"10.1093/mnras/stad1412","publisher":"Oxford University Press","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"text":"In this paper, we study how gaseous dynamical friction (DF) affects the motion of fly-by stellar-mass black holes (sBHs) embedded in active galactic nucleus (AGN) discs. We perform three-body integrations of the interaction of two co-planar sBHs in nearby, initially circular orbits around the supermassive black hole. We find that DF can facilitate the formation of gravitationally bound near-Keplerian binaries in AGN discs, and we delineate the discrete ranges of impact parameters and AGN disc parameters for which such captures occur. We also report trends in the bound binaries’ eccentricity and sense of rotation (prograde or retrograde with respect to the background AGN disc) as a function of the impact parameter of the initial encounter. While based on an approximate description of gaseous friction, our results suggest that binary formation in AGN discs should be common and may produce both prograde and retrograde, as well as both circular and eccentric binaries.","lang":"eng"}],"title":"Gas dynamical friction as a binary formation mechanism in AGN discs","page":"1126-1139","date_updated":"2024-09-12T09:46:18Z","issue":"1","intvolume":"       523","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad1412"}],"oa_version":"Published Version","month":"05","article_processing_charge":"No","year":"2023","oa":1,"publication_status":"published","article_type":"original","author":[{"full_name":"DeLaurentiis, Stanislav","first_name":"Stanislav","last_name":"DeLaurentiis"},{"full_name":"Epstein-Martin, Marguerite","first_name":"Marguerite","last_name":"Epstein-Martin"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán","last_name":"Haiman"}],"quality_controlled":"1","volume":523,"publication_identifier":{"issn":["0035-8711","1365-2966"]},"publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","date_created":"2024-09-05T09:53:03Z","extern":"1","citation":{"chicago":"DeLaurentiis, Stanislav, Marguerite Epstein-Martin, and Zoltán Haiman. “Gas Dynamical Friction as a Binary Formation Mechanism in AGN Discs.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnras/stad1412\">https://doi.org/10.1093/mnras/stad1412</a>.","ieee":"S. DeLaurentiis, M. Epstein-Martin, and Z. Haiman, “Gas dynamical friction as a binary formation mechanism in AGN discs,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 523, no. 1. Oxford University Press, pp. 1126–1139, 2023.","apa":"DeLaurentiis, S., Epstein-Martin, M., &#38; Haiman, Z. (2023). Gas dynamical friction as a binary formation mechanism in AGN discs. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stad1412\">https://doi.org/10.1093/mnras/stad1412</a>","short":"S. DeLaurentiis, M. Epstein-Martin, Z. Haiman, Monthly Notices of the Royal Astronomical Society 523 (2023) 1126–1139.","mla":"DeLaurentiis, Stanislav, et al. “Gas Dynamical Friction as a Binary Formation Mechanism in AGN Discs.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 523, no. 1, Oxford University Press, 2023, pp. 1126–39, doi:<a href=\"https://doi.org/10.1093/mnras/stad1412\">10.1093/mnras/stad1412</a>.","ama":"DeLaurentiis S, Epstein-Martin M, Haiman Z. Gas dynamical friction as a binary formation mechanism in AGN discs. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;523(1):1126-1139. doi:<a href=\"https://doi.org/10.1093/mnras/stad1412\">10.1093/mnras/stad1412</a>","ista":"DeLaurentiis S, Epstein-Martin M, Haiman Z. 2023. Gas dynamical friction as a binary formation mechanism in AGN discs. Monthly Notices of the Royal Astronomical Society. 523(1), 1126–1139."}},{"article_processing_charge":"No","oa":1,"year":"2023","month":"04","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad1070"}],"intvolume":"       522","issue":"1","oa_version":"Published Version","publication_status":"published","article_type":"original","author":[{"first_name":"Alessia","full_name":"Franchini, Alessia","last_name":"Franchini"},{"first_name":"Alessandro","full_name":"Lupi, Alessandro","last_name":"Lupi"},{"last_name":"Sesana","first_name":"Alberto","full_name":"Sesana, Alberto"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"}],"volume":522,"publication_identifier":{"issn":["0035-8711","1365-2966"]},"quality_controlled":"1","citation":{"ama":"Franchini A, Lupi A, Sesana A, Haiman Z. The importance of live binary evolution in numerical simulations of binaries embedded in circumbinary discs. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;522(1):1569-1574. doi:<a href=\"https://doi.org/10.1093/mnras/stad1070\">10.1093/mnras/stad1070</a>","mla":"Franchini, Alessia, et al. “The Importance of Live Binary Evolution in Numerical Simulations of Binaries Embedded in Circumbinary Discs.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 522, no. 1, Oxford University Press, 2023, pp. 1569–74, doi:<a href=\"https://doi.org/10.1093/mnras/stad1070\">10.1093/mnras/stad1070</a>.","ista":"Franchini A, Lupi A, Sesana A, Haiman Z. 2023. The importance of live binary evolution in numerical simulations of binaries embedded in circumbinary discs. Monthly Notices of the Royal Astronomical Society. 522(1), 1569–1574.","chicago":"Franchini, Alessia, Alessandro Lupi, Alberto Sesana, and Zoltán Haiman. “The Importance of Live Binary Evolution in Numerical Simulations of Binaries Embedded in Circumbinary Discs.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnras/stad1070\">https://doi.org/10.1093/mnras/stad1070</a>.","short":"A. Franchini, A. Lupi, A. Sesana, Z. Haiman, Monthly Notices of the Royal Astronomical Society 522 (2023) 1569–1574.","ieee":"A. Franchini, A. Lupi, A. Sesana, and Z. Haiman, “The importance of live binary evolution in numerical simulations of binaries embedded in circumbinary discs,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 522, no. 1. Oxford University Press, pp. 1569–1574, 2023.","apa":"Franchini, A., Lupi, A., Sesana, A., &#38; Haiman, Z. (2023). The importance of live binary evolution in numerical simulations of binaries embedded in circumbinary discs. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stad1070\">https://doi.org/10.1093/mnras/stad1070</a>"},"extern":"1","scopus_import":"1","date_created":"2024-09-05T10:08:46Z","publication":"Monthly Notices of the Royal Astronomical Society","fulldoi":"https://doi.org/10.1093/mnras/stad1070","language":[{"iso":"eng"}],"day":"12","date_published":"2023-04-12T00:00:00Z","publisher":"Oxford University Press","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","doi":"10.1093/mnras/stad1070","type":"journal_article","_id":"17548","status":"public","page":"1569-1574","date_updated":"2024-09-18T09:30:21Z","title":"The importance of live binary evolution in numerical simulations of binaries embedded in circumbinary discs","abstract":[{"text":"The shrinking of a binary orbit driven by the interaction with a gaseous circumbinary disc, initially advocated as a potential way to catalyse the binary merger, has recently been debated in the case of geometrically thick (i.e. with H/R ≳ 0.1) discs. However, a clear consensus is still missing mainly owing to numerical limitations, such as fixed orbit binaries or lack of resolution inside the cavity carved by the binary in its circumbinary disc. In this work, we assess the importance of evolving the binary orbit by means of hydrodynamic simulations performed with the code gizmo in meshless finite mass mode. In order to model the interaction between equal mass circular binaries and their locally isothermal circumbinary discs, we enforce hyper-Lagrangian resolution inside the cavity. We find that fixing the binary orbit ultimately leads to an overestimate of the gravitational torque that the gas exerts on the binary and an underestimate of the torque due to the accretion of material on to the binary components. Furthermore, we find that the modulation of the accretion rate on the binary orbital period is strongly suppressed in the fixed orbit simulation, while it is clearly present in the live binary simulations. This has potential implications for the prediction of the observable periodicities in massive black hole binary candidates.","lang":"eng"}]},{"quality_controlled":"1","volume":951,"publication_identifier":{"issn":["2041-8205","2041-8213"]},"article_number":"L5","publication":"The Astrophysical Journal Letters","scopus_import":"1","date_created":"2024-09-05T10:11:02Z","extern":"1","citation":{"ista":"Yang J, Wang F, Fan X, Hennawi JF, Barth AJ, Bañados E, Sun F, Liu W, Cai Z, Jiang L, Li Z, Onoue M, Schindler J-T, Shen Y, Wu Y, Bhowmick AK, Bieri R, Blecha L, Bosman S, Champagne JB, Colina L, Connor T, Costa T, Davies FB, Decarli R, De Rosa G, Drake AB, Egami E, Eilers A-C, Evans AE, Farina EP, Habouzit M, Haiman Z, Jin X, Jun HD, Kakiichi K, Khusanova Y, Kulkarni G, Loiacono F, Lupi A, Mazzucchelli C, Pan Z, Rojas-Ruiz S, Strauss MA, Tee WL, Trakhtenbrot B, Trebitsch M, Venemans B, Vestergaard M, Volonteri M, Walter F, Xie Z-L, Yue M, Zhang H, Zhang H, Zou S. 2023. A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of &#62; 6.5 quasars using JWST. The Astrophysical Journal Letters. 951(1), L5.","mla":"Yang, Jinyi, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-Frame Optical Spectra of &#62; 6.5 Quasars Using JWST.” <i>The Astrophysical Journal Letters</i>, vol. 951, no. 1, L5, American Astronomical Society, 2023, doi:<a href=\"https://doi.org/10.3847/2041-8213/acc9c8\">10.3847/2041-8213/acc9c8</a>.","ama":"Yang J, Wang F, Fan X, et al. A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of &#62; 6.5 quasars using JWST. <i>The Astrophysical Journal Letters</i>. 2023;951(1). doi:<a href=\"https://doi.org/10.3847/2041-8213/acc9c8\">10.3847/2041-8213/acc9c8</a>","short":"J. Yang, F. Wang, X. Fan, J.F. Hennawi, A.J. Barth, E. Bañados, F. Sun, W. Liu, Z. Cai, L. Jiang, Z. Li, M. Onoue, J.-T. Schindler, Y. Shen, Y. Wu, A.K. Bhowmick, R. Bieri, L. Blecha, S. Bosman, J.B. Champagne, L. Colina, T. Connor, T. Costa, F.B. Davies, R. Decarli, G. De Rosa, A.B. Drake, E. Egami, A.-C. Eilers, A.E. Evans, E.P. Farina, M. Habouzit, Z. Haiman, X. Jin, H.D. Jun, K. Kakiichi, Y. Khusanova, G. Kulkarni, F. Loiacono, A. Lupi, C. Mazzucchelli, Z. Pan, S. Rojas-Ruiz, M.A. Strauss, W.L. Tee, B. Trakhtenbrot, M. Trebitsch, B. Venemans, M. Vestergaard, M. Volonteri, F. Walter, Z.-L. Xie, M. Yue, H. Zhang, H. Zhang, S. Zou, The Astrophysical Journal Letters 951 (2023).","ieee":"J. Yang <i>et al.</i>, “A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of &#62; 6.5 quasars using JWST,” <i>The Astrophysical Journal Letters</i>, vol. 951, no. 1. American Astronomical Society, 2023.","apa":"Yang, J., Wang, F., Fan, X., Hennawi, J. F., Barth, A. J., Bañados, E., … Zou, S. (2023). A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of &#62; 6.5 quasars using JWST. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/acc9c8\">https://doi.org/10.3847/2041-8213/acc9c8</a>","chicago":"Yang, Jinyi, Feige Wang, Xiaohui Fan, Joseph F. Hennawi, Aaron J. Barth, Eduardo Bañados, Fengwu Sun, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-Frame Optical Spectra of &#62; 6.5 Quasars Using JWST.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2023. <a href=\"https://doi.org/10.3847/2041-8213/acc9c8\">https://doi.org/10.3847/2041-8213/acc9c8</a>."},"main_file_link":[{"url":"https://doi.org/10.3847/2041-8213/acc9c8","open_access":"1"}],"oa_version":"Published Version","intvolume":"       951","issue":"1","month":"06","article_processing_charge":"No","oa":1,"year":"2023","publication_status":"published","article_type":"original","author":[{"full_name":"Yang, Jinyi","first_name":"Jinyi","last_name":"Yang"},{"full_name":"Wang, Feige","first_name":"Feige","last_name":"Wang"},{"last_name":"Fan","first_name":"Xiaohui","full_name":"Fan, Xiaohui"},{"full_name":"Hennawi, Joseph F.","first_name":"Joseph F.","last_name":"Hennawi"},{"first_name":"Aaron J.","full_name":"Barth, Aaron J.","last_name":"Barth"},{"last_name":"Bañados","full_name":"Bañados, Eduardo","first_name":"Eduardo"},{"last_name":"Sun","full_name":"Sun, Fengwu","first_name":"Fengwu"},{"last_name":"Liu","first_name":"Weizhe","full_name":"Liu, Weizhe"},{"last_name":"Cai","first_name":"Zheng","full_name":"Cai, Zheng"},{"last_name":"Jiang","full_name":"Jiang, Linhua","first_name":"Linhua"},{"last_name":"Li","full_name":"Li, Zihao","first_name":"Zihao"},{"last_name":"Onoue","full_name":"Onoue, Masafusa","first_name":"Masafusa"},{"last_name":"Schindler","first_name":"Jan-Torge","full_name":"Schindler, Jan-Torge"},{"last_name":"Shen","full_name":"Shen, Yue","first_name":"Yue"},{"first_name":"Yunjing","full_name":"Wu, Yunjing","last_name":"Wu"},{"last_name":"Bhowmick","first_name":"Aklant K.","full_name":"Bhowmick, Aklant K."},{"full_name":"Bieri, Rebekka","first_name":"Rebekka","last_name":"Bieri"},{"last_name":"Blecha","full_name":"Blecha, Laura","first_name":"Laura"},{"last_name":"Bosman","full_name":"Bosman, Sarah","first_name":"Sarah"},{"full_name":"Champagne, Jaclyn B.","first_name":"Jaclyn B.","last_name":"Champagne"},{"last_name":"Colina","first_name":"Luis","full_name":"Colina, Luis"},{"last_name":"Connor","first_name":"Thomas","full_name":"Connor, Thomas"},{"last_name":"Costa","full_name":"Costa, Tiago","first_name":"Tiago"},{"last_name":"Davies","first_name":"Frederick B.","full_name":"Davies, Frederick B."},{"first_name":"Roberto","full_name":"Decarli, Roberto","last_name":"Decarli"},{"last_name":"De Rosa","full_name":"De Rosa, Gisella","first_name":"Gisella"},{"first_name":"Alyssa B.","full_name":"Drake, Alyssa B.","last_name":"Drake"},{"first_name":"Eiichi","full_name":"Egami, Eiichi","last_name":"Egami"},{"first_name":"Anna-Christina","full_name":"Eilers, Anna-Christina","last_name":"Eilers"},{"first_name":"Analis E.","full_name":"Evans, Analis E.","last_name":"Evans"},{"full_name":"Farina, Emanuele Paolo","first_name":"Emanuele Paolo","last_name":"Farina"},{"last_name":"Habouzit","full_name":"Habouzit, Melanie","first_name":"Melanie"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"last_name":"Jin","first_name":"Xiangyu","full_name":"Jin, Xiangyu"},{"last_name":"Jun","full_name":"Jun, Hyunsung D.","first_name":"Hyunsung D."},{"full_name":"Kakiichi, Koki","first_name":"Koki","last_name":"Kakiichi"},{"last_name":"Khusanova","full_name":"Khusanova, Yana","first_name":"Yana"},{"full_name":"Kulkarni, Girish","first_name":"Girish","last_name":"Kulkarni"},{"full_name":"Loiacono, Federica","first_name":"Federica","last_name":"Loiacono"},{"last_name":"Lupi","full_name":"Lupi, Alessandro","first_name":"Alessandro"},{"last_name":"Mazzucchelli","first_name":"Chiara","full_name":"Mazzucchelli, Chiara"},{"first_name":"Zhiwei","full_name":"Pan, Zhiwei","last_name":"Pan"},{"last_name":"Rojas-Ruiz","full_name":"Rojas-Ruiz, Sofía","first_name":"Sofía"},{"first_name":"Michael A.","full_name":"Strauss, Michael A.","last_name":"Strauss"},{"last_name":"Tee","full_name":"Tee, Wei Leong","first_name":"Wei Leong"},{"last_name":"Trakhtenbrot","full_name":"Trakhtenbrot, Benny","first_name":"Benny"},{"first_name":"Maxime","full_name":"Trebitsch, Maxime","last_name":"Trebitsch"},{"first_name":"Bram","full_name":"Venemans, Bram","last_name":"Venemans"},{"last_name":"Vestergaard","full_name":"Vestergaard, Marianne","first_name":"Marianne"},{"last_name":"Volonteri","first_name":"Marta","full_name":"Volonteri, Marta"},{"full_name":"Walter, Fabian","first_name":"Fabian","last_name":"Walter"},{"full_name":"Xie, Zhang-Liang","first_name":"Zhang-Liang","last_name":"Xie"},{"full_name":"Yue, Minghao","first_name":"Minghao","last_name":"Yue"},{"first_name":"Haowen","full_name":"Zhang, Haowen","last_name":"Zhang"},{"last_name":"Zhang","full_name":"Zhang, Huanian","first_name":"Huanian"},{"full_name":"Zou, Siwei","first_name":"Siwei","last_name":"Zou"}],"type":"journal_article","_id":"17549","status":"public","doi":"10.3847/2041-8213/acc9c8","publisher":"American Astronomical Society","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"lang":"eng","text":"Studies of rest-frame optical emission in quasars at z>6 have historically been limited by the wavelengths accessible by ground-based telescopes. The James Webb Space Telescope (JWST) now offers the opportunity to probe this emission deep into the reionization epoch. We report the observations of eight quasars at z>6.5 using the JWST/NIRCam Wide Field Slitless Spectroscopy, as a part of the ''A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE)\" program. Our JWST spectra cover the quasars' emission between rest frame ∼ 4100 and 5100 Å. The profiles of these quasars' broad Hβ emission lines span a FWHM from 3000 to 6000 km s−1. The Hβ-based virial black hole (BH) masses, ranging from 0.6 to 2.1 billion solar masses, are generally consistent with their MgII-based BH masses. The new measurements based on the more reliable Hβ tracer thus confirm the existence of billion solar-mass BHs in the reionization epoch. In the observed [OIII] λλ4960,5008 doublets of these luminous quasars, broad components are more common than narrow core components (≤ 1200 km s−1), and only one quasar shows stronger narrow components than broad. Two quasars exhibit significantly broad and blueshifted [OIII] emission, thought to trace galactic-scale outflows, with median velocities of −610 km s−1 and −1430 km s−1 relative to the [CII] 158μm line. All eight quasars show strong optical FeII emission, and follow the Eigenvector 1 relations defined by low-redshift quasars. The entire ASPIRE program will eventually cover 25 quasars and provide a statistical sample for the studies of the BHs and quasar spectral properties."}],"title":"A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of > 6.5 quasars using JWST","date_updated":"2024-09-18T09:53:12Z","date_published":"2023-06-29T00:00:00Z","day":"29","fulldoi":"https://doi.org/10.3847/2041-8213/acc9c8","language":[{"iso":"eng"}]},{"author":[{"first_name":"Tianhuan","full_name":"Lu, Tianhuan","last_name":"Lu"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"last_name":"Li","first_name":"Xiangchong","full_name":"Li, Xiangchong"}],"article_type":"original","publication_status":"published","month":"03","issue":"2","intvolume":"       521","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad686"}],"oa_version":"Published Version","year":"2023","oa":1,"article_processing_charge":"No","date_created":"2024-09-05T10:14:34Z","scopus_import":"1","publication":"Monthly Notices of the Royal Astronomical Society","citation":{"mla":"Lu, Tianhuan, et al. “Cosmological Constraints from HSC Survey First-Year Data Using Deep Learning.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 521, no. 2, Oxford University Press, 2023, pp. 2050–66, doi:<a href=\"https://doi.org/10.1093/mnras/stad686\">10.1093/mnras/stad686</a>.","ama":"Lu T, Haiman Z, Li X. Cosmological constraints from HSC survey first-year data using deep learning. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;521(2):2050-2066. doi:<a href=\"https://doi.org/10.1093/mnras/stad686\">10.1093/mnras/stad686</a>","ista":"Lu T, Haiman Z, Li X. 2023. Cosmological constraints from HSC survey first-year data using deep learning. Monthly Notices of the Royal Astronomical Society. 521(2), 2050–2066.","chicago":"Lu, Tianhuan, Zoltán Haiman, and Xiangchong Li. “Cosmological Constraints from HSC Survey First-Year Data Using Deep Learning.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnras/stad686\">https://doi.org/10.1093/mnras/stad686</a>.","short":"T. Lu, Z. Haiman, X. Li, Monthly Notices of the Royal Astronomical Society 521 (2023) 2050–2066.","ieee":"T. Lu, Z. Haiman, and X. Li, “Cosmological constraints from HSC survey first-year data using deep learning,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 521, no. 2. Oxford University Press, pp. 2050–2066, 2023.","apa":"Lu, T., Haiman, Z., &#38; Li, X. (2023). Cosmological constraints from HSC survey first-year data using deep learning. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stad686\">https://doi.org/10.1093/mnras/stad686</a>"},"extern":"1","volume":521,"publication_identifier":{"issn":["0035-8711","1365-2966"]},"quality_controlled":"1","date_published":"2023-03-06T00:00:00Z","day":"06","language":[{"iso":"eng"}],"fulldoi":"https://doi.org/10.1093/mnras/stad686","title":"Cosmological constraints from HSC survey first-year data using deep learning","abstract":[{"text":"We present cosmological constraints from the Subaru Hyper Suprime-Cam (HSC) first-year weak lensing shear catalogue using convolutional neural networks (CNNs) and conventional summary statistics. We crop 19 3×3deg2 sub-fields from the first-year area, divide the galaxies with redshift 0.3≤z≤1.5 into four equally-spaced redshift bins, and perform tomographic analyses. We develop a pipeline to generate simulated convergence maps from cosmological N-body simulations, where we account for effects such as intrinsic alignments (IAs), baryons, photometric redshift errors, and point spread function errors, to match characteristics of the real catalogue. We train CNNs that can predict the underlying parameters from the simulated maps, and we use them to construct likelihood functions for Bayesian analyses. In the Λ cold dark matter model with two free cosmological parameters Ωm and σ8, we find Ωm=0.278+0.037−0.035, S8≡(Ωm/0.3)0.5σ8=0.793+0.017−0.018, and the IA amplitude AIA=0.20+0.55−0.58. In a model with four additional free baryonic parameters, we find Ωm=0.268+0.040−0.036, S8=0.819+0.034−0.024, and AIA=−0.16+0.59−0.58, with the baryonic parameters not being well-constrained. We also find that statistical uncertainties of the parameters by the CNNs are smaller than those from the power spectrum (5--24 percent smaller for S8 and a factor of 2.5--3.0 smaller for Ωm), showing the effectiveness of CNNs for uncovering additional cosmological information from the HSC data. With baryons, the S8 discrepancy between HSC first-year data and Planck 2018 is reduced from ∼2.2σ to 0.3--0.5σ.","lang":"eng"}],"page":"2050-2066","date_updated":"2024-09-18T10:09:01Z","status":"public","_id":"17551","type":"journal_article","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publisher":"Oxford University Press","doi":"10.1093/mnras/stad686"},{"doi":"10.1093/mnras/stad3641","publisher":"Oxford University Press (OUP)","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","type":"journal_article","status":"public","_id":"17557","date_updated":"2024-09-18T12:11:28Z","page":"10448-10468","abstract":[{"text":"The black hole (BH) binaries in active galactic nuclei (AGN) are expected to form mainly through scattering encounters in the ambient gaseous medium. Recent simulations, including our own, have confirmed this formation pathway is highly efficient. We perform 3D smoothed particle hydrodynamics (SPH) simulations of BH scattering encounters in AGN discs. Using a range of impact parameters, we probe the necessary conditions for binary capture and how different orbital trajectories affect the dissipative effects from the gas. We identify a single range of impact parameters, typically of width ∼0.86−1.59 binary Hill radii depending on AGN disc density, that reliably leads to binary formation. The periapsis of the first encounter is the primary variable that determines the outcome of the initial scattering. We find an associated power law between the energy dissipated and the periapsis depth to be ΔE ∝ r−b with b = 0.42 ± 0.16, where deeper encounters dissipate more energy. Excluding accretion physics does not significantly alter these results. We identify the region of parameter space in initial energy versus impact parameter where a scattering leads to binary formation. Based on our findings, we provide a ready-to-use analytic criterion that utilizes these two pre-encounter parameters to determine the outcome of an encounter, with a reliability rate of &amp;gt;90 per cent. As the criterion is based directly on our simulations, it provides a reliable and highly physically motivated criterion for predicting binary scattering outcomes which can be used in population studies of BH binaries and mergers around AGN.","lang":"eng"}],"title":"Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings","fulldoi":"https://doi.org/10.1093/mnras/stad3641","language":[{"iso":"eng"}],"date_published":"2023-01-01T00:00:00Z","quality_controlled":"1","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":527,"extern":"1","citation":{"chicago":"Rowan, Connar, Henry Whitehead, Tjarda Boekholt, Bence Kocsis, and Zoltán Haiman. “Black Hole Binaries in AGN Accretion Discs – II. Gas Effects on Black Hole Satellite Scatterings.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press (OUP), 2023. <a href=\"https://doi.org/10.1093/mnras/stad3641\">https://doi.org/10.1093/mnras/stad3641</a>.","apa":"Rowan, C., Whitehead, H., Boekholt, T., Kocsis, B., &#38; Haiman, Z. (2023). Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press (OUP). <a href=\"https://doi.org/10.1093/mnras/stad3641\">https://doi.org/10.1093/mnras/stad3641</a>","ieee":"C. Rowan, H. Whitehead, T. Boekholt, B. Kocsis, and Z. Haiman, “Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 527, no. 4. Oxford University Press (OUP), pp. 10448–10468, 2023.","short":"C. Rowan, H. Whitehead, T. Boekholt, B. Kocsis, Z. Haiman, Monthly Notices of the Royal Astronomical Society 527 (2023) 10448–10468.","ama":"Rowan C, Whitehead H, Boekholt T, Kocsis B, Haiman Z. Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;527(4):10448-10468. doi:<a href=\"https://doi.org/10.1093/mnras/stad3641\">10.1093/mnras/stad3641</a>","mla":"Rowan, Connar, et al. “Black Hole Binaries in AGN Accretion Discs – II. Gas Effects on Black Hole Satellite Scatterings.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 527, no. 4, Oxford University Press (OUP), 2023, pp. 10448–68, doi:<a href=\"https://doi.org/10.1093/mnras/stad3641\">10.1093/mnras/stad3641</a>.","ista":"Rowan C, Whitehead H, Boekholt T, Kocsis B, Haiman Z. 2023. Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings. Monthly Notices of the Royal Astronomical Society. 527(4), 10448–10468."},"publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","date_created":"2024-09-05T10:32:08Z","article_processing_charge":"No","oa":1,"year":"2023","oa_version":"Published Version","issue":"4","intvolume":"       527","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad3641"}],"month":"01","publication_status":"published","article_type":"original","author":[{"full_name":"Rowan, Connar","first_name":"Connar","last_name":"Rowan"},{"full_name":"Whitehead, Henry","first_name":"Henry","last_name":"Whitehead"},{"first_name":"Tjarda","full_name":"Boekholt, Tjarda","last_name":"Boekholt"},{"first_name":"Bence","full_name":"Kocsis, Bence","last_name":"Kocsis"},{"last_name":"Haiman","first_name":"Zoltán","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}]},{"arxiv":1,"quality_controlled":"1","publication_identifier":{"issn":["0028-0836","1476-4687"]},"volume":621,"extern":"1","citation":{"ista":"Ding X, Onoue M, Silverman JD, Matsuoka Y, Izumi T, Strauss MA, Jahnke K, Phillips CL, Li J, Volonteri M, Haiman Z, Andika IT, Aoki K, Baba S, Bieri R, Bosman SEI, Bottrell C, Eilers A-C, Fujimoto S, Habouzit M, Imanishi M, Inayoshi K, Iwasawa K, Kashikawa N, Kawaguchi T, Kohno K, Lee C-H, Lupi A, Lyu J, Nagao T, Overzier R, Schindler J-T, Schramm M, Shimasaku K, Toba Y, Trakhtenbrot B, Trebitsch M, Treu T, Umehata H, Venemans BP, Vestergaard M, Walter F, Wang F, Yang J. 2023. Detection of stellar light from quasar host galaxies at redshifts above 6. Nature. 621(7977), 51–55.","mla":"Ding, Xuheng, et al. “Detection of Stellar Light from Quasar Host Galaxies at Redshifts above 6.” <i>Nature</i>, vol. 621, no. 7977, Springer Science and Business Media LLC, 2023, pp. 51–55, doi:<a href=\"https://doi.org/10.1038/s41586-023-06345-5\">10.1038/s41586-023-06345-5</a>.","ama":"Ding X, Onoue M, Silverman JD, et al. Detection of stellar light from quasar host galaxies at redshifts above 6. <i>Nature</i>. 2023;621(7977):51-55. doi:<a href=\"https://doi.org/10.1038/s41586-023-06345-5\">10.1038/s41586-023-06345-5</a>","apa":"Ding, X., Onoue, M., Silverman, J. D., Matsuoka, Y., Izumi, T., Strauss, M. A., … Yang, J. (2023). Detection of stellar light from quasar host galaxies at redshifts above 6. <i>Nature</i>. Springer Science and Business Media LLC. <a href=\"https://doi.org/10.1038/s41586-023-06345-5\">https://doi.org/10.1038/s41586-023-06345-5</a>","ieee":"X. Ding <i>et al.</i>, “Detection of stellar light from quasar host galaxies at redshifts above 6,” <i>Nature</i>, vol. 621, no. 7977. Springer Science and Business Media LLC, pp. 51–55, 2023.","short":"X. Ding, M. Onoue, J.D. Silverman, Y. Matsuoka, T. Izumi, M.A. Strauss, K. Jahnke, C.L. Phillips, J. Li, M. Volonteri, Z. Haiman, I.T. Andika, K. Aoki, S. Baba, R. Bieri, S.E.I. Bosman, C. Bottrell, A.-C. Eilers, S. Fujimoto, M. Habouzit, M. Imanishi, K. Inayoshi, K. Iwasawa, N. Kashikawa, T. Kawaguchi, K. Kohno, C.-H. Lee, A. Lupi, J. Lyu, T. Nagao, R. Overzier, J.-T. Schindler, M. Schramm, K. Shimasaku, Y. Toba, B. Trakhtenbrot, M. Trebitsch, T. Treu, H. Umehata, B.P. Venemans, M. Vestergaard, F. Walter, F. Wang, J. Yang, Nature 621 (2023) 51–55.","chicago":"Ding, Xuheng, Masafusa Onoue, John D. Silverman, Yoshiki Matsuoka, Takuma Izumi, Michael A. Strauss, Knud Jahnke, et al. “Detection of Stellar Light from Quasar Host Galaxies at Redshifts above 6.” <i>Nature</i>. Springer Science and Business Media LLC, 2023. <a href=\"https://doi.org/10.1038/s41586-023-06345-5\">https://doi.org/10.1038/s41586-023-06345-5</a>."},"publication":"Nature","date_created":"2024-09-05T11:28:21Z","scopus_import":"1","oa":1,"year":"2023","article_processing_charge":"No","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.2211.14329","open_access":"1"}],"issue":"7977","intvolume":"       621","oa_version":"Preprint","month":"06","author":[{"last_name":"Ding","first_name":"Xuheng","full_name":"Ding, Xuheng"},{"first_name":"Masafusa","full_name":"Onoue, Masafusa","last_name":"Onoue"},{"first_name":"John D.","full_name":"Silverman, John D.","last_name":"Silverman"},{"full_name":"Matsuoka, Yoshiki","first_name":"Yoshiki","last_name":"Matsuoka"},{"first_name":"Takuma","full_name":"Izumi, Takuma","last_name":"Izumi"},{"last_name":"Strauss","full_name":"Strauss, Michael A.","first_name":"Michael A."},{"full_name":"Jahnke, Knud","first_name":"Knud","last_name":"Jahnke"},{"last_name":"Phillips","full_name":"Phillips, Camryn L.","first_name":"Camryn L."},{"last_name":"Li","full_name":"Li, Junyao","first_name":"Junyao"},{"first_name":"Marta","full_name":"Volonteri, Marta","last_name":"Volonteri"},{"last_name":"Haiman","first_name":"Zoltán","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"full_name":"Andika, Irham Taufik","first_name":"Irham Taufik","last_name":"Andika"},{"last_name":"Aoki","full_name":"Aoki, Kentaro","first_name":"Kentaro"},{"last_name":"Baba","full_name":"Baba, Shunsuke","first_name":"Shunsuke"},{"last_name":"Bieri","first_name":"Rebekka","full_name":"Bieri, Rebekka"},{"last_name":"Bosman","full_name":"Bosman, Sarah E. I.","first_name":"Sarah E. I."},{"last_name":"Bottrell","first_name":"Connor","full_name":"Bottrell, Connor"},{"first_name":"Anna-Christina","full_name":"Eilers, Anna-Christina","last_name":"Eilers"},{"first_name":"Seiji","full_name":"Fujimoto, Seiji","last_name":"Fujimoto"},{"last_name":"Habouzit","full_name":"Habouzit, Melanie","first_name":"Melanie"},{"full_name":"Imanishi, Masatoshi","first_name":"Masatoshi","last_name":"Imanishi"},{"full_name":"Inayoshi, Kohei","first_name":"Kohei","last_name":"Inayoshi"},{"full_name":"Iwasawa, Kazushi","first_name":"Kazushi","last_name":"Iwasawa"},{"last_name":"Kashikawa","first_name":"Nobunari","full_name":"Kashikawa, Nobunari"},{"last_name":"Kawaguchi","full_name":"Kawaguchi, Toshihiro","first_name":"Toshihiro"},{"last_name":"Kohno","first_name":"Kotaro","full_name":"Kohno, Kotaro"},{"first_name":"Chien-Hsiu","full_name":"Lee, Chien-Hsiu","last_name":"Lee"},{"first_name":"Alessandro","full_name":"Lupi, Alessandro","last_name":"Lupi"},{"full_name":"Lyu, Jianwei","first_name":"Jianwei","last_name":"Lyu"},{"full_name":"Nagao, Tohru","first_name":"Tohru","last_name":"Nagao"},{"first_name":"Roderik","full_name":"Overzier, Roderik","last_name":"Overzier"},{"first_name":"Jan-Torge","full_name":"Schindler, Jan-Torge","last_name":"Schindler"},{"full_name":"Schramm, Malte","first_name":"Malte","last_name":"Schramm"},{"full_name":"Shimasaku, Kazuhiro","first_name":"Kazuhiro","last_name":"Shimasaku"},{"full_name":"Toba, Yoshiki","first_name":"Yoshiki","last_name":"Toba"},{"full_name":"Trakhtenbrot, Benny","first_name":"Benny","last_name":"Trakhtenbrot"},{"last_name":"Trebitsch","first_name":"Maxime","full_name":"Trebitsch, Maxime"},{"first_name":"Tommaso","full_name":"Treu, Tommaso","last_name":"Treu"},{"last_name":"Umehata","full_name":"Umehata, Hideki","first_name":"Hideki"},{"last_name":"Venemans","full_name":"Venemans, Bram P.","first_name":"Bram P."},{"last_name":"Vestergaard","first_name":"Marianne","full_name":"Vestergaard, Marianne"},{"first_name":"Fabian","full_name":"Walter, Fabian","last_name":"Walter"},{"first_name":"Feige","full_name":"Wang, Feige","last_name":"Wang"},{"full_name":"Yang, Jinyi","first_name":"Jinyi","last_name":"Yang"}],"article_type":"original","publication_status":"published","doi":"10.1038/s41586-023-06345-5","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publisher":"Springer Science and Business Media LLC","_id":"17558","status":"public","type":"journal_article","date_updated":"2024-09-18T12:19:50Z","page":"51-55","abstract":[{"lang":"eng","text":"The detection of starlight from the host galaxies of quasars during the reionization epoch (z > 6) has been elusive, even with deep Hubble Space Telescope observations1,2. The current highest redshift quasar host detected3, at z = 4.5, required the magnifying effect of a foreground lensing galaxy. Low-luminosity quasars4,5,6 from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP)7 mitigate the challenge of detecting their underlying, previously undetected host galaxies. Here we report rest-frame optical images and spectroscopy of two HSC-SSP quasars at z > 6 with the JWST. Using near-infrared camera imaging at 3.6 and 1.5 μm and subtracting the light from the unresolved quasars, we find that the host galaxies are massive (stellar masses of 13 × and 3.4 × 1010 M☉, respectively), compact and disc-like. Near-infrared spectroscopy at medium resolution shows stellar absorption lines in the more massive quasar, confirming the detection of the host. Velocity-broadened gas in the vicinity of these quasars enables measurements of their black hole masses (1.4 × 109 and 2.0 × 108 M☉, respectively). Their location in the black hole mass–stellar mass plane is consistent with the distribution at low redshift, suggesting that the relation between black holes and their host galaxies was already in place less than a billion years after the Big Bang."}],"title":"Detection of stellar light from quasar host galaxies at redshifts above 6","language":[{"iso":"eng"}],"fulldoi":"https://doi.org/10.1038/s41586-023-06345-5","external_id":{"arxiv":["2211.14329"]},"date_published":"2023-06-28T00:00:00Z","day":"28"},{"extern":"1","citation":{"ista":"Amaro-Seoane P et al. 2023. Astrophysics with the laser interferometer space antenna. Living Reviews in Relativity. 26(1), 2.","ama":"Amaro-Seoane P, Andrews J, Arca Sedda M, et al. Astrophysics with the laser interferometer space antenna. <i>Living Reviews in Relativity</i>. 2023;26(1). doi:<a href=\"https://doi.org/10.1007/s41114-022-00041-y\">10.1007/s41114-022-00041-y</a>","mla":"Amaro-Seoane, Pau, et al. “Astrophysics with the Laser Interferometer Space Antenna.” <i>Living Reviews in Relativity</i>, vol. 26, no. 1, 2, Springer Science and Business Media LLC, 2023, doi:<a href=\"https://doi.org/10.1007/s41114-022-00041-y\">10.1007/s41114-022-00041-y</a>.","ieee":"P. Amaro-Seoane <i>et al.</i>, “Astrophysics with the laser interferometer space antenna,” <i>Living Reviews in Relativity</i>, vol. 26, no. 1. Springer Science and Business Media LLC, 2023.","apa":"Amaro-Seoane, P., Andrews, J., Arca Sedda, M., Askar, A., Baghi, Q., Balasov, R., … Vigna-Gómez, A. (2023). Astrophysics with the laser interferometer space antenna. <i>Living Reviews in Relativity</i>. Springer Science and Business Media LLC. <a href=\"https://doi.org/10.1007/s41114-022-00041-y\">https://doi.org/10.1007/s41114-022-00041-y</a>","short":"P. Amaro-Seoane, J. Andrews, M. Arca Sedda, A. Askar, Q. Baghi, R. Balasov, I. Bartos, S.S. Bavera, J. Bellovary, C.P.L. Berry, E. Berti, S. Bianchi, L. Blecha, S. Blondin, T. Bogdanović, S. Boissier, M. Bonetti, S. Bonoli, E. Bortolas, K. Breivik, P.R. Capelo, L. Caramete, F. Cattorini, M. Charisi, S. Chaty, X. Chen, M. Chruślińska, A.J.K. Chua, R. Church, M. Colpi, D. D’Orazio, C. Danielski, M.B. Davies, P. Dayal, A. De Rosa, A. Derdzinski, K. Destounis, M. Dotti, I. Duţan, I. Dvorkin, G. Fabj, T. Foglizzo, S. Ford, J.-B. Fouvry, A. Franchini, T. Fragos, C. Fryer, M. Gaspari, D. Gerosa, L. Graziani, P. Groot, M. Habouzit, D. Haggard, Z. Haiman, W.-B. Han, A. Istrate, P.H. Johansson, F.M. Khan, T. Kimpson, K. Kokkotas, A. Kong, V. Korol, K. Kremer, T. Kupfer, A. Lamberts, S. Larson, M. Lau, D. Liu, N. Lloyd-Ronning, G. Lodato, A. Lupi, C.-P. Ma, T. Maccarone, I. Mandel, A. Mangiagli, M. Mapelli, S. Mathis, L. Mayer, S. McGee, B. McKernan, M.C. Miller, D.F. Mota, M. Mumpower, S.S. Nasim, G. Nelemans, S. Noble, F. Pacucci, F. Panessa, V. Paschalidis, H. Pfister, D. Porquet, J. Quenby, A. Ricarte, F.K. Röpke, J. Regan, S. Rosswog, A. Ruiter, M. Ruiz, J. Runnoe, R. Schneider, J. Schnittman, A. Secunda, A. Sesana, N. Seto, L. Shao, S. Shapiro, C. Sopuerta, N.C. Stone, A. Suvorov, N. Tamanini, T. Tamfal, T. Tauris, K. Temmink, J. Tomsick, S. Toonen, A. Torres-Orjuela, M. Toscani, A. Tsokaros, C. Unal, V. Vázquez-Aceves, R. Valiante, M. van Putten, J. van Roestel, C. Vignali, M. Volonteri, K. Wu, Z. Younsi, S. Yu, S. Zane, L. Zwick, F. Antonini, V. Baibhav, E. Barausse, A. Bonilla Rivera, M. Branchesi, G. Branduardi-Raymont, K. Burdge, S. Chakraborty, J. Cuadra, K. Dage, B. Davis, S.E. de Mink, R. Decarli, D. Doneva, S. Escoffier, P. Gandhi, F. Haardt, C.O. Lousto, S. Nissanke, J. Nordhaus, R. O’Shaughnessy, S. Portegies Zwart, A. Pound, F. Schussler, O. Sergijenko, A. Spallicci, D. Vernieri, A. Vigna-Gómez, Living Reviews in Relativity 26 (2023).","chicago":"Amaro-Seoane, Pau, Jeff Andrews, Manuel Arca Sedda, Abbas Askar, Quentin Baghi, Razvan Balasov, Imre Bartos, et al. “Astrophysics with the Laser Interferometer Space Antenna.” <i>Living Reviews in Relativity</i>. Springer Science and Business Media LLC, 2023. <a href=\"https://doi.org/10.1007/s41114-022-00041-y\">https://doi.org/10.1007/s41114-022-00041-y</a>."},"publication":"Living Reviews in Relativity","scopus_import":"1","date_created":"2024-09-05T12:16:33Z","article_number":"2","quality_controlled":"1","publication_identifier":{"issn":["1433-8351"]},"volume":26,"article_type":"original","publication_status":"published","author":[{"first_name":"Pau","full_name":"Amaro-Seoane, Pau","last_name":"Amaro-Seoane"},{"first_name":"Jeff","full_name":"Andrews, Jeff","last_name":"Andrews"},{"full_name":"Arca Sedda, Manuel","first_name":"Manuel","last_name":"Arca Sedda"},{"last_name":"Askar","full_name":"Askar, Abbas","first_name":"Abbas"},{"last_name":"Baghi","full_name":"Baghi, Quentin","first_name":"Quentin"},{"full_name":"Balasov, Razvan","first_name":"Razvan","last_name":"Balasov"},{"last_name":"Bartos","full_name":"Bartos, Imre","first_name":"Imre"},{"full_name":"Bavera, Simone S.","first_name":"Simone S.","last_name":"Bavera"},{"last_name":"Bellovary","full_name":"Bellovary, Jillian","first_name":"Jillian"},{"full_name":"Berry, Christopher P. L.","first_name":"Christopher P. L.","last_name":"Berry"},{"full_name":"Berti, Emanuele","first_name":"Emanuele","last_name":"Berti"},{"first_name":"Stefano","full_name":"Bianchi, Stefano","last_name":"Bianchi"},{"last_name":"Blecha","full_name":"Blecha, Laura","first_name":"Laura"},{"first_name":"Stéphane","full_name":"Blondin, Stéphane","last_name":"Blondin"},{"first_name":"Tamara","full_name":"Bogdanović, Tamara","last_name":"Bogdanović"},{"first_name":"Samuel","full_name":"Boissier, Samuel","last_name":"Boissier"},{"last_name":"Bonetti","first_name":"Matteo","full_name":"Bonetti, Matteo"},{"last_name":"Bonoli","first_name":"Silvia","full_name":"Bonoli, Silvia"},{"first_name":"Elisa","full_name":"Bortolas, Elisa","last_name":"Bortolas"},{"last_name":"Breivik","first_name":"Katelyn","full_name":"Breivik, Katelyn"},{"first_name":"Pedro R.","full_name":"Capelo, Pedro R.","last_name":"Capelo"},{"full_name":"Caramete, Laurentiu","first_name":"Laurentiu","last_name":"Caramete"},{"full_name":"Cattorini, Federico","first_name":"Federico","last_name":"Cattorini"},{"last_name":"Charisi","first_name":"Maria","full_name":"Charisi, Maria"},{"first_name":"Sylvain","full_name":"Chaty, Sylvain","last_name":"Chaty"},{"last_name":"Chen","full_name":"Chen, Xian","first_name":"Xian"},{"first_name":"Martyna","full_name":"Chruślińska, Martyna","last_name":"Chruślińska"},{"first_name":"Alvin J. K.","full_name":"Chua, Alvin J. K.","last_name":"Chua"},{"full_name":"Church, Ross","first_name":"Ross","last_name":"Church"},{"last_name":"Colpi","full_name":"Colpi, Monica","first_name":"Monica"},{"full_name":"D’Orazio, Daniel","first_name":"Daniel","last_name":"D’Orazio"},{"last_name":"Danielski","first_name":"Camilla","full_name":"Danielski, Camilla"},{"last_name":"Davies","full_name":"Davies, Melvyn B.","first_name":"Melvyn B."},{"full_name":"Dayal, Pratika","first_name":"Pratika","last_name":"Dayal"},{"last_name":"De Rosa","first_name":"Alessandra","full_name":"De Rosa, Alessandra"},{"last_name":"Derdzinski","full_name":"Derdzinski, Andrea","first_name":"Andrea"},{"full_name":"Destounis, Kyriakos","first_name":"Kyriakos","last_name":"Destounis"},{"full_name":"Dotti, Massimo","first_name":"Massimo","last_name":"Dotti"},{"last_name":"Duţan","first_name":"Ioana","full_name":"Duţan, Ioana"},{"last_name":"Dvorkin","full_name":"Dvorkin, Irina","first_name":"Irina"},{"first_name":"Gaia","full_name":"Fabj, Gaia","last_name":"Fabj"},{"full_name":"Foglizzo, Thierry","first_name":"Thierry","last_name":"Foglizzo"},{"last_name":"Ford","full_name":"Ford, Saavik","first_name":"Saavik"},{"first_name":"Jean-Baptiste","full_name":"Fouvry, Jean-Baptiste","last_name":"Fouvry"},{"first_name":"Alessia","full_name":"Franchini, Alessia","last_name":"Franchini"},{"last_name":"Fragos","full_name":"Fragos, Tassos","first_name":"Tassos"},{"last_name":"Fryer","full_name":"Fryer, Chris","first_name":"Chris"},{"last_name":"Gaspari","full_name":"Gaspari, Massimo","first_name":"Massimo"},{"full_name":"Gerosa, Davide","first_name":"Davide","last_name":"Gerosa"},{"full_name":"Graziani, Luca","first_name":"Luca","last_name":"Graziani"},{"first_name":"Paul","full_name":"Groot, Paul","last_name":"Groot"},{"last_name":"Habouzit","first_name":"Melanie","full_name":"Habouzit, Melanie"},{"first_name":"Daryl","full_name":"Haggard, Daryl","last_name":"Haggard"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"first_name":"Wen-Biao","full_name":"Han, Wen-Biao","last_name":"Han"},{"full_name":"Istrate, Alina","first_name":"Alina","last_name":"Istrate"},{"last_name":"Johansson","first_name":"Peter H.","full_name":"Johansson, Peter H."},{"first_name":"Fazeel Mahmood","full_name":"Khan, Fazeel Mahmood","last_name":"Khan"},{"last_name":"Kimpson","first_name":"Tomas","full_name":"Kimpson, Tomas"},{"first_name":"Kostas","full_name":"Kokkotas, Kostas","last_name":"Kokkotas"},{"first_name":"Albert","full_name":"Kong, Albert","last_name":"Kong"},{"last_name":"Korol","full_name":"Korol, Valeriya","first_name":"Valeriya"},{"first_name":"Kyle","full_name":"Kremer, Kyle","last_name":"Kremer"},{"first_name":"Thomas","full_name":"Kupfer, Thomas","last_name":"Kupfer"},{"last_name":"Lamberts","full_name":"Lamberts, Astrid","first_name":"Astrid"},{"last_name":"Larson","full_name":"Larson, Shane","first_name":"Shane"},{"full_name":"Lau, Mike","first_name":"Mike","last_name":"Lau"},{"last_name":"Liu","full_name":"Liu, Dongliang","first_name":"Dongliang"},{"first_name":"Nicole","full_name":"Lloyd-Ronning, Nicole","last_name":"Lloyd-Ronning"},{"full_name":"Lodato, Giuseppe","first_name":"Giuseppe","last_name":"Lodato"},{"last_name":"Lupi","full_name":"Lupi, Alessandro","first_name":"Alessandro"},{"last_name":"Ma","full_name":"Ma, Chung-Pei","first_name":"Chung-Pei"},{"last_name":"Maccarone","full_name":"Maccarone, Tomas","first_name":"Tomas"},{"last_name":"Mandel","first_name":"Ilya","full_name":"Mandel, Ilya"},{"first_name":"Alberto","full_name":"Mangiagli, Alberto","last_name":"Mangiagli"},{"full_name":"Mapelli, Michela","first_name":"Michela","last_name":"Mapelli"},{"last_name":"Mathis","first_name":"Stéphane","full_name":"Mathis, Stéphane"},{"last_name":"Mayer","first_name":"Lucio","full_name":"Mayer, Lucio"},{"full_name":"McGee, Sean","first_name":"Sean","last_name":"McGee"},{"first_name":"Berry","full_name":"McKernan, Berry","last_name":"McKernan"},{"last_name":"Miller","full_name":"Miller, M. Coleman","first_name":"M. Coleman"},{"last_name":"Mota","first_name":"David F.","full_name":"Mota, David F."},{"first_name":"Matthew","full_name":"Mumpower, Matthew","last_name":"Mumpower"},{"last_name":"Nasim","full_name":"Nasim, Syeda S.","first_name":"Syeda S."},{"full_name":"Nelemans, Gijs","first_name":"Gijs","last_name":"Nelemans"},{"first_name":"Scott","full_name":"Noble, Scott","last_name":"Noble"},{"last_name":"Pacucci","full_name":"Pacucci, Fabio","first_name":"Fabio"},{"last_name":"Panessa","first_name":"Francesca","full_name":"Panessa, Francesca"},{"last_name":"Paschalidis","full_name":"Paschalidis, Vasileios","first_name":"Vasileios"},{"last_name":"Pfister","full_name":"Pfister, Hugo","first_name":"Hugo"},{"first_name":"Delphine","full_name":"Porquet, Delphine","last_name":"Porquet"},{"full_name":"Quenby, John","first_name":"John","last_name":"Quenby"},{"full_name":"Ricarte, Angelo","first_name":"Angelo","last_name":"Ricarte"},{"last_name":"Röpke","first_name":"Friedrich K.","full_name":"Röpke, Friedrich K."},{"full_name":"Regan, John","first_name":"John","last_name":"Regan"},{"first_name":"Stephan","full_name":"Rosswog, Stephan","last_name":"Rosswog"},{"full_name":"Ruiter, Ashley","first_name":"Ashley","last_name":"Ruiter"},{"first_name":"Milton","full_name":"Ruiz, Milton","last_name":"Ruiz"},{"full_name":"Runnoe, Jessie","first_name":"Jessie","last_name":"Runnoe"},{"last_name":"Schneider","full_name":"Schneider, Raffaella","first_name":"Raffaella"},{"last_name":"Schnittman","first_name":"Jeremy","full_name":"Schnittman, Jeremy"},{"first_name":"Amy","full_name":"Secunda, Amy","last_name":"Secunda"},{"full_name":"Sesana, Alberto","first_name":"Alberto","last_name":"Sesana"},{"full_name":"Seto, Naoki","first_name":"Naoki","last_name":"Seto"},{"first_name":"Lijing","full_name":"Shao, Lijing","last_name":"Shao"},{"first_name":"Stuart","full_name":"Shapiro, Stuart","last_name":"Shapiro"},{"last_name":"Sopuerta","first_name":"Carlos","full_name":"Sopuerta, Carlos"},{"full_name":"Stone, Nicholas C.","first_name":"Nicholas C.","last_name":"Stone"},{"full_name":"Suvorov, Arthur","first_name":"Arthur","last_name":"Suvorov"},{"last_name":"Tamanini","first_name":"Nicola","full_name":"Tamanini, Nicola"},{"last_name":"Tamfal","full_name":"Tamfal, Tomas","first_name":"Tomas"},{"last_name":"Tauris","first_name":"Thomas","full_name":"Tauris, Thomas"},{"last_name":"Temmink","first_name":"Karel","full_name":"Temmink, Karel"},{"last_name":"Tomsick","first_name":"John","full_name":"Tomsick, John"},{"last_name":"Toonen","first_name":"Silvia","full_name":"Toonen, Silvia"},{"first_name":"Alejandro","full_name":"Torres-Orjuela, Alejandro","last_name":"Torres-Orjuela"},{"first_name":"Martina","full_name":"Toscani, Martina","last_name":"Toscani"},{"last_name":"Tsokaros","full_name":"Tsokaros, Antonios","first_name":"Antonios"},{"full_name":"Unal, Caner","first_name":"Caner","last_name":"Unal"},{"last_name":"Vázquez-Aceves","full_name":"Vázquez-Aceves, Verónica","first_name":"Verónica"},{"last_name":"Valiante","first_name":"Rosa","full_name":"Valiante, Rosa"},{"last_name":"van Putten","full_name":"van Putten, Maurice","first_name":"Maurice"},{"first_name":"Jan","full_name":"van Roestel, Jan","last_name":"van Roestel"},{"first_name":"Christian","full_name":"Vignali, Christian","last_name":"Vignali"},{"full_name":"Volonteri, Marta","first_name":"Marta","last_name":"Volonteri"},{"last_name":"Wu","first_name":"Kinwah","full_name":"Wu, Kinwah"},{"full_name":"Younsi, Ziri","first_name":"Ziri","last_name":"Younsi"},{"last_name":"Yu","full_name":"Yu, Shenghua","first_name":"Shenghua"},{"first_name":"Silvia","full_name":"Zane, Silvia","last_name":"Zane"},{"full_name":"Zwick, Lorenz","first_name":"Lorenz","last_name":"Zwick"},{"full_name":"Antonini, Fabio","first_name":"Fabio","last_name":"Antonini"},{"last_name":"Baibhav","first_name":"Vishal","full_name":"Baibhav, Vishal"},{"first_name":"Enrico","full_name":"Barausse, Enrico","last_name":"Barausse"},{"last_name":"Bonilla Rivera","first_name":"Alexander","full_name":"Bonilla Rivera, Alexander"},{"full_name":"Branchesi, Marica","first_name":"Marica","last_name":"Branchesi"},{"last_name":"Branduardi-Raymont","first_name":"Graziella","full_name":"Branduardi-Raymont, Graziella"},{"first_name":"Kevin","full_name":"Burdge, Kevin","last_name":"Burdge"},{"first_name":"Srija","full_name":"Chakraborty, Srija","last_name":"Chakraborty"},{"full_name":"Cuadra, Jorge","first_name":"Jorge","last_name":"Cuadra"},{"full_name":"Dage, Kristen","first_name":"Kristen","last_name":"Dage"},{"first_name":"Benjamin","full_name":"Davis, Benjamin","last_name":"Davis"},{"last_name":"de Mink","first_name":"Selma E.","full_name":"de Mink, Selma E."},{"full_name":"Decarli, Roberto","first_name":"Roberto","last_name":"Decarli"},{"first_name":"Daniela","full_name":"Doneva, Daniela","last_name":"Doneva"},{"last_name":"Escoffier","full_name":"Escoffier, Stephanie","first_name":"Stephanie"},{"full_name":"Gandhi, Poshak","first_name":"Poshak","last_name":"Gandhi"},{"full_name":"Haardt, Francesco","first_name":"Francesco","last_name":"Haardt"},{"last_name":"Lousto","first_name":"Carlos O.","full_name":"Lousto, Carlos O."},{"last_name":"Nissanke","full_name":"Nissanke, Samaya","first_name":"Samaya"},{"last_name":"Nordhaus","full_name":"Nordhaus, Jason","first_name":"Jason"},{"last_name":"O’Shaughnessy","first_name":"Richard","full_name":"O’Shaughnessy, Richard"},{"last_name":"Portegies Zwart","full_name":"Portegies Zwart, Simon","first_name":"Simon"},{"last_name":"Pound","first_name":"Adam","full_name":"Pound, Adam"},{"last_name":"Schussler","first_name":"Fabian","full_name":"Schussler, Fabian"},{"last_name":"Sergijenko","full_name":"Sergijenko, Olga","first_name":"Olga"},{"last_name":"Spallicci","first_name":"Alessandro","full_name":"Spallicci, Alessandro"},{"last_name":"Vernieri","first_name":"Daniele","full_name":"Vernieri, Daniele"},{"last_name":"Vigna-Gómez","full_name":"Vigna-Gómez, Alejandro","first_name":"Alejandro"}],"article_processing_charge":"No","year":"2023","oa":1,"main_file_link":[{"url":"https://doi.org/10.1007/s41114-022-00041-y","open_access":"1"}],"oa_version":"Published Version","issue":"1","intvolume":"        26","month":"03","date_updated":"2024-09-19T07:31:45Z","abstract":[{"text":"The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA’s first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultra-compact stellar-mass binaries, massive black hole binaries, and extreme or interme-diate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe.","lang":"eng"}],"title":"Astrophysics with the laser interferometer space antenna","doi":"10.1007/s41114-022-00041-y","publisher":"Springer Science and Business Media LLC","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","type":"journal_article","status":"public","_id":"17573","fulldoi":"https://doi.org/10.1007/s41114-022-00041-y","language":[{"iso":"eng"}],"day":"14","date_published":"2023-03-14T00:00:00Z"},{"title":"High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei","abstract":[{"text":"Some Seyfert galaxies are detected in high-energy gamma rays, but the mechanism and site of gamma-ray emission are unknown. Also, the origins of the cosmic high-energy neutrino and MeV gamma-ray backgrounds have been veiled in mystery since their discoveries. We propose emission from stellar-mass BHs (sBHs) embedded in disks of active galactic nuclei as their possible sources. These sBHs are predicted to launch jets due to the Blandford–Znajek mechanism, which can produce intense electromagnetic, neutrino, and cosmic-ray emissions. We investigate whether these emissions can be the sources of cosmic high-energy particles. We find that emission from internal shocks in the jets can explain gamma rays from nearby radio-quiet Seyfert galaxies including NGC 1068, if the Lorentz factor of the jets (Γj) is high. On the other hand, for moderate Γj, the emission can significantly contribute to the background gamma-ray and neutrino intensities in the ~MeV and ≲PeV bands, respectively. Furthermore, for moderate Γj with efficient amplification of the magnetic field and cosmic-ray acceleration, the neutrino emission from NGC 1068 and the ultrahigh-energy cosmic rays can be explained. These results suggest that the neutrino flux from NGC 1068 as well as the background intensities of MeV gamma rays, neutrinos, and the ultrahigh-energy cosmic rays can be explained by a unified model. Future MeV gamma-ray satellites will test our scenario for neutrino emission.","lang":"eng"}],"date_updated":"2024-09-19T11:45:10Z","type":"journal_article","_id":"17584","status":"public","publisher":"American Astronomical Society","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","doi":"10.3847/1538-4357/ace71d","date_published":"2023-09-12T00:00:00Z","day":"12","fulldoi":"https://doi.org/10.3847/1538-4357/ace71d","language":[{"iso":"eng"}],"scopus_import":"1","date_created":"2024-09-05T12:28:06Z","publication":"The Astrophysical Journal","citation":{"short":"H. Tagawa, S.S. Kimura, Z. Haiman, The Astrophysical Journal 955 (2023).","apa":"Tagawa, H., Kimura, S. S., &#38; Haiman, Z. (2023). High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ace71d\">https://doi.org/10.3847/1538-4357/ace71d</a>","ieee":"H. Tagawa, S. S. Kimura, and Z. Haiman, “High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei,” <i>The Astrophysical Journal</i>, vol. 955, no. 1. American Astronomical Society, 2023.","chicago":"Tagawa, Hiromichi, Shigeo S. Kimura, and Zoltán Haiman. “High-Energy Electromagnetic, Neutrino, and Cosmic-Ray Emission by Stellar-Mass Black Holes in Disks of Active Galactic Nuclei.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2023. <a href=\"https://doi.org/10.3847/1538-4357/ace71d\">https://doi.org/10.3847/1538-4357/ace71d</a>.","ista":"Tagawa H, Kimura SS, Haiman Z. 2023. High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei. The Astrophysical Journal. 955(1), 23.","mla":"Tagawa, Hiromichi, et al. “High-Energy Electromagnetic, Neutrino, and Cosmic-Ray Emission by Stellar-Mass Black Holes in Disks of Active Galactic Nuclei.” <i>The Astrophysical Journal</i>, vol. 955, no. 1, 23, American Astronomical Society, 2023, doi:<a href=\"https://doi.org/10.3847/1538-4357/ace71d\">10.3847/1538-4357/ace71d</a>.","ama":"Tagawa H, Kimura SS, Haiman Z. High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei. <i>The Astrophysical Journal</i>. 2023;955(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ace71d\">10.3847/1538-4357/ace71d</a>"},"extern":"1","publication_identifier":{"issn":["0004-637X","1538-4357"]},"volume":955,"quality_controlled":"1","article_number":"23","publication_status":"published","article_type":"original","author":[{"last_name":"Tagawa","full_name":"Tagawa, Hiromichi","first_name":"Hiromichi"},{"last_name":"Kimura","full_name":"Kimura, Shigeo S.","first_name":"Shigeo S."},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán","last_name":"Haiman"}],"month":"09","oa_version":"Published Version","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/ace71d"}],"issue":"1","intvolume":"       955","article_processing_charge":"No","oa":1,"year":"2023"},{"article_number":"13","publication_identifier":{"issn":["0004-637X","1538-4357"]},"volume":950,"quality_controlled":"1","citation":{"chicago":"Tagawa, Hiromichi, Shigeo S. Kimura, Zoltán Haiman, Rosalba Perna, and Imre Bartos. “Observable Signature of Merging Stellar-Mass Black Holes in Active Galactic Nuclei.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2023. <a href=\"https://doi.org/10.3847/1538-4357/acc4bb\">https://doi.org/10.3847/1538-4357/acc4bb</a>.","short":"H. Tagawa, S.S. Kimura, Z. Haiman, R. Perna, I. Bartos, The Astrophysical Journal 950 (2023).","apa":"Tagawa, H., Kimura, S. S., Haiman, Z., Perna, R., &#38; Bartos, I. (2023). Observable signature of merging stellar-mass black holes in active galactic nuclei. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/acc4bb\">https://doi.org/10.3847/1538-4357/acc4bb</a>","ieee":"H. Tagawa, S. S. Kimura, Z. Haiman, R. Perna, and I. Bartos, “Observable signature of merging stellar-mass black holes in active galactic nuclei,” <i>The Astrophysical Journal</i>, vol. 950, no. 1. American Astronomical Society, 2023.","ama":"Tagawa H, Kimura SS, Haiman Z, Perna R, Bartos I. Observable signature of merging stellar-mass black holes in active galactic nuclei. <i>The Astrophysical Journal</i>. 2023;950(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/acc4bb\">10.3847/1538-4357/acc4bb</a>","mla":"Tagawa, Hiromichi, et al. “Observable Signature of Merging Stellar-Mass Black Holes in Active Galactic Nuclei.” <i>The Astrophysical Journal</i>, vol. 950, no. 1, 13, American Astronomical Society, 2023, doi:<a href=\"https://doi.org/10.3847/1538-4357/acc4bb\">10.3847/1538-4357/acc4bb</a>.","ista":"Tagawa H, Kimura SS, Haiman Z, Perna R, Bartos I. 2023. Observable signature of merging stellar-mass black holes in active galactic nuclei. The Astrophysical Journal. 950(1), 13."},"extern":"1","scopus_import":"1","date_created":"2024-09-05T12:41:47Z","publication":"The Astrophysical Journal","article_processing_charge":"No","year":"2023","oa":1,"month":"06","issue":"1","intvolume":"       950","oa_version":"Published Version","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/acc4bb"}],"publication_status":"published","article_type":"original","author":[{"full_name":"Tagawa, Hiromichi","first_name":"Hiromichi","last_name":"Tagawa"},{"first_name":"Shigeo S.","full_name":"Kimura, Shigeo S.","last_name":"Kimura"},{"last_name":"Haiman","full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"first_name":"Rosalba","full_name":"Perna, Rosalba","last_name":"Perna"},{"first_name":"Imre","full_name":"Bartos, Imre","last_name":"Bartos"}],"publisher":"American Astronomical Society","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","doi":"10.3847/1538-4357/acc4bb","type":"journal_article","status":"public","_id":"17594","date_updated":"2024-09-23T12:36:58Z","title":"Observable signature of merging stellar-mass black holes in active galactic nuclei","abstract":[{"text":"The origin of stellar-mass black hole mergers discovered through gravitational waves is being widely debated. Mergers in the disks of active galactic nuclei (AGNs) represent a promising source of origin, with possible observational clues in the gravitational-wave data. Beyond gravitational waves, a unique signature of AGN-assisted mergers is electromagnetic emission from the accreting black holes. Here we show that jets launched by accreting black holes merging in an AGN disk can be detected as peculiar transients by infrared, optical, and X-ray observatories. We further show that this emission mechanism can explain the possible associations between gravitational-wave events and the optical transient ZTF 19abanrhr and the proposed gamma-ray counterparts GW150914-GBM and LVT151012-GBM. We demonstrate how these associations, if genuine, can be used to reconstruct the properties of these events’ environments. Searching for infrared and X-ray counterparts to similar electromagnetic transients in the future, once host galaxies are localized by optical observations, could provide a smoking-gun signature of the mergers’ AGN origin.","lang":"eng"}],"fulldoi":"https://doi.org/10.3847/1538-4357/acc4bb","language":[{"iso":"eng"}],"date_published":"2023-06-06T00:00:00Z","day":"06"},{"fulldoi":"https://doi.org/10.1093/mnras/stad1926","language":[{"iso":"eng"}],"day":"03","date_published":"2023-07-03T00:00:00Z","page":"2770-2796","date_updated":"2024-09-23T13:42:19Z","abstract":[{"lang":"eng","text":"Motivated by the increasing number of detections of merging black holes by LIGO-VIRGO-KAGRA, black hole (BH) binary mergers in the discs of active galactic nuclei (AGNs) is investigated as a possible merger channel. In this pathway, BH encounters in the gas disc form mutually bound BH binary systems through interaction with the gas in the disc and subsequently inspiral through gravitational torques induced by the local gas. To determine the feasibility of this merger pathway, we present the first three-dimensional global hydrodynamic simulations of the formation and evolution of a stellar-mass BH binaries AGN discs with three different AGN disc masses and five different initial radial separations. These 15 simulations show binary capture of prograde and retrograde binaries can be successful in a range of disc densities including cases well below that of a standard radiatively efficient alpha disc, identifying that the majority of these captured binaries are then subsequently hardened by the surrounding gas. The eccentricity evolution depends strongly on the orbital rotation where prograde binaries are governed by gravitational torques form their circumbinary mini disc, with eccentricities being damped, while for retrograde binaries the eccentricities are excited to >∼ 0.9 by accretion torques. In two cases, retrograde binaries ultimately undergo a close periapsis passage which results in a merger via gravitational waves after only a few thousand binary orbits. Thus, the merger time-scale can be far shorter than the AGN disc lifetime. These simulations support an efficient AGN disc merger pathway for BHs."}],"title":"Black hole binary formation in AGN discs: from isolation to merger","doi":"10.1093/mnras/stad1926","publisher":"Oxford University Press","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","type":"journal_article","status":"public","_id":"17602","publication_status":"published","article_type":"original","author":[{"first_name":"Connar","full_name":"Rowan, Connar","last_name":"Rowan"},{"full_name":"Boekholt, Tjarda","first_name":"Tjarda","last_name":"Boekholt"},{"last_name":"Kocsis","first_name":"Bence","full_name":"Kocsis, Bence"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman"}],"article_processing_charge":"No","year":"2023","oa":1,"oa_version":"Published Version","issue":"2","intvolume":"       524","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stad1926","open_access":"1"}],"month":"07","extern":"1","citation":{"chicago":"Rowan, Connar, Tjarda Boekholt, Bence Kocsis, and Zoltán Haiman. “Black Hole Binary Formation in AGN Discs: From Isolation to Merger.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnras/stad1926\">https://doi.org/10.1093/mnras/stad1926</a>.","short":"C. Rowan, T. Boekholt, B. Kocsis, Z. Haiman, Monthly Notices of the Royal Astronomical Society 524 (2023) 2770–2796.","ieee":"C. Rowan, T. Boekholt, B. Kocsis, and Z. Haiman, “Black hole binary formation in AGN discs: from isolation to merger,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 524, no. 2. Oxford University Press, pp. 2770–2796, 2023.","apa":"Rowan, C., Boekholt, T., Kocsis, B., &#38; Haiman, Z. (2023). Black hole binary formation in AGN discs: from isolation to merger. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stad1926\">https://doi.org/10.1093/mnras/stad1926</a>","mla":"Rowan, Connar, et al. “Black Hole Binary Formation in AGN Discs: From Isolation to Merger.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 524, no. 2, Oxford University Press, 2023, pp. 2770–96, doi:<a href=\"https://doi.org/10.1093/mnras/stad1926\">10.1093/mnras/stad1926</a>.","ama":"Rowan C, Boekholt T, Kocsis B, Haiman Z. Black hole binary formation in AGN discs: from isolation to merger. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;524(2):2770-2796. doi:<a href=\"https://doi.org/10.1093/mnras/stad1926\">10.1093/mnras/stad1926</a>","ista":"Rowan C, Boekholt T, Kocsis B, Haiman Z. 2023. Black hole binary formation in AGN discs: from isolation to merger. Monthly Notices of the Royal Astronomical Society. 524(2), 2770–2796."},"publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","date_created":"2024-09-05T13:09:11Z","quality_controlled":"1","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":524},{"article_number":"L4","quality_controlled":"1","volume":951,"publication_identifier":{"issn":["2041-8205","2041-8213"]},"extern":"1","citation":{"ama":"Wang F, Yang J, Hennawi JF, et al. A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar. <i>The Astrophysical Journal Letters</i>. 2023;951(1). doi:<a href=\"https://doi.org/10.3847/2041-8213/accd6f\">10.3847/2041-8213/accd6f</a>","mla":"Wang, Feige, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar.” <i>The Astrophysical Journal Letters</i>, vol. 951, no. 1, L4, American Astronomical Society, 2023, doi:<a href=\"https://doi.org/10.3847/2041-8213/accd6f\">10.3847/2041-8213/accd6f</a>.","ista":"Wang F, Yang J, Hennawi JF, Fan X, Sun F, Champagne JB, Costa T, Habouzit M, Endsley R, Li Z, Lin X, Meyer RA, Schindler J, Wu Y, Bañados E, Barth AJ, Bhowmick AK, Bieri R, Blecha L, Bosman S, Cai Z, Colina L, Connor T, Davies FB, Decarli R, De Rosa G, Drake AB, Egami E, Eilers A-C, Evans AE, Farina EP, Haiman Z, Jiang L, Jin X, Jun HD, Kakiichi K, Khusanova Y, Kulkarni G, Li M, Liu W, Loiacono F, Lupi A, Mazzucchelli C, Onoue M, Pudoka MA, Rojas-Ruiz S, Shen Y, Strauss MA, Tee WL, Trakhtenbrot B, Trebitsch M, Venemans B, Volonteri M, Walter F, Xie Z-L, Yue M, Zhang H, Zhang H, Zou S. 2023. A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar. The Astrophysical Journal Letters. 951(1), L4.","chicago":"Wang, Feige, Jinyi Yang, Joseph F. Hennawi, Xiaohui Fan, Fengwu Sun, Jaclyn B. Champagne, Tiago Costa, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2023. <a href=\"https://doi.org/10.3847/2041-8213/accd6f\">https://doi.org/10.3847/2041-8213/accd6f</a>.","short":"F. Wang, J. Yang, J.F. Hennawi, X. Fan, F. Sun, J.B. Champagne, T. Costa, M. Habouzit, R. Endsley, Z. Li, X. Lin, R.A. Meyer, J. Schindler, Y. Wu, E. Bañados, A.J. Barth, A.K. Bhowmick, R. Bieri, L. Blecha, S. Bosman, Z. Cai, L. Colina, T. Connor, F.B. Davies, R. Decarli, G. De Rosa, A.B. Drake, E. Egami, A.-C. Eilers, A.E. Evans, E.P. Farina, Z. Haiman, L. Jiang, X. Jin, H.D. Jun, K. Kakiichi, Y. Khusanova, G. Kulkarni, M. Li, W. Liu, F. Loiacono, A. Lupi, C. Mazzucchelli, M. Onoue, M.A. Pudoka, S. Rojas-Ruiz, Y. Shen, M.A. Strauss, W.L. Tee, B. Trakhtenbrot, M. Trebitsch, B. Venemans, M. Volonteri, F. Walter, Z.-L. Xie, M. Yue, H. Zhang, H. Zhang, S. Zou, The Astrophysical Journal Letters 951 (2023).","apa":"Wang, F., Yang, J., Hennawi, J. F., Fan, X., Sun, F., Champagne, J. B., … Zou, S. (2023). A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/accd6f\">https://doi.org/10.3847/2041-8213/accd6f</a>","ieee":"F. Wang <i>et al.</i>, “A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar,” <i>The Astrophysical Journal Letters</i>, vol. 951, no. 1. American Astronomical Society, 2023."},"publication":"The Astrophysical Journal Letters","date_created":"2024-09-05T13:14:46Z","scopus_import":"1","oa":1,"year":"2023","article_processing_charge":"No","oa_version":"Published Version","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/2041-8213/accd6f"}],"issue":"1","intvolume":"       951","month":"06","author":[{"last_name":"Wang","first_name":"Feige","full_name":"Wang, Feige"},{"last_name":"Yang","first_name":"Jinyi","full_name":"Yang, Jinyi"},{"last_name":"Hennawi","full_name":"Hennawi, Joseph F.","first_name":"Joseph F."},{"first_name":"Xiaohui","full_name":"Fan, Xiaohui","last_name":"Fan"},{"last_name":"Sun","full_name":"Sun, Fengwu","first_name":"Fengwu"},{"first_name":"Jaclyn B.","full_name":"Champagne, Jaclyn B.","last_name":"Champagne"},{"full_name":"Costa, Tiago","first_name":"Tiago","last_name":"Costa"},{"last_name":"Habouzit","full_name":"Habouzit, Melanie","first_name":"Melanie"},{"first_name":"Ryan","full_name":"Endsley, Ryan","last_name":"Endsley"},{"first_name":"Zihao","full_name":"Li, Zihao","last_name":"Li"},{"full_name":"Lin, Xiaojing","first_name":"Xiaojing","last_name":"Lin"},{"last_name":"Meyer","full_name":"Meyer, Romain A.","first_name":"Romain A."},{"full_name":"Schindler, Jan–Torge","first_name":"Jan–Torge","last_name":"Schindler"},{"last_name":"Wu","full_name":"Wu, Yunjing","first_name":"Yunjing"},{"last_name":"Bañados","full_name":"Bañados, Eduardo","first_name":"Eduardo"},{"last_name":"Barth","first_name":"Aaron J.","full_name":"Barth, Aaron J."},{"full_name":"Bhowmick, Aklant K.","first_name":"Aklant K.","last_name":"Bhowmick"},{"first_name":"Rebekka","full_name":"Bieri, Rebekka","last_name":"Bieri"},{"full_name":"Blecha, Laura","first_name":"Laura","last_name":"Blecha"},{"full_name":"Bosman, Sarah","first_name":"Sarah","last_name":"Bosman"},{"full_name":"Cai, Zheng","first_name":"Zheng","last_name":"Cai"},{"full_name":"Colina, Luis","first_name":"Luis","last_name":"Colina"},{"first_name":"Thomas","full_name":"Connor, Thomas","last_name":"Connor"},{"first_name":"Frederick B.","full_name":"Davies, Frederick B.","last_name":"Davies"},{"last_name":"Decarli","full_name":"Decarli, Roberto","first_name":"Roberto"},{"last_name":"De Rosa","first_name":"Gisella","full_name":"De Rosa, Gisella"},{"last_name":"Drake","full_name":"Drake, Alyssa B.","first_name":"Alyssa B."},{"full_name":"Egami, Eiichi","first_name":"Eiichi","last_name":"Egami"},{"full_name":"Eilers, Anna-Christina","first_name":"Anna-Christina","last_name":"Eilers"},{"last_name":"Evans","first_name":"Analis E.","full_name":"Evans, Analis E."},{"last_name":"Farina","full_name":"Farina, Emanuele Paolo","first_name":"Emanuele Paolo"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"first_name":"Linhua","full_name":"Jiang, Linhua","last_name":"Jiang"},{"last_name":"Jin","full_name":"Jin, Xiangyu","first_name":"Xiangyu"},{"full_name":"Jun, Hyunsung D.","first_name":"Hyunsung D.","last_name":"Jun"},{"first_name":"Koki","full_name":"Kakiichi, Koki","last_name":"Kakiichi"},{"last_name":"Khusanova","full_name":"Khusanova, Yana","first_name":"Yana"},{"full_name":"Kulkarni, Girish","first_name":"Girish","last_name":"Kulkarni"},{"first_name":"Mingyu","full_name":"Li, Mingyu","last_name":"Li"},{"first_name":"Weizhe","full_name":"Liu, Weizhe","last_name":"Liu"},{"last_name":"Loiacono","first_name":"Federica","full_name":"Loiacono, Federica"},{"full_name":"Lupi, Alessandro","first_name":"Alessandro","last_name":"Lupi"},{"last_name":"Mazzucchelli","full_name":"Mazzucchelli, Chiara","first_name":"Chiara"},{"first_name":"Masafusa","full_name":"Onoue, Masafusa","last_name":"Onoue"},{"first_name":"Maria A.","full_name":"Pudoka, Maria A.","last_name":"Pudoka"},{"last_name":"Rojas-Ruiz","full_name":"Rojas-Ruiz, Sofía","first_name":"Sofía"},{"full_name":"Shen, Yue","first_name":"Yue","last_name":"Shen"},{"first_name":"Michael A.","full_name":"Strauss, Michael A.","last_name":"Strauss"},{"last_name":"Tee","full_name":"Tee, Wei Leong","first_name":"Wei Leong"},{"last_name":"Trakhtenbrot","full_name":"Trakhtenbrot, Benny","first_name":"Benny"},{"full_name":"Trebitsch, Maxime","first_name":"Maxime","last_name":"Trebitsch"},{"full_name":"Venemans, Bram","first_name":"Bram","last_name":"Venemans"},{"last_name":"Volonteri","full_name":"Volonteri, Marta","first_name":"Marta"},{"last_name":"Walter","first_name":"Fabian","full_name":"Walter, Fabian"},{"first_name":"Zhang-Liang","full_name":"Xie, Zhang-Liang","last_name":"Xie"},{"last_name":"Yue","first_name":"Minghao","full_name":"Yue, Minghao"},{"last_name":"Zhang","full_name":"Zhang, Haowen","first_name":"Haowen"},{"last_name":"Zhang","first_name":"Huanian","full_name":"Zhang, Huanian"},{"first_name":"Siwei","full_name":"Zou, Siwei","last_name":"Zou"}],"publication_status":"published","article_type":"original","doi":"10.3847/2041-8213/accd6f","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publisher":"American Astronomical Society","_id":"17606","status":"public","type":"journal_article","date_updated":"2024-09-23T14:08:58Z","abstract":[{"text":"We present the first results from the JWST ASPIRE program (A SPectroscopic survey of biased halos In the Reionization Era). This program represents an imaging and spectroscopic survey of 25 reionization-era quasars and their environments by utilizing the unprecedented capabilities of NIRCam Wide Field Slitless Spectroscopy (WFSS) mode. ASPIRE will deliver the largest (∼280 arcmin^2) galaxy redshift survey at 3-4 μm among JWST Cycle-1 programs and provide extensive legacy values for studying the formation of the earliest supermassive black holes (SMBHs), the assembly of galaxies, early metal enrichment, and cosmic reionization. In this first ASPIRE paper, we report the discovery of a filamentary structure traced by the luminous quasar J0305-3150 and ten [OIII] emitters at z=6.6. This structure has a 3D galaxy overdensity of δgal=12.6 over 637 cMpc3, one of the most overdense structures known in the early universe, and could eventually evolve into a massive galaxy cluster. Together with existing VLT/MUSE and ALMA observations of this field, our JWST observations reveal that J0305-3150 traces a complex environment where both UV-bright and dusty galaxies are present, and indicate that the early evolution of galaxies around the quasar is not simultaneous. In addition, we discovered 31 [OIII] emitters in this field at other redshifts, 5.3<z<6.7, with half of them situated at z∼5.4 and z∼6.2. This indicates that star-forming galaxies, such as [OIII] emitters, are generally clustered at high redshifts. These discoveries demonstrate the unparalleled redshift survey capabilities of NIRCam WFSS and the potential of the full ASPIRE survey dataset.","lang":"eng"}],"title":"A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar","language":[{"iso":"eng"}],"fulldoi":"https://doi.org/10.3847/2041-8213/accd6f","date_published":"2023-06-29T00:00:00Z","day":"29"},{"article_type":"original","publication_status":"published","author":[{"last_name":"Komossa","first_name":"S","full_name":"Komossa, S"},{"first_name":"D","full_name":"Grupe, D","last_name":"Grupe"},{"full_name":"Kraus, A","first_name":"A","last_name":"Kraus"},{"first_name":"M A","full_name":"Gurwell, M A","last_name":"Gurwell"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán","last_name":"Haiman"},{"full_name":"Liu, F K","first_name":"F K","last_name":"Liu"},{"full_name":"Tchekhovskoy, A","first_name":"A","last_name":"Tchekhovskoy"},{"full_name":"Gallo, L C","first_name":"L C","last_name":"Gallo"},{"first_name":"M","full_name":"Berton, M","last_name":"Berton"},{"first_name":"R","full_name":"Blandford, R","last_name":"Blandford"},{"full_name":"Gómez, J L","first_name":"J L","last_name":"Gómez"},{"last_name":"Gonzalez","full_name":"Gonzalez, A G","first_name":"A G"}],"article_processing_charge":"No","oa":1,"year":"2023","oa_version":"Published Version","intvolume":"       522","issue":"1","main_file_link":[{"url":"https://doi.org/10.1093/mnrasl/slad016","open_access":"1"}],"month":"02","extern":"1","citation":{"ama":"Komossa S, Grupe D, Kraus A, et al. Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios. <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. 2023;522(1):L84-L88. doi:<a href=\"https://doi.org/10.1093/mnrasl/slad016\">10.1093/mnrasl/slad016</a>","mla":"Komossa, S., et al. “Absence of the Predicted 2022 October Outburst of OJ 287 and Implications for Binary SMBH Scenarios.” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>, vol. 522, no. 1, Oxford University Press, 2023, pp. L84–88, doi:<a href=\"https://doi.org/10.1093/mnrasl/slad016\">10.1093/mnrasl/slad016</a>.","ista":"Komossa S, Grupe D, Kraus A, Gurwell MA, Haiman Z, Liu FK, Tchekhovskoy A, Gallo LC, Berton M, Blandford R, Gómez JL, Gonzalez AG. 2023. Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios. Monthly Notices of the Royal Astronomical Society: Letters. 522(1), L84–L88.","chicago":"Komossa, S, D Grupe, A Kraus, M A Gurwell, Zoltán Haiman, F K Liu, A Tchekhovskoy, et al. “Absence of the Predicted 2022 October Outburst of OJ 287 and Implications for Binary SMBH Scenarios.” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnrasl/slad016\">https://doi.org/10.1093/mnrasl/slad016</a>.","apa":"Komossa, S., Grupe, D., Kraus, A., Gurwell, M. A., Haiman, Z., Liu, F. K., … Gonzalez, A. G. (2023). Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios. <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnrasl/slad016\">https://doi.org/10.1093/mnrasl/slad016</a>","ieee":"S. Komossa <i>et al.</i>, “Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios,” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>, vol. 522, no. 1. Oxford University Press, pp. L84–L88, 2023.","short":"S. Komossa, D. Grupe, A. Kraus, M.A. Gurwell, Z. Haiman, F.K. Liu, A. Tchekhovskoy, L.C. Gallo, M. Berton, R. Blandford, J.L. Gómez, A.G. Gonzalez, Monthly Notices of the Royal Astronomical Society: Letters 522 (2023) L84–L88."},"publication":"Monthly Notices of the Royal Astronomical Society: Letters","scopus_import":"1","date_created":"2024-09-05T13:23:29Z","quality_controlled":"1","volume":522,"publication_identifier":{"issn":["1745-3925","1745-3933"]},"fulldoi":"https://doi.org/10.1093/mnrasl/slad016","language":[{"iso":"eng"}],"day":"23","date_published":"2023-02-23T00:00:00Z","page":"L84-L88","date_updated":"2024-09-24T07:22:28Z","abstract":[{"text":"The project MOMO (Multiwavelength Observations and Modelling of OJ 287) was set up to test predictions of binary supermassive black hole (SMBH) scenarios and to understand disc–jet physics of the blazar OJ 287. After a correction, the precessing binary (PB) SMBH model predicted the next main outburst of OJ 287 in 2022 October, making the outburst well observable and the model testable. We have densely covered this period in our ongoing multifrequency radio, optical, ultraviolet (UV), and X-ray monitoring. The predicted outburst was not detected. Instead, OJ 287 was at low optical–UV emission levels, declining further into November. The predicted thermal bremsstrahlung spectrum was not observed either, at any epoch. Further, applying scaling relations, we estimate an SMBH mass of OJ 287 of 108 M⊙. The latest in a sequence of deep low states that recur every 1–2 yr is used to determine an upper limit on the Eddington ratio and on the accretion-disc luminosity. This limit is at least a factor of 10 lower than required by the PB model with its massive primary SMBH of &amp;gt;1010 M⊙. All these results favour alternative binary SMBH models of OJ 287 that require neither strong orbital precession nor a very large mass of the primary SMBH.","lang":"eng"}],"title":"Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios","doi":"10.1093/mnrasl/slad016","publisher":"Oxford University Press","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","type":"journal_article","status":"public","_id":"17611"},{"abstract":[{"lang":"eng","text":"Understanding and tuning charge transport over a single molecule is a fundamental topic in molecular electronics. Single-molecule junctions composed of individual molecules attached to two electrodes are the most common components built for single-molecule charge transport studies. During the past two decades, rapid technical and theoretical advances in single-molecule junctions have increased our understanding of the conductance properties and functions of molecular devices. In this perspective article, we introduce the basic principles of charge transport in single-molecule junctions, then give an overview of recent progress in modulating single-molecule transport through external stimuli such as electric field and potential, light, mechanical force, heat, and chemical environment. Lastly, we discuss challenges and offer views on future developments in molecular electronics."}],"title":"Modulating single-molecule charge transport through external stimulus","date_updated":"2024-11-25T12:41:14Z","_id":"17863","status":"public","type":"journal_article","doi":"10.1016/j.esci.2023.100115","user_id":"68b8ca59-c5b3-11ee-8790-cd641c68093d","publisher":"Elsevier BV","date_published":"2023-05-01T00:00:00Z","language":[{"iso":"eng"}],"fulldoi":"https://doi.org/10.1016/j.esci.2023.100115","publication":"eScience","date_created":"2024-09-06T12:56:54Z","scopus_import":"1","extern":"1","citation":{"mla":"Zou, Qi, et al. “Modulating Single-Molecule Charge Transport through External Stimulus.” <i>EScience</i>, vol. 3, no. 3, 100115, Elsevier BV, 2023, doi:<a href=\"https://doi.org/10.1016/j.esci.2023.100115\">10.1016/j.esci.2023.100115</a>.","ama":"Zou Q, Qiu J, Zang Y, Tian H, Venkataraman L. Modulating single-molecule charge transport through external stimulus. <i>eScience</i>. 2023;3(3). doi:<a href=\"https://doi.org/10.1016/j.esci.2023.100115\">10.1016/j.esci.2023.100115</a>","ista":"Zou Q, Qiu J, Zang Y, Tian H, Venkataraman L. 2023. Modulating single-molecule charge transport through external stimulus. eScience. 3(3), 100115.","chicago":"Zou, Qi, Jin Qiu, Yaping Zang, He Tian, and Latha Venkataraman. “Modulating Single-Molecule Charge Transport through External Stimulus.” <i>EScience</i>. Elsevier BV, 2023. <a href=\"https://doi.org/10.1016/j.esci.2023.100115\">https://doi.org/10.1016/j.esci.2023.100115</a>.","short":"Q. Zou, J. Qiu, Y. Zang, H. Tian, L. Venkataraman, EScience 3 (2023).","ieee":"Q. Zou, J. Qiu, Y. Zang, H. Tian, and L. Venkataraman, “Modulating single-molecule charge transport through external stimulus,” <i>eScience</i>, vol. 3, no. 3. Elsevier BV, 2023.","apa":"Zou, Q., Qiu, J., Zang, Y., Tian, H., &#38; Venkataraman, L. (2023). Modulating single-molecule charge transport through external stimulus. <i>EScience</i>. Elsevier BV. <a href=\"https://doi.org/10.1016/j.esci.2023.100115\">https://doi.org/10.1016/j.esci.2023.100115</a>"},"quality_controlled":"1","OA_place":"publisher","OA_type":"gold","volume":3,"publication_identifier":{"eissn":["2667-1417"]},"article_number":"100115","author":[{"last_name":"Zou","full_name":"Zou, Qi","first_name":"Qi"},{"last_name":"Qiu","full_name":"Qiu, Jin","first_name":"Jin"},{"full_name":"Zang, Yaping","first_name":"Yaping","last_name":"Zang"},{"last_name":"Tian","full_name":"Tian, He","first_name":"He"},{"first_name":"Latha","orcid":"0000-0002-6957-6089","full_name":"Venkataraman, Latha","id":"9ebb78a5-cc0d-11ee-8322-fae086a32caf","last_name":"Venkataraman"}],"article_type":"original","publication_status":"published","main_file_link":[{"url":"https://www.sciencedirect.com/science/article/pii/S2667141723000332?via%3Dihub","open_access":"1"}],"intvolume":"         3","oa_version":"Published Version","issue":"3","month":"05","year":"2023","oa":1,"article_processing_charge":"No"},{"day":"16","date_published":"2023-01-16T00:00:00Z","external_id":{"pmid":["36819847"]},"language":[{"iso":"eng"}],"fulldoi":"https://doi.org/10.1039/d2sc06411a","status":"public","_id":"17866","type":"journal_article","user_id":"68b8ca59-c5b3-11ee-8790-cd641c68093d","publisher":"Royal Society of Chemistry","doi":"10.1039/d2sc06411a","title":"Electric fields drive bond homolysis","abstract":[{"lang":"eng","text":"Electric fields have been used to control and direct chemical reactions in biochemistry and enzymatic catalysis, yet directly applying external electric fields to activate reactions in bulk solution and to characterize them ex situ remains a challenge. Here we utilize the scanning tunneling microscope-based break-junction technique to investigate the electric field driven homolytic cleavage of the radical initiator 4-(methylthio)benzoic peroxyanhydride at ambient temperatures in bulk solution, without the use of co-initiators or photochemical activators. Through time-dependent ex situ quantification by high performance liquid chromatography using a UV-vis detector, we find that the electric field catalyzes the reaction. Importantly, we demonstrate that the reaction rate in a field increases linearly with the solvent dielectric constant. Using density functional theory calculations, we show that the applied electric field decreases the dissociation energy of the O–O bond and stabilizes the product relative to the reactant due to their different dipole moments."}],"pmid":1,"date_updated":"2024-11-25T15:01:40Z","page":"1769-1774","month":"01","issue":"7","intvolume":"        14","oa_version":"Published Version","main_file_link":[{"open_access":"1","url":"https://europepmc.org/article/pmc/pmc9931054"}],"year":"2023","oa":1,"article_processing_charge":"Yes","author":[{"first_name":"Boyuan","full_name":"Zhang, Boyuan","last_name":"Zhang"},{"full_name":"Schaack, Cedric","first_name":"Cedric","last_name":"Schaack"},{"first_name":"Claudia R.","full_name":"Prindle, Claudia R.","last_name":"Prindle"},{"full_name":"Vo, Ethan A.","first_name":"Ethan A.","last_name":"Vo"},{"last_name":"Aziz","full_name":"Aziz, Miriam","first_name":"Miriam"},{"first_name":"Michael L.","full_name":"Steigerwald, Michael L.","last_name":"Steigerwald"},{"last_name":"Berkelbach","full_name":"Berkelbach, Timothy C.","first_name":"Timothy C."},{"full_name":"Nuckolls, Colin","first_name":"Colin","last_name":"Nuckolls"},{"id":"9ebb78a5-cc0d-11ee-8322-fae086a32caf","first_name":"Latha","orcid":"0000-0002-6957-6089","full_name":"Venkataraman, Latha","last_name":"Venkataraman"}],"article_type":"original","publication_status":"published","publication_identifier":{"eissn":["2041-6539"],"issn":["2041-6520"]},"volume":14,"quality_controlled":"1","OA_place":"publisher","OA_type":"gold","date_created":"2024-09-06T12:59:45Z","publication":"Chemical Science","citation":{"mla":"Zhang, Boyuan, et al. “Electric Fields Drive Bond Homolysis.” <i>Chemical Science</i>, vol. 14, no. 7, Royal Society of Chemistry, 2023, pp. 1769–74, doi:<a href=\"https://doi.org/10.1039/d2sc06411a\">10.1039/d2sc06411a</a>.","ama":"Zhang B, Schaack C, Prindle CR, et al. Electric fields drive bond homolysis. <i>Chemical Science</i>. 2023;14(7):1769-1774. doi:<a href=\"https://doi.org/10.1039/d2sc06411a\">10.1039/d2sc06411a</a>","ista":"Zhang B, Schaack C, Prindle CR, Vo EA, Aziz M, Steigerwald ML, Berkelbach TC, Nuckolls C, Venkataraman L. 2023. Electric fields drive bond homolysis. Chemical Science. 14(7), 1769–1774.","chicago":"Zhang, Boyuan, Cedric Schaack, Claudia R. Prindle, Ethan A. Vo, Miriam Aziz, Michael L. Steigerwald, Timothy C. Berkelbach, Colin Nuckolls, and Latha Venkataraman. “Electric Fields Drive Bond Homolysis.” <i>Chemical Science</i>. Royal Society of Chemistry, 2023. <a href=\"https://doi.org/10.1039/d2sc06411a\">https://doi.org/10.1039/d2sc06411a</a>.","short":"B. Zhang, C. Schaack, C.R. Prindle, E.A. Vo, M. Aziz, M.L. Steigerwald, T.C. Berkelbach, C. Nuckolls, L. Venkataraman, Chemical Science 14 (2023) 1769–1774.","apa":"Zhang, B., Schaack, C., Prindle, C. R., Vo, E. A., Aziz, M., Steigerwald, M. L., … Venkataraman, L. (2023). Electric fields drive bond homolysis. <i>Chemical Science</i>. Royal Society of Chemistry. <a href=\"https://doi.org/10.1039/d2sc06411a\">https://doi.org/10.1039/d2sc06411a</a>","ieee":"B. Zhang <i>et al.</i>, “Electric fields drive bond homolysis,” <i>Chemical Science</i>, vol. 14, no. 7. Royal Society of Chemistry, pp. 1769–1774, 2023."},"extern":"1"},{"date_published":"2023-06-21T00:00:00Z","day":"21","external_id":{"pmid":["37344594 "],"arxiv":["2210.10919"]},"fulldoi":"https://doi.org/10.1038/s41586-023-06122-4","language":[{"iso":"eng"}],"title":"Realization of a fractional quantum Hall state with ultracold atoms","abstract":[{"text":"Strongly interacting topological matter1 exhibits fundamentally new phenomena with potential applications in quantum information technology2,3. Emblematic instances are fractional quantum Hall (FQH) states4, in which the interplay of a magnetic field and strong interactions gives rise to fractionally charged quasi-particles, long-ranged entanglement and anyonic exchange statistics. Progress in engineering synthetic magnetic fields5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21 has raised the hope to create these exotic states in controlled quantum systems. However, except for a recent Laughlin state of light22, preparing FQH states in engineered systems remains elusive. Here we realize a FQH state with ultracold atoms in an optical lattice. The state is a lattice version of a bosonic ν = 1/2 Laughlin state4,23 with two particles on 16 sites. This minimal system already captures many hallmark features of Laughlin-type FQH states24,25,26,27,28: we observe a suppression of two-body interactions, we find a distinctive vortex structure in the density correlations and we measure a fractional Hall conductivity of σH/σ0 = 0.6(2) by means of the bulk response to a magnetic perturbation. Furthermore, by tuning the magnetic field, we map out the transition point between the normal and the FQH regime through a spectroscopic investigation of the many-body gap. Our work provides a starting point for exploring highly entangled topological matter with ultracold atoms29,30,31,32,33.","lang":"eng"}],"pmid":1,"date_updated":"2024-10-08T11:09:24Z","page":"495-499","type":"journal_article","status":"public","_id":"18189","publisher":"Springer Nature","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","doi":"10.1038/s41586-023-06122-4","publication_status":"published","article_type":"original","author":[{"first_name":"Julian","full_name":"Leonard, Julian","id":"b75b3f45-7995-11ef-9bfd-9a9cd02c3577","last_name":"Leonard"},{"last_name":"Kim","full_name":"Kim, Sooshin","first_name":"Sooshin"},{"last_name":"Kwan","full_name":"Kwan, Joyce","first_name":"Joyce"},{"last_name":"Segura","full_name":"Segura, Perrin","first_name":"Perrin"},{"first_name":"Fabian","full_name":"Grusdt, Fabian","last_name":"Grusdt"},{"full_name":"Repellin, Cécile","first_name":"Cécile","last_name":"Repellin"},{"first_name":"Nathan","full_name":"Goldman, Nathan","last_name":"Goldman"},{"last_name":"Greiner","full_name":"Greiner, Markus","first_name":"Markus"}],"month":"06","oa_version":"Preprint","intvolume":"       619","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2210.10919","open_access":"1"}],"issue":"7970","article_processing_charge":"No","year":"2023","oa":1,"scopus_import":"1","date_created":"2024-10-07T11:46:13Z","publication":"Nature","citation":{"short":"J. Leonard, S. Kim, J. Kwan, P. Segura, F. Grusdt, C. Repellin, N. Goldman, M. Greiner, Nature 619 (2023) 495–499.","ieee":"J. Leonard <i>et al.</i>, “Realization of a fractional quantum Hall state with ultracold atoms,” <i>Nature</i>, vol. 619, no. 7970. Springer Nature, pp. 495–499, 2023.","apa":"Leonard, J., Kim, S., Kwan, J., Segura, P., Grusdt, F., Repellin, C., … Greiner, M. (2023). Realization of a fractional quantum Hall state with ultracold atoms. <i>Nature</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41586-023-06122-4\">https://doi.org/10.1038/s41586-023-06122-4</a>","chicago":"Leonard, Julian, Sooshin Kim, Joyce Kwan, Perrin Segura, Fabian Grusdt, Cécile Repellin, Nathan Goldman, and Markus Greiner. “Realization of a Fractional Quantum Hall State with Ultracold Atoms.” <i>Nature</i>. Springer Nature, 2023. <a href=\"https://doi.org/10.1038/s41586-023-06122-4\">https://doi.org/10.1038/s41586-023-06122-4</a>.","ista":"Leonard J, Kim S, Kwan J, Segura P, Grusdt F, Repellin C, Goldman N, Greiner M. 2023. Realization of a fractional quantum Hall state with ultracold atoms. Nature. 619(7970), 495–499.","ama":"Leonard J, Kim S, Kwan J, et al. Realization of a fractional quantum Hall state with ultracold atoms. <i>Nature</i>. 2023;619(7970):495-499. doi:<a href=\"https://doi.org/10.1038/s41586-023-06122-4\">10.1038/s41586-023-06122-4</a>","mla":"Leonard, Julian, et al. “Realization of a Fractional Quantum Hall State with Ultracold Atoms.” <i>Nature</i>, vol. 619, no. 7970, Springer Nature, 2023, pp. 495–99, doi:<a href=\"https://doi.org/10.1038/s41586-023-06122-4\">10.1038/s41586-023-06122-4</a>."},"extern":"1","publication_identifier":{"eissn":["1476-4687"],"issn":["0028-0836"]},"volume":619,"arxiv":1,"quality_controlled":"1"},{"author":[{"last_name":"Leonard","first_name":"Julian","full_name":"Leonard, Julian","id":"b75b3f45-7995-11ef-9bfd-9a9cd02c3577"},{"full_name":"Kim, Sooshin","first_name":"Sooshin","last_name":"Kim"},{"last_name":"Rispoli","full_name":"Rispoli, Matthew","first_name":"Matthew"},{"first_name":"Alexander","full_name":"Lukin, Alexander","last_name":"Lukin"},{"last_name":"Schittko","first_name":"Robert","full_name":"Schittko, Robert"},{"last_name":"Kwan","full_name":"Kwan, Joyce","first_name":"Joyce"},{"first_name":"Eugene","full_name":"Demler, Eugene","last_name":"Demler"},{"last_name":"Sels","full_name":"Sels, Dries","first_name":"Dries"},{"first_name":"Markus","full_name":"Greiner, Markus","last_name":"Greiner"}],"article_type":"letter_note","publication_status":"published","year":"2023","oa":1,"article_processing_charge":"No","month":"01","oa_version":"Preprint","intvolume":"        19","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2012.15270","open_access":"1"}],"issue":"4","citation":{"ama":"Leonard J, Kim S, Rispoli M, et al. Probing the onset of quantum avalanches in a many-body localized system. <i>Nature Physics</i>. 2023;19(4):481-485. doi:<a href=\"https://doi.org/10.1038/s41567-022-01887-3\">10.1038/s41567-022-01887-3</a>","mla":"Leonard, Julian, et al. “Probing the Onset of Quantum Avalanches in a Many-Body Localized System.” <i>Nature Physics</i>, vol. 19, no. 4, Springer Nature, 2023, pp. 481–85, doi:<a href=\"https://doi.org/10.1038/s41567-022-01887-3\">10.1038/s41567-022-01887-3</a>.","ista":"Leonard J, Kim S, Rispoli M, Lukin A, Schittko R, Kwan J, Demler E, Sels D, Greiner M. 2023. Probing the onset of quantum avalanches in a many-body localized system. Nature Physics. 19(4), 481–485.","chicago":"Leonard, Julian, Sooshin Kim, Matthew Rispoli, Alexander Lukin, Robert Schittko, Joyce Kwan, Eugene Demler, Dries Sels, and Markus Greiner. “Probing the Onset of Quantum Avalanches in a Many-Body Localized System.” <i>Nature Physics</i>. Springer Nature, 2023. <a href=\"https://doi.org/10.1038/s41567-022-01887-3\">https://doi.org/10.1038/s41567-022-01887-3</a>.","short":"J. Leonard, S. Kim, M. Rispoli, A. Lukin, R. Schittko, J. Kwan, E. Demler, D. Sels, M. Greiner, Nature Physics 19 (2023) 481–485.","apa":"Leonard, J., Kim, S., Rispoli, M., Lukin, A., Schittko, R., Kwan, J., … Greiner, M. (2023). Probing the onset of quantum avalanches in a many-body localized system. <i>Nature Physics</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41567-022-01887-3\">https://doi.org/10.1038/s41567-022-01887-3</a>","ieee":"J. Leonard <i>et al.</i>, “Probing the onset of quantum avalanches in a many-body localized system,” <i>Nature Physics</i>, vol. 19, no. 4. Springer Nature, pp. 481–485, 2023."},"extern":"1","date_created":"2024-10-07T11:46:33Z","scopus_import":"1","publication":"Nature Physics","volume":19,"publication_identifier":{"issn":["1745-2473"],"eissn":["1745-2481"]},"arxiv":1,"quality_controlled":"1","external_id":{"arxiv":["2012.15270"]},"language":[{"iso":"eng"}],"fulldoi":"https://doi.org/10.1038/s41567-022-01887-3","day":"26","date_published":"2023-01-26T00:00:00Z","page":"481-485","date_updated":"2024-10-08T10:52:08Z","title":"Probing the onset of quantum avalanches in a many-body localized system","abstract":[{"text":"Strongly correlated systems can exhibit unexpected phenomena when brought in a state far from equilibrium. An example is many-body localization, which prevents generic interacting systems from reaching thermal equilibrium even at long times1,2. The stability of the many-body localized phase has been predicted to be hindered by the presence of small thermal inclusions that act as a bath, leading to the delocalization of the entire system through an avalanche propagation mechanism3,4,5,6,7,8. Here we study the dynamics of a thermal inclusion of variable size when it is coupled to a many-body localized system. We find evidence for accelerated transport of thermal inclusion into the localized region. We monitor how the avalanche spreads through the localized system and thermalizes it site by site by measuring the site-resolved entropy over time. Furthermore, we isolate the strongly correlated bath-induced dynamics with multipoint correlations between the bath and the system. Our results have implications on the robustness of many-body localized systems and their critical behaviour.","lang":"eng"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publisher":"Springer Nature","doi":"10.1038/s41567-022-01887-3","_id":"18190","status":"public","type":"journal_article"},{"publisher":"Springer Nature","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","doi":"10.1038/s41598-023-32821-z","type":"journal_article","status":"public","_id":"18207","pmid":1,"date_updated":"2024-10-09T10:39:26Z","license":"https://creativecommons.org/licenses/by/4.0/","title":"Water stabilizes an alternate turn conformation in horse heart myoglobin","abstract":[{"text":"Comparison of myoglobin structures reveals that protein isolated from horse heart consistently adopts an alternate turn conformation in comparison to its homologues. Analysis of hundreds of high-resolution structures discounts crystallization conditions or the surrounding amino acid protein environment as explaining this difference, that is also not captured by the AlphaFold prediction. Rather, a water molecule is identified as stabilizing the conformation in the horse heart structure, which immediately reverts to the whale conformation in molecular dynamics simulations excluding that structural water.","lang":"eng"}],"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","short":"CC BY (4.0)"},"external_id":{"pmid":["37055458"]},"fulldoi":"https://doi.org/10.1038/s41598-023-32821-z","language":[{"iso":"eng"}],"day":"13","date_published":"2023-04-13T00:00:00Z","article_number":"6094","volume":13,"publication_identifier":{"issn":["2045-2322"]},"quality_controlled":"1","citation":{"ista":"Bronstein AM, Marx A. 2023. Water stabilizes an alternate turn conformation in horse heart myoglobin. Scientific Reports. 13, 6094.","mla":"Bronstein, Alex M., and Ailie Marx. “Water Stabilizes an Alternate Turn Conformation in Horse Heart Myoglobin.” <i>Scientific Reports</i>, vol. 13, 6094, Springer Nature, 2023, doi:<a href=\"https://doi.org/10.1038/s41598-023-32821-z\">10.1038/s41598-023-32821-z</a>.","ama":"Bronstein AM, Marx A. Water stabilizes an alternate turn conformation in horse heart myoglobin. <i>Scientific Reports</i>. 2023;13. doi:<a href=\"https://doi.org/10.1038/s41598-023-32821-z\">10.1038/s41598-023-32821-z</a>","ieee":"A. M. Bronstein and A. Marx, “Water stabilizes an alternate turn conformation in horse heart myoglobin,” <i>Scientific Reports</i>, vol. 13. Springer Nature, 2023.","apa":"Bronstein, A. M., &#38; Marx, A. (2023). Water stabilizes an alternate turn conformation in horse heart myoglobin. <i>Scientific Reports</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41598-023-32821-z\">https://doi.org/10.1038/s41598-023-32821-z</a>","short":"A.M. Bronstein, A. Marx, Scientific Reports 13 (2023).","chicago":"Bronstein, Alex M., and Ailie Marx. “Water Stabilizes an Alternate Turn Conformation in Horse Heart Myoglobin.” <i>Scientific Reports</i>. Springer Nature, 2023. <a href=\"https://doi.org/10.1038/s41598-023-32821-z\">https://doi.org/10.1038/s41598-023-32821-z</a>."},"extern":"1","has_accepted_license":"1","scopus_import":"1","date_created":"2024-10-08T12:46:41Z","publication":"Scientific Reports","article_processing_charge":"No","oa":1,"year":"2023","month":"04","oa_version":"Published Version","intvolume":"        13","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1038/s41598-023-32821-z"}],"article_type":"original","publication_status":"published","author":[{"last_name":"Bronstein","id":"58f3726e-7cba-11ef-ad8b-e6e8cb3904e6","full_name":"Bronstein, Alexander","orcid":"0000-0001-9699-8730","first_name":"Alexander"},{"first_name":"Ailie","full_name":"Marx, Ailie","last_name":"Marx"}]},{"external_id":{"pmid":["38177755"]},"fulldoi":"https://doi.org/10.1038/s43588-023-00532-0","language":[{"iso":"eng"}],"date_published":"2023-10-05T00:00:00Z","day":"05","publisher":"Springer Nature","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","doi":"10.1038/s43588-023-00532-0","type":"journal_article","_id":"18208","status":"public","pmid":1,"date_updated":"2024-10-09T10:44:41Z","page":"873-882","title":"Guided diffusion for inverse molecular design","abstract":[{"lang":"eng","text":"The holy grail of materials science is de novo molecular design, meaning engineering molecules with desired characteristics. The introduction of generative deep learning has greatly advanced efforts in this direction, yet molecular discovery remains challenging and often inefficient. Herein we introduce GaUDI, a guided diffusion model for inverse molecular design that combines an equivariant graph neural net for property prediction and a generative diffusion model. We demonstrate GaUDI’s effectiveness in designing molecules for organic electronic applications by using single- and multiple-objective tasks applied to a generated dataset of 475,000 polycyclic aromatic systems. GaUDI shows improved conditional design, generating molecules with optimal properties and even going beyond the original distribution to suggest better molecules than those in the dataset. In addition to point-wise targets, GaUDI can also be guided toward open-ended targets (for example, a minimum or maximum) and in all cases achieves close to 100% validity of generated molecules."}],"article_processing_charge":"No","oa":1,"year":"2023","month":"10","main_file_link":[{"url":"https://doi.org/10.26434/chemrxiv-2023-z8ltp","open_access":"1"}],"intvolume":"         3","oa_version":"Preprint","issue":"10","publication_status":"published","article_type":"original","author":[{"full_name":"Weiss, Tomer","first_name":"Tomer","last_name":"Weiss"},{"full_name":"Mayo Yanes, Eduardo","first_name":"Eduardo","last_name":"Mayo Yanes"},{"last_name":"Chakraborty","first_name":"Sabyasachi","full_name":"Chakraborty, Sabyasachi"},{"last_name":"Cosmo","full_name":"Cosmo, Luca","first_name":"Luca"},{"last_name":"Bronstein","orcid":"0000-0001-9699-8730","full_name":"Bronstein, Alexander","first_name":"Alexander","id":"58f3726e-7cba-11ef-ad8b-e6e8cb3904e6"},{"first_name":"Renana","full_name":"Gershoni-Poranne, Renana","last_name":"Gershoni-Poranne"}],"volume":3,"publication_identifier":{"issn":["2662-8457"]},"quality_controlled":"1","citation":{"ista":"Weiss T, Mayo Yanes E, Chakraborty S, Cosmo L, Bronstein AM, Gershoni-Poranne R. 2023. Guided diffusion for inverse molecular design. Nature Computational Science. 3(10), 873–882.","ama":"Weiss T, Mayo Yanes E, Chakraborty S, Cosmo L, Bronstein AM, Gershoni-Poranne R. Guided diffusion for inverse molecular design. <i>Nature Computational Science</i>. 2023;3(10):873-882. doi:<a href=\"https://doi.org/10.1038/s43588-023-00532-0\">10.1038/s43588-023-00532-0</a>","mla":"Weiss, Tomer, et al. “Guided Diffusion for Inverse Molecular Design.” <i>Nature Computational Science</i>, vol. 3, no. 10, Springer Nature, 2023, pp. 873–82, doi:<a href=\"https://doi.org/10.1038/s43588-023-00532-0\">10.1038/s43588-023-00532-0</a>.","short":"T. Weiss, E. Mayo Yanes, S. Chakraborty, L. Cosmo, A.M. Bronstein, R. Gershoni-Poranne, Nature Computational Science 3 (2023) 873–882.","apa":"Weiss, T., Mayo Yanes, E., Chakraborty, S., Cosmo, L., Bronstein, A. M., &#38; Gershoni-Poranne, R. (2023). Guided diffusion for inverse molecular design. <i>Nature Computational Science</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s43588-023-00532-0\">https://doi.org/10.1038/s43588-023-00532-0</a>","ieee":"T. Weiss, E. Mayo Yanes, S. Chakraborty, L. Cosmo, A. M. Bronstein, and R. Gershoni-Poranne, “Guided diffusion for inverse molecular design,” <i>Nature Computational Science</i>, vol. 3, no. 10. Springer Nature, pp. 873–882, 2023.","chicago":"Weiss, Tomer, Eduardo Mayo Yanes, Sabyasachi Chakraborty, Luca Cosmo, Alex M. Bronstein, and Renana Gershoni-Poranne. “Guided Diffusion for Inverse Molecular Design.” <i>Nature Computational Science</i>. Springer Nature, 2023. <a href=\"https://doi.org/10.1038/s43588-023-00532-0\">https://doi.org/10.1038/s43588-023-00532-0</a>."},"extern":"1","scopus_import":"1","date_created":"2024-10-08T12:46:58Z","publication":"Nature Computational Science"}]