[{"citation":{"ista":"Krauth LM, Davelaar J, Westernacher-Schneider JR, Haiman Z, Zrake J, MacFadyen A. 2023. Disappearing thermal X-ray emission as a tell-tale signature of merging massive black hole binaries. Monthly Notices of the Royal Astronomical Society. 526(4), 5441–5454.","chicago":"Krauth, Luke Major, Jordy Davelaar, John Ryan Westernacher-Schneider, Zoltán Haiman, Jonathan Zrake, and Andrew MacFadyen. “Disappearing Thermal X-Ray Emission as a Tell-Tale Signature of Merging Massive Black Hole Binaries.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/mnras/stad3095\">https://doi.org/10.1093/mnras/stad3095</a>.","mla":"Krauth, Luke Major, et al. “Disappearing Thermal X-Ray Emission as a Tell-Tale Signature of Merging Massive Black Hole Binaries.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 526, no. 4, Oxford University Press, 2023, pp. 5441–54, doi:<a href=\"https://doi.org/10.1093/mnras/stad3095\">10.1093/mnras/stad3095</a>.","ama":"Krauth LM, Davelaar J, Westernacher-Schneider JR, Haiman Z, Zrake J, MacFadyen A. Disappearing thermal X-ray emission as a tell-tale signature of merging massive black hole binaries. <i>Monthly Notices of the Royal Astronomical Society</i>. 2023;526(4):5441-5454. doi:<a href=\"https://doi.org/10.1093/mnras/stad3095\">10.1093/mnras/stad3095</a>","short":"L.M. Krauth, J. Davelaar, J.R. Westernacher-Schneider, Z. Haiman, J. Zrake, A. MacFadyen, Monthly Notices of the Royal Astronomical Society 526 (2023) 5441–5454.","apa":"Krauth, L. M., Davelaar, J., Westernacher-Schneider, J. R., Haiman, Z., Zrake, J., &#38; MacFadyen, A. (2023). Disappearing thermal X-ray emission as a tell-tale signature of merging massive black hole binaries. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stad3095\">https://doi.org/10.1093/mnras/stad3095</a>","ieee":"L. M. Krauth, J. Davelaar, J. R. Westernacher-Schneider, Z. Haiman, J. Zrake, and A. MacFadyen, “Disappearing thermal X-ray emission as a tell-tale signature of merging massive black hole binaries,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 526, no. 4. Oxford University Press, pp. 5441–5454, 2023."},"day":"13","publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","page":"5441-5454","title":"Disappearing thermal X-ray emission as a tell-tale signature of merging massive black hole binaries","type":"journal_article","oa_version":"Published Version","date_published":"2023-10-13T00:00:00Z","quality_controlled":"1","intvolume":"       526","month":"10","publication_status":"published","date_updated":"2024-09-10T14:43:04Z","_id":"17521","doi":"10.1093/mnras/stad3095","extern":"1","article_processing_charge":"No","status":"public","language":[{"iso":"eng"}],"year":"2023","author":[{"full_name":"Krauth, Luke Major","first_name":"Luke Major","last_name":"Krauth"},{"full_name":"Davelaar, Jordy","first_name":"Jordy","last_name":"Davelaar"},{"full_name":"Westernacher-Schneider, John Ryan","last_name":"Westernacher-Schneider","first_name":"John Ryan"},{"full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán"},{"first_name":"Jonathan","last_name":"Zrake","full_name":"Zrake, Jonathan"},{"full_name":"MacFadyen, Andrew","last_name":"MacFadyen","first_name":"Andrew"}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad3095"}],"abstract":[{"text":"The upcoming Laser Interferometer Space Antenna (LISA) is expected to detect gravitational waves (GWs) from massive black hole binaries (MBHB). Finding the electromagnetic (EM) counterparts for these GW events will be crucial for understanding how and where MBHBs merge, measuring their redshifts, constraining the Hubble constant and the graviton mass, and for other novel science applications. However, due to poor GW sky localization, multiwavelength, time-dependent EM models are needed to identify the right host galaxy. We studied merging MBHBs embedded in a circumbinary disc (CBD) using high-resolution two-dimensional simulations, with a Γ-law equation of state, incorporating viscous heating, shock heating, and radiative cooling. We simulate the binary from large separation until after merger, allowing us to model the decoupling of the binary from the CBD. We compute the EM signatures and identify distinct features before, during, and after the merger. Our main result is a multiband EM signature: we find that the MBHB produces strong thermal X-ray emission until 1–2 d prior to the merger. However, as the binary decouples from the CBD, the X-ray-bright minidiscs rapidly shrink in size, become disrupted, and the accretion rate drops precipitously. As a result, the thermal X-ray luminosity drops by orders of magnitude, and the source remains X-ray dark for several days, regardless of any post-merger effects such as GW recoil or mass-loss. Looking for the abrupt spectral change where the thermal X-ray disappears is a tell-tale EM signature of LISA mergers that does not require extensive pre-merger monitoring.","lang":"eng"}],"issue":"4","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":526,"article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publisher":"Oxford University Press","oa":1,"date_created":"2024-09-05T09:20:27Z"},{"status":"public","language":[{"iso":"eng"}],"year":"2023","author":[{"full_name":"Su, Kung-Yi","last_name":"Su","first_name":"Kung-Yi"},{"full_name":"Bryan, Greg L","last_name":"Bryan","first_name":"Greg L"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán","full_name":"Haiman, Zoltán"},{"first_name":"Rachel S","last_name":"Somerville","full_name":"Somerville, Rachel S"},{"last_name":"Hayward","first_name":"Christopher C","full_name":"Hayward, Christopher C"},{"first_name":"Claude-André","last_name":"Faucher-Giguère","full_name":"Faucher-Giguère, Claude-André"}],"issue":"3","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"}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad252"}],"article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":520,"oa":1,"publisher":"Oxford University Press","date_created":"2024-09-05T09:22:35Z","citation":{"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.","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>","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.","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.","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>","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>.","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>."},"day":"27","publication":"Monthly Notices of the Royal Astronomical Society","page":"4258-4275","title":"Self-regulation of black hole accretion via jets in early protogalaxies","type":"journal_article","scopus_import":"1","oa_version":"Published Version","date_published":"2023-01-27T00:00:00Z","date_updated":"2024-09-11T07:39:21Z","publication_status":"published","_id":"17522","quality_controlled":"1","intvolume":"       520","month":"01","doi":"10.1093/mnras/stad252","article_processing_charge":"No","extern":"1"},{"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","volume":526,"publication_identifier":{"issn":["0035-8711","1365-2966"]},"issue":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad2616"}],"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"}],"date_created":"2024-09-05T09:30:18Z","publisher":"Oxford University Press","oa":1,"status":"public","author":[{"full_name":"Tagawa, Hiromichi","first_name":"Hiromichi","last_name":"Tagawa"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}],"year":"2023","language":[{"iso":"eng"}],"_id":"17527","publication_status":"published","date_updated":"2024-09-11T08:52:17Z","month":"09","intvolume":"       526","quality_controlled":"1","date_published":"2023-09-05T00:00:00Z","article_processing_charge":"No","extern":"1","doi":"10.1093/mnras/stad2616","publication":"Monthly Notices of the Royal Astronomical Society","day":"05","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>.","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>.","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.","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>","short":"H. Tagawa, Z. Haiman, Monthly Notices of the Royal Astronomical Society 526 (2023) 69–79."},"oa_version":"Published Version","title":"Flares from stars crossing active galactic nucleus discs on low-inclination orbits","type":"journal_article","page":"69-79","scopus_import":"1"},{"oa_version":"Published Version","scopus_import":"1","title":"Gas dynamical friction as a binary formation mechanism in AGN discs","type":"journal_article","page":"1126-1139","publication":"Monthly Notices of the Royal Astronomical Society","day":"10","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>.","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>","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>.","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.","short":"S. DeLaurentiis, M. Epstein-Martin, Z. Haiman, Monthly Notices of the Royal Astronomical Society 523 (2023) 1126–1139.","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>","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."},"extern":"1","article_processing_charge":"No","doi":"10.1093/mnras/stad1412","month":"05","intvolume":"       523","quality_controlled":"1","_id":"17539","date_updated":"2024-09-12T09:46:18Z","publication_status":"published","date_published":"2023-05-10T00:00:00Z","author":[{"first_name":"Stanislav","last_name":"DeLaurentiis","full_name":"DeLaurentiis, Stanislav"},{"full_name":"Epstein-Martin, Marguerite","last_name":"Epstein-Martin","first_name":"Marguerite"},{"full_name":"Haiman, Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán"}],"year":"2023","language":[{"iso":"eng"}],"status":"public","date_created":"2024-09-05T09:53:03Z","oa":1,"publisher":"Oxford University Press","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":523,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stad1412","open_access":"1"}],"abstract":[{"lang":"eng","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."}],"issue":"1"},{"oa_version":"Published Version","scopus_import":"1","page":"1569-1574","type":"journal_article","title":"The importance of live binary evolution in numerical simulations of binaries embedded in circumbinary discs","publication":"Monthly Notices of the Royal Astronomical Society","day":"12","citation":{"short":"A. Franchini, A. Lupi, A. Sesana, Z. Haiman, Monthly Notices of the Royal Astronomical Society 522 (2023) 1569–1574.","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>","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.","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>.","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."},"extern":"1","article_processing_charge":"No","doi":"10.1093/mnras/stad1070","quality_controlled":"1","month":"04","intvolume":"       522","date_updated":"2024-09-18T09:30:21Z","publication_status":"published","_id":"17548","date_published":"2023-04-12T00:00:00Z","year":"2023","language":[{"iso":"eng"}],"author":[{"first_name":"Alessia","last_name":"Franchini","full_name":"Franchini, Alessia"},{"full_name":"Lupi, Alessandro","first_name":"Alessandro","last_name":"Lupi"},{"last_name":"Sesana","first_name":"Alberto","full_name":"Sesana, Alberto"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}],"status":"public","publisher":"Oxford University Press","oa":1,"date_created":"2024-09-05T10:08:46Z","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":522,"article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad1070"}],"abstract":[{"lang":"eng","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."}],"issue":"1"},{"date_created":"2024-09-05T10:11:02Z","oa":1,"publisher":"American Astronomical Society","volume":951,"publication_identifier":{"issn":["2041-8205","2041-8213"]},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/2041-8213/acc9c8"}],"abstract":[{"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.","lang":"eng"}],"issue":"1","author":[{"full_name":"Yang, Jinyi","last_name":"Yang","first_name":"Jinyi"},{"full_name":"Wang, Feige","last_name":"Wang","first_name":"Feige"},{"first_name":"Xiaohui","last_name":"Fan","full_name":"Fan, Xiaohui"},{"last_name":"Hennawi","first_name":"Joseph F.","full_name":"Hennawi, Joseph F."},{"last_name":"Barth","first_name":"Aaron J.","full_name":"Barth, Aaron J."},{"first_name":"Eduardo","last_name":"Bañados","full_name":"Bañados, Eduardo"},{"full_name":"Sun, Fengwu","first_name":"Fengwu","last_name":"Sun"},{"last_name":"Liu","first_name":"Weizhe","full_name":"Liu, Weizhe"},{"first_name":"Zheng","last_name":"Cai","full_name":"Cai, Zheng"},{"full_name":"Jiang, Linhua","last_name":"Jiang","first_name":"Linhua"},{"first_name":"Zihao","last_name":"Li","full_name":"Li, Zihao"},{"first_name":"Masafusa","last_name":"Onoue","full_name":"Onoue, Masafusa"},{"last_name":"Schindler","first_name":"Jan-Torge","full_name":"Schindler, Jan-Torge"},{"last_name":"Shen","first_name":"Yue","full_name":"Shen, Yue"},{"last_name":"Wu","first_name":"Yunjing","full_name":"Wu, Yunjing"},{"full_name":"Bhowmick, Aklant K.","first_name":"Aklant K.","last_name":"Bhowmick"},{"full_name":"Bieri, Rebekka","last_name":"Bieri","first_name":"Rebekka"},{"first_name":"Laura","last_name":"Blecha","full_name":"Blecha, Laura"},{"last_name":"Bosman","first_name":"Sarah","full_name":"Bosman, Sarah"},{"last_name":"Champagne","first_name":"Jaclyn B.","full_name":"Champagne, Jaclyn B."},{"full_name":"Colina, Luis","last_name":"Colina","first_name":"Luis"},{"first_name":"Thomas","last_name":"Connor","full_name":"Connor, Thomas"},{"first_name":"Tiago","last_name":"Costa","full_name":"Costa, Tiago"},{"full_name":"Davies, Frederick B.","first_name":"Frederick B.","last_name":"Davies"},{"full_name":"Decarli, Roberto","first_name":"Roberto","last_name":"Decarli"},{"first_name":"Gisella","last_name":"De Rosa","full_name":"De Rosa, Gisella"},{"last_name":"Drake","first_name":"Alyssa B.","full_name":"Drake, Alyssa B."},{"last_name":"Egami","first_name":"Eiichi","full_name":"Egami, Eiichi"},{"full_name":"Eilers, Anna-Christina","first_name":"Anna-Christina","last_name":"Eilers"},{"last_name":"Evans","first_name":"Analis E.","full_name":"Evans, Analis E."},{"first_name":"Emanuele Paolo","last_name":"Farina","full_name":"Farina, Emanuele Paolo"},{"first_name":"Melanie","last_name":"Habouzit","full_name":"Habouzit, Melanie"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"last_name":"Jin","first_name":"Xiangyu","full_name":"Jin, Xiangyu"},{"full_name":"Jun, Hyunsung D.","last_name":"Jun","first_name":"Hyunsung D."},{"last_name":"Kakiichi","first_name":"Koki","full_name":"Kakiichi, Koki"},{"full_name":"Khusanova, Yana","first_name":"Yana","last_name":"Khusanova"},{"first_name":"Girish","last_name":"Kulkarni","full_name":"Kulkarni, Girish"},{"last_name":"Loiacono","first_name":"Federica","full_name":"Loiacono, Federica"},{"last_name":"Lupi","first_name":"Alessandro","full_name":"Lupi, Alessandro"},{"first_name":"Chiara","last_name":"Mazzucchelli","full_name":"Mazzucchelli, Chiara"},{"full_name":"Pan, Zhiwei","last_name":"Pan","first_name":"Zhiwei"},{"first_name":"Sofía","last_name":"Rojas-Ruiz","full_name":"Rojas-Ruiz, Sofía"},{"first_name":"Michael A.","last_name":"Strauss","full_name":"Strauss, Michael A."},{"first_name":"Wei Leong","last_name":"Tee","full_name":"Tee, Wei Leong"},{"full_name":"Trakhtenbrot, Benny","first_name":"Benny","last_name":"Trakhtenbrot"},{"last_name":"Trebitsch","first_name":"Maxime","full_name":"Trebitsch, Maxime"},{"first_name":"Bram","last_name":"Venemans","full_name":"Venemans, Bram"},{"first_name":"Marianne","last_name":"Vestergaard","full_name":"Vestergaard, Marianne"},{"full_name":"Volonteri, Marta","last_name":"Volonteri","first_name":"Marta"},{"full_name":"Walter, Fabian","last_name":"Walter","first_name":"Fabian"},{"last_name":"Xie","first_name":"Zhang-Liang","full_name":"Xie, Zhang-Liang"},{"full_name":"Yue, Minghao","last_name":"Yue","first_name":"Minghao"},{"first_name":"Haowen","last_name":"Zhang","full_name":"Zhang, Haowen"},{"last_name":"Zhang","first_name":"Huanian","full_name":"Zhang, Huanian"},{"full_name":"Zou, Siwei","first_name":"Siwei","last_name":"Zou"}],"language":[{"iso":"eng"}],"year":"2023","status":"public","extern":"1","article_processing_charge":"No","doi":"10.3847/2041-8213/acc9c8","article_number":"L5","intvolume":"       951","month":"06","quality_controlled":"1","_id":"17549","publication_status":"published","date_updated":"2024-09-18T09:53:12Z","date_published":"2023-06-29T00:00:00Z","oa_version":"Published Version","scopus_import":"1","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","type":"journal_article","publication":"The Astrophysical Journal Letters","day":"29","citation":{"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>","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).","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>","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>.","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."}},{"status":"public","author":[{"full_name":"Lu, Tianhuan","first_name":"Tianhuan","last_name":"Lu"},{"first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán"},{"full_name":"Li, Xiangchong","last_name":"Li","first_name":"Xiangchong"}],"language":[{"iso":"eng"}],"year":"2023","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad686"}],"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"}],"issue":"2","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":521,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","date_created":"2024-09-05T10:14:34Z","oa":1,"publisher":"Oxford University Press","citation":{"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>","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.","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>.","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>","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>."},"day":"06","publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","type":"journal_article","title":"Cosmological constraints from HSC survey first-year data using deep learning","page":"2050-2066","oa_version":"Published Version","date_published":"2023-03-06T00:00:00Z","month":"03","intvolume":"       521","quality_controlled":"1","_id":"17551","date_updated":"2024-09-18T10:09:01Z","publication_status":"published","doi":"10.1093/mnras/stad686","extern":"1","article_processing_charge":"No"},{"publisher":"Oxford University Press (OUP)","oa":1,"date_created":"2024-09-05T10:32:08Z","issue":"4","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stad3641","open_access":"1"}],"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"}],"article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","volume":527,"publication_identifier":{"issn":["0035-8711","1365-2966"]},"year":"2023","language":[{"iso":"eng"}],"author":[{"full_name":"Rowan, Connar","first_name":"Connar","last_name":"Rowan"},{"full_name":"Whitehead, Henry","last_name":"Whitehead","first_name":"Henry"},{"first_name":"Tjarda","last_name":"Boekholt","full_name":"Boekholt, Tjarda"},{"first_name":"Bence","last_name":"Kocsis","full_name":"Kocsis, Bence"},{"first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán"}],"status":"public","doi":"10.1093/mnras/stad3641","article_processing_charge":"No","extern":"1","date_published":"2023-01-01T00:00:00Z","date_updated":"2024-09-18T12:11:28Z","publication_status":"published","_id":"17557","quality_controlled":"1","intvolume":"       527","month":"01","page":"10448-10468","title":"Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings","type":"journal_article","scopus_import":"1","oa_version":"Published Version","citation":{"short":"C. Rowan, H. Whitehead, T. Boekholt, B. Kocsis, Z. Haiman, Monthly Notices of the Royal Astronomical Society 527 (2023) 10448–10468.","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.","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.","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>.","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>.","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>"},"publication":"Monthly Notices of the Royal Astronomical Society"},{"status":"public","author":[{"first_name":"Xuheng","last_name":"Ding","full_name":"Ding, Xuheng"},{"last_name":"Onoue","first_name":"Masafusa","full_name":"Onoue, Masafusa"},{"full_name":"Silverman, John D.","last_name":"Silverman","first_name":"John D."},{"last_name":"Matsuoka","first_name":"Yoshiki","full_name":"Matsuoka, Yoshiki"},{"full_name":"Izumi, Takuma","first_name":"Takuma","last_name":"Izumi"},{"first_name":"Michael A.","last_name":"Strauss","full_name":"Strauss, Michael A."},{"full_name":"Jahnke, Knud","first_name":"Knud","last_name":"Jahnke"},{"last_name":"Phillips","first_name":"Camryn L.","full_name":"Phillips, Camryn L."},{"full_name":"Li, Junyao","first_name":"Junyao","last_name":"Li"},{"first_name":"Marta","last_name":"Volonteri","full_name":"Volonteri, Marta"},{"first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","full_name":"Haiman, Zoltán"},{"full_name":"Andika, Irham Taufik","last_name":"Andika","first_name":"Irham Taufik"},{"full_name":"Aoki, Kentaro","first_name":"Kentaro","last_name":"Aoki"},{"first_name":"Shunsuke","last_name":"Baba","full_name":"Baba, Shunsuke"},{"last_name":"Bieri","first_name":"Rebekka","full_name":"Bieri, Rebekka"},{"last_name":"Bosman","first_name":"Sarah E. I.","full_name":"Bosman, Sarah E. I."},{"full_name":"Bottrell, Connor","first_name":"Connor","last_name":"Bottrell"},{"last_name":"Eilers","first_name":"Anna-Christina","full_name":"Eilers, Anna-Christina"},{"full_name":"Fujimoto, Seiji","first_name":"Seiji","last_name":"Fujimoto"},{"full_name":"Habouzit, Melanie","first_name":"Melanie","last_name":"Habouzit"},{"full_name":"Imanishi, Masatoshi","last_name":"Imanishi","first_name":"Masatoshi"},{"full_name":"Inayoshi, Kohei","last_name":"Inayoshi","first_name":"Kohei"},{"first_name":"Kazushi","last_name":"Iwasawa","full_name":"Iwasawa, Kazushi"},{"last_name":"Kashikawa","first_name":"Nobunari","full_name":"Kashikawa, Nobunari"},{"first_name":"Toshihiro","last_name":"Kawaguchi","full_name":"Kawaguchi, Toshihiro"},{"full_name":"Kohno, Kotaro","first_name":"Kotaro","last_name":"Kohno"},{"first_name":"Chien-Hsiu","last_name":"Lee","full_name":"Lee, Chien-Hsiu"},{"last_name":"Lupi","first_name":"Alessandro","full_name":"Lupi, Alessandro"},{"full_name":"Lyu, Jianwei","last_name":"Lyu","first_name":"Jianwei"},{"full_name":"Nagao, Tohru","last_name":"Nagao","first_name":"Tohru"},{"full_name":"Overzier, Roderik","last_name":"Overzier","first_name":"Roderik"},{"full_name":"Schindler, Jan-Torge","first_name":"Jan-Torge","last_name":"Schindler"},{"first_name":"Malte","last_name":"Schramm","full_name":"Schramm, Malte"},{"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"},{"full_name":"Treu, Tommaso","first_name":"Tommaso","last_name":"Treu"},{"full_name":"Umehata, Hideki","first_name":"Hideki","last_name":"Umehata"},{"full_name":"Venemans, Bram P.","last_name":"Venemans","first_name":"Bram P."},{"last_name":"Vestergaard","first_name":"Marianne","full_name":"Vestergaard, Marianne"},{"full_name":"Walter, Fabian","last_name":"Walter","first_name":"Fabian"},{"first_name":"Feige","last_name":"Wang","full_name":"Wang, Feige"},{"full_name":"Yang, Jinyi","first_name":"Jinyi","last_name":"Yang"}],"year":"2023","language":[{"iso":"eng"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","publication_identifier":{"issn":["0028-0836","1476-4687"]},"volume":621,"arxiv":1,"issue":"7977","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."}],"main_file_link":[{"url":" https://doi.org/10.48550/arXiv.2211.14329","open_access":"1"}],"date_created":"2024-09-05T11:28:21Z","oa":1,"publisher":"Springer Science and Business Media LLC","day":"28","publication":"Nature","external_id":{"arxiv":["2211.14329"]},"citation":{"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.","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>","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.","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>","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>."},"oa_version":"Preprint","title":"Detection of stellar light from quasar host galaxies at redshifts above 6","type":"journal_article","page":"51-55","scopus_import":"1","_id":"17558","publication_status":"published","date_updated":"2024-09-18T12:19:50Z","month":"06","intvolume":"       621","quality_controlled":"1","date_published":"2023-06-28T00:00:00Z","article_processing_charge":"No","extern":"1","doi":"10.1038/s41586-023-06345-5"},{"date_created":"2024-09-05T12:16:33Z","publisher":"Springer Science and Business Media LLC","oa":1,"issue":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1007/s41114-022-00041-y"}],"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"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","volume":26,"publication_identifier":{"issn":["1433-8351"]},"author":[{"full_name":"Amaro-Seoane, Pau","first_name":"Pau","last_name":"Amaro-Seoane"},{"full_name":"Andrews, Jeff","last_name":"Andrews","first_name":"Jeff"},{"full_name":"Arca Sedda, Manuel","first_name":"Manuel","last_name":"Arca Sedda"},{"last_name":"Askar","first_name":"Abbas","full_name":"Askar, Abbas"},{"full_name":"Baghi, Quentin","last_name":"Baghi","first_name":"Quentin"},{"last_name":"Balasov","first_name":"Razvan","full_name":"Balasov, Razvan"},{"full_name":"Bartos, Imre","first_name":"Imre","last_name":"Bartos"},{"first_name":"Simone S.","last_name":"Bavera","full_name":"Bavera, Simone S."},{"full_name":"Bellovary, Jillian","last_name":"Bellovary","first_name":"Jillian"},{"first_name":"Christopher P. L.","last_name":"Berry","full_name":"Berry, Christopher P. L."},{"full_name":"Berti, Emanuele","last_name":"Berti","first_name":"Emanuele"},{"first_name":"Stefano","last_name":"Bianchi","full_name":"Bianchi, Stefano"},{"full_name":"Blecha, Laura","first_name":"Laura","last_name":"Blecha"},{"last_name":"Blondin","first_name":"Stéphane","full_name":"Blondin, Stéphane"},{"full_name":"Bogdanović, Tamara","first_name":"Tamara","last_name":"Bogdanović"},{"full_name":"Boissier, Samuel","last_name":"Boissier","first_name":"Samuel"},{"full_name":"Bonetti, Matteo","last_name":"Bonetti","first_name":"Matteo"},{"full_name":"Bonoli, Silvia","last_name":"Bonoli","first_name":"Silvia"},{"first_name":"Elisa","last_name":"Bortolas","full_name":"Bortolas, Elisa"},{"last_name":"Breivik","first_name":"Katelyn","full_name":"Breivik, Katelyn"},{"first_name":"Pedro R.","last_name":"Capelo","full_name":"Capelo, Pedro R."},{"full_name":"Caramete, Laurentiu","last_name":"Caramete","first_name":"Laurentiu"},{"full_name":"Cattorini, Federico","last_name":"Cattorini","first_name":"Federico"},{"first_name":"Maria","last_name":"Charisi","full_name":"Charisi, Maria"},{"full_name":"Chaty, Sylvain","last_name":"Chaty","first_name":"Sylvain"},{"full_name":"Chen, Xian","last_name":"Chen","first_name":"Xian"},{"full_name":"Chruślińska, Martyna","first_name":"Martyna","last_name":"Chruślińska"},{"full_name":"Chua, Alvin J. K.","first_name":"Alvin J. 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Coleman","last_name":"Miller","full_name":"Miller, M. 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K.","last_name":"Röpke","first_name":"Friedrich K."},{"last_name":"Regan","first_name":"John","full_name":"Regan, John"},{"full_name":"Rosswog, Stephan","last_name":"Rosswog","first_name":"Stephan"},{"first_name":"Ashley","last_name":"Ruiter","full_name":"Ruiter, Ashley"},{"first_name":"Milton","last_name":"Ruiz","full_name":"Ruiz, Milton"},{"last_name":"Runnoe","first_name":"Jessie","full_name":"Runnoe, Jessie"},{"full_name":"Schneider, Raffaella","last_name":"Schneider","first_name":"Raffaella"},{"last_name":"Schnittman","first_name":"Jeremy","full_name":"Schnittman, Jeremy"},{"last_name":"Secunda","first_name":"Amy","full_name":"Secunda, Amy"},{"last_name":"Sesana","first_name":"Alberto","full_name":"Sesana, Alberto"},{"first_name":"Naoki","last_name":"Seto","full_name":"Seto, Naoki"},{"last_name":"Shao","first_name":"Lijing","full_name":"Shao, Lijing"},{"last_name":"Shapiro","first_name":"Stuart","full_name":"Shapiro, Stuart"},{"full_name":"Sopuerta, Carlos","first_name":"Carlos","last_name":"Sopuerta"},{"last_name":"Stone","first_name":"Nicholas C.","full_name":"Stone, Nicholas C."},{"full_name":"Suvorov, Arthur","last_name":"Suvorov","first_name":"Arthur"},{"first_name":"Nicola","last_name":"Tamanini","full_name":"Tamanini, Nicola"},{"full_name":"Tamfal, Tomas","first_name":"Tomas","last_name":"Tamfal"},{"full_name":"Tauris, Thomas","first_name":"Thomas","last_name":"Tauris"},{"last_name":"Temmink","first_name":"Karel","full_name":"Temmink, Karel"},{"full_name":"Tomsick, John","first_name":"John","last_name":"Tomsick"},{"first_name":"Silvia","last_name":"Toonen","full_name":"Toonen, Silvia"},{"full_name":"Torres-Orjuela, Alejandro","last_name":"Torres-Orjuela","first_name":"Alejandro"},{"last_name":"Toscani","first_name":"Martina","full_name":"Toscani, Martina"},{"full_name":"Tsokaros, Antonios","first_name":"Antonios","last_name":"Tsokaros"},{"full_name":"Unal, Caner","last_name":"Unal","first_name":"Caner"},{"full_name":"Vázquez-Aceves, Verónica","first_name":"Verónica","last_name":"Vázquez-Aceves"},{"full_name":"Valiante, Rosa","first_name":"Rosa","last_name":"Valiante"},{"first_name":"Maurice","last_name":"van Putten","full_name":"van Putten, Maurice"},{"full_name":"van Roestel, Jan","first_name":"Jan","last_name":"van Roestel"},{"full_name":"Vignali, Christian","last_name":"Vignali","first_name":"Christian"},{"last_name":"Volonteri","first_name":"Marta","full_name":"Volonteri, Marta"},{"full_name":"Wu, Kinwah","first_name":"Kinwah","last_name":"Wu"},{"full_name":"Younsi, Ziri","last_name":"Younsi","first_name":"Ziri"},{"first_name":"Shenghua","last_name":"Yu","full_name":"Yu, Shenghua"},{"full_name":"Zane, Silvia","last_name":"Zane","first_name":"Silvia"},{"full_name":"Zwick, Lorenz","first_name":"Lorenz","last_name":"Zwick"},{"last_name":"Antonini","first_name":"Fabio","full_name":"Antonini, Fabio"},{"full_name":"Baibhav, Vishal","first_name":"Vishal","last_name":"Baibhav"},{"full_name":"Barausse, Enrico","first_name":"Enrico","last_name":"Barausse"},{"full_name":"Bonilla Rivera, Alexander","first_name":"Alexander","last_name":"Bonilla Rivera"},{"last_name":"Branchesi","first_name":"Marica","full_name":"Branchesi, Marica"},{"full_name":"Branduardi-Raymont, Graziella","first_name":"Graziella","last_name":"Branduardi-Raymont"},{"full_name":"Burdge, Kevin","first_name":"Kevin","last_name":"Burdge"},{"full_name":"Chakraborty, Srija","first_name":"Srija","last_name":"Chakraborty"},{"last_name":"Cuadra","first_name":"Jorge","full_name":"Cuadra, Jorge"},{"full_name":"Dage, Kristen","first_name":"Kristen","last_name":"Dage"},{"full_name":"Davis, Benjamin","first_name":"Benjamin","last_name":"Davis"},{"full_name":"de Mink, Selma E.","first_name":"Selma E.","last_name":"de Mink"},{"full_name":"Decarli, Roberto","first_name":"Roberto","last_name":"Decarli"},{"last_name":"Doneva","first_name":"Daniela","full_name":"Doneva, Daniela"},{"first_name":"Stephanie","last_name":"Escoffier","full_name":"Escoffier, Stephanie"},{"last_name":"Gandhi","first_name":"Poshak","full_name":"Gandhi, Poshak"},{"last_name":"Haardt","first_name":"Francesco","full_name":"Haardt, Francesco"},{"full_name":"Lousto, Carlos O.","last_name":"Lousto","first_name":"Carlos O."},{"full_name":"Nissanke, Samaya","last_name":"Nissanke","first_name":"Samaya"},{"full_name":"Nordhaus, Jason","last_name":"Nordhaus","first_name":"Jason"},{"last_name":"O’Shaughnessy","first_name":"Richard","full_name":"O’Shaughnessy, Richard"},{"full_name":"Portegies Zwart, Simon","first_name":"Simon","last_name":"Portegies Zwart"},{"full_name":"Pound, Adam","last_name":"Pound","first_name":"Adam"},{"first_name":"Fabian","last_name":"Schussler","full_name":"Schussler, Fabian"},{"full_name":"Sergijenko, Olga","first_name":"Olga","last_name":"Sergijenko"},{"first_name":"Alessandro","last_name":"Spallicci","full_name":"Spallicci, Alessandro"},{"full_name":"Vernieri, Daniele","first_name":"Daniele","last_name":"Vernieri"},{"full_name":"Vigna-Gómez, Alejandro","last_name":"Vigna-Gómez","first_name":"Alejandro"}],"language":[{"iso":"eng"}],"year":"2023","status":"public","doi":"10.1007/s41114-022-00041-y","article_number":"2","article_processing_charge":"No","extern":"1","date_published":"2023-03-14T00:00:00Z","_id":"17573","date_updated":"2024-09-19T07:31:45Z","publication_status":"published","intvolume":"        26","month":"03","quality_controlled":"1","title":"Astrophysics with the laser interferometer space antenna","type":"journal_article","scopus_import":"1","oa_version":"Published Version","citation":{"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).","ista":"Amaro-Seoane P et al. 2023. Astrophysics with the laser interferometer space antenna. Living Reviews in Relativity. 26(1), 2.","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>.","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>","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>."},"day":"14","publication":"Living Reviews in Relativity"},{"title":"High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei","type":"journal_article","scopus_import":"1","oa_version":"Published Version","citation":{"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.","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>","short":"H. Tagawa, S.S. Kimura, Z. Haiman, The Astrophysical Journal 955 (2023).","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>","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."},"publication":"The Astrophysical Journal","day":"12","article_number":"23","doi":"10.3847/1538-4357/ace71d","article_processing_charge":"No","extern":"1","date_published":"2023-09-12T00:00:00Z","date_updated":"2024-09-19T11:45:10Z","publication_status":"published","_id":"17584","quality_controlled":"1","month":"09","intvolume":"       955","language":[{"iso":"eng"}],"year":"2023","author":[{"last_name":"Tagawa","first_name":"Hiromichi","full_name":"Tagawa, Hiromichi"},{"full_name":"Kimura, Shigeo S.","last_name":"Kimura","first_name":"Shigeo S."},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán","full_name":"Haiman, Zoltán"}],"status":"public","publisher":"American Astronomical Society","oa":1,"date_created":"2024-09-05T12:28:06Z","issue":"1","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"}],"main_file_link":[{"url":"https://doi.org/10.3847/1538-4357/ace71d","open_access":"1"}],"article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","volume":955,"publication_identifier":{"issn":["0004-637X","1538-4357"]}},{"article_number":"13","doi":"10.3847/1538-4357/acc4bb","article_processing_charge":"No","extern":"1","date_published":"2023-06-06T00:00:00Z","publication_status":"published","date_updated":"2024-09-23T12:36:58Z","_id":"17594","quality_controlled":"1","intvolume":"       950","month":"06","title":"Observable signature of merging stellar-mass black holes in active galactic nuclei","type":"journal_article","scopus_import":"1","oa_version":"Published Version","citation":{"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.","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>.","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>.","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>","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."},"day":"06","publication":"The Astrophysical Journal","oa":1,"publisher":"American Astronomical Society","date_created":"2024-09-05T12:41:47Z","issue":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/acc4bb"}],"abstract":[{"lang":"eng","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."}],"article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication_identifier":{"issn":["0004-637X","1538-4357"]},"volume":950,"language":[{"iso":"eng"}],"year":"2023","author":[{"full_name":"Tagawa, Hiromichi","first_name":"Hiromichi","last_name":"Tagawa"},{"first_name":"Shigeo S.","last_name":"Kimura","full_name":"Kimura, Shigeo S."},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"},{"last_name":"Perna","first_name":"Rosalba","full_name":"Perna, Rosalba"},{"full_name":"Bartos, Imre","last_name":"Bartos","first_name":"Imre"}],"status":"public"},{"article_processing_charge":"No","extern":"1","doi":"10.1093/mnras/stad1926","date_updated":"2024-09-23T13:42:19Z","publication_status":"published","_id":"17602","quality_controlled":"1","intvolume":"       524","month":"07","date_published":"2023-07-03T00:00:00Z","oa_version":"Published Version","page":"2770-2796","type":"journal_article","title":"Black hole binary formation in AGN discs: from isolation to merger","scopus_import":"1","day":"03","publication":"Monthly Notices of the Royal Astronomical Society","citation":{"short":"C. Rowan, T. Boekholt, B. Kocsis, Z. Haiman, Monthly Notices of the Royal Astronomical Society 524 (2023) 2770–2796.","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>","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.","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>.","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."},"publisher":"Oxford University Press","oa":1,"date_created":"2024-09-05T13:09:11Z","article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication_identifier":{"issn":["0035-8711","1365-2966"]},"volume":524,"issue":"2","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."}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stad1926"}],"language":[{"iso":"eng"}],"year":"2023","author":[{"first_name":"Connar","last_name":"Rowan","full_name":"Rowan, Connar"},{"full_name":"Boekholt, Tjarda","last_name":"Boekholt","first_name":"Tjarda"},{"full_name":"Kocsis, Bence","last_name":"Kocsis","first_name":"Bence"},{"first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán"}],"status":"public"},{"date_created":"2024-09-05T13:14:46Z","publisher":"American Astronomical Society","oa":1,"issue":"1","abstract":[{"lang":"eng","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."}],"main_file_link":[{"url":"https://doi.org/10.3847/2041-8213/accd6f","open_access":"1"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","volume":951,"publication_identifier":{"issn":["2041-8205","2041-8213"]},"author":[{"last_name":"Wang","first_name":"Feige","full_name":"Wang, Feige"},{"full_name":"Yang, Jinyi","last_name":"Yang","first_name":"Jinyi"},{"full_name":"Hennawi, Joseph F.","last_name":"Hennawi","first_name":"Joseph F."},{"full_name":"Fan, Xiaohui","first_name":"Xiaohui","last_name":"Fan"},{"full_name":"Sun, Fengwu","first_name":"Fengwu","last_name":"Sun"},{"full_name":"Champagne, Jaclyn B.","last_name":"Champagne","first_name":"Jaclyn B."},{"full_name":"Costa, Tiago","first_name":"Tiago","last_name":"Costa"},{"first_name":"Melanie","last_name":"Habouzit","full_name":"Habouzit, Melanie"},{"full_name":"Endsley, Ryan","first_name":"Ryan","last_name":"Endsley"},{"full_name":"Li, Zihao","last_name":"Li","first_name":"Zihao"},{"last_name":"Lin","first_name":"Xiaojing","full_name":"Lin, Xiaojing"},{"first_name":"Romain A.","last_name":"Meyer","full_name":"Meyer, Romain A."},{"last_name":"Schindler","first_name":"Jan–Torge","full_name":"Schindler, Jan–Torge"},{"full_name":"Wu, Yunjing","last_name":"Wu","first_name":"Yunjing"},{"full_name":"Bañados, Eduardo","last_name":"Bañados","first_name":"Eduardo"},{"first_name":"Aaron J.","last_name":"Barth","full_name":"Barth, Aaron J."},{"first_name":"Aklant K.","last_name":"Bhowmick","full_name":"Bhowmick, Aklant K."},{"full_name":"Bieri, Rebekka","first_name":"Rebekka","last_name":"Bieri"},{"first_name":"Laura","last_name":"Blecha","full_name":"Blecha, Laura"},{"last_name":"Bosman","first_name":"Sarah","full_name":"Bosman, Sarah"},{"first_name":"Zheng","last_name":"Cai","full_name":"Cai, Zheng"},{"first_name":"Luis","last_name":"Colina","full_name":"Colina, Luis"},{"last_name":"Connor","first_name":"Thomas","full_name":"Connor, Thomas"},{"full_name":"Davies, Frederick B.","first_name":"Frederick B.","last_name":"Davies"},{"last_name":"Decarli","first_name":"Roberto","full_name":"Decarli, Roberto"},{"full_name":"De Rosa, Gisella","first_name":"Gisella","last_name":"De Rosa"},{"last_name":"Drake","first_name":"Alyssa B.","full_name":"Drake, Alyssa B."},{"full_name":"Egami, Eiichi","first_name":"Eiichi","last_name":"Egami"},{"last_name":"Eilers","first_name":"Anna-Christina","full_name":"Eilers, Anna-Christina"},{"full_name":"Evans, Analis E.","last_name":"Evans","first_name":"Analis E."},{"full_name":"Farina, Emanuele Paolo","last_name":"Farina","first_name":"Emanuele Paolo"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"},{"last_name":"Jiang","first_name":"Linhua","full_name":"Jiang, Linhua"},{"last_name":"Jin","first_name":"Xiangyu","full_name":"Jin, Xiangyu"},{"last_name":"Jun","first_name":"Hyunsung D.","full_name":"Jun, Hyunsung D."},{"last_name":"Kakiichi","first_name":"Koki","full_name":"Kakiichi, Koki"},{"last_name":"Khusanova","first_name":"Yana","full_name":"Khusanova, Yana"},{"last_name":"Kulkarni","first_name":"Girish","full_name":"Kulkarni, Girish"},{"full_name":"Li, Mingyu","first_name":"Mingyu","last_name":"Li"},{"last_name":"Liu","first_name":"Weizhe","full_name":"Liu, Weizhe"},{"full_name":"Loiacono, Federica","first_name":"Federica","last_name":"Loiacono"},{"full_name":"Lupi, Alessandro","first_name":"Alessandro","last_name":"Lupi"},{"first_name":"Chiara","last_name":"Mazzucchelli","full_name":"Mazzucchelli, Chiara"},{"full_name":"Onoue, Masafusa","last_name":"Onoue","first_name":"Masafusa"},{"first_name":"Maria A.","last_name":"Pudoka","full_name":"Pudoka, Maria A."},{"full_name":"Rojas-Ruiz, Sofía","last_name":"Rojas-Ruiz","first_name":"Sofía"},{"full_name":"Shen, Yue","last_name":"Shen","first_name":"Yue"},{"last_name":"Strauss","first_name":"Michael A.","full_name":"Strauss, Michael A."},{"first_name":"Wei Leong","last_name":"Tee","full_name":"Tee, Wei Leong"},{"first_name":"Benny","last_name":"Trakhtenbrot","full_name":"Trakhtenbrot, Benny"},{"full_name":"Trebitsch, Maxime","last_name":"Trebitsch","first_name":"Maxime"},{"first_name":"Bram","last_name":"Venemans","full_name":"Venemans, Bram"},{"full_name":"Volonteri, Marta","first_name":"Marta","last_name":"Volonteri"},{"full_name":"Walter, Fabian","first_name":"Fabian","last_name":"Walter"},{"last_name":"Xie","first_name":"Zhang-Liang","full_name":"Xie, Zhang-Liang"},{"last_name":"Yue","first_name":"Minghao","full_name":"Yue, Minghao"},{"full_name":"Zhang, Haowen","last_name":"Zhang","first_name":"Haowen"},{"full_name":"Zhang, Huanian","last_name":"Zhang","first_name":"Huanian"},{"full_name":"Zou, Siwei","first_name":"Siwei","last_name":"Zou"}],"language":[{"iso":"eng"}],"year":"2023","status":"public","doi":"10.3847/2041-8213/accd6f","article_number":"L4","article_processing_charge":"No","extern":"1","date_published":"2023-06-29T00:00:00Z","_id":"17606","date_updated":"2024-09-23T14:08:58Z","publication_status":"published","intvolume":"       951","month":"06","quality_controlled":"1","title":"A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar","type":"journal_article","scopus_import":"1","oa_version":"Published Version","citation":{"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>.","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.","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>","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).","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","day":"29"},{"date_published":"2023-02-23T00:00:00Z","_id":"17611","publication_status":"published","date_updated":"2024-09-24T07:22:28Z","month":"02","intvolume":"       522","quality_controlled":"1","doi":"10.1093/mnrasl/slad016","article_processing_charge":"No","extern":"1","citation":{"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>.","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>.","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>","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>","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.","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."},"publication":"Monthly Notices of the Royal Astronomical Society: Letters","day":"23","type":"journal_article","title":"Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios","page":"L84-L88","scopus_import":"1","oa_version":"Published Version","issue":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnrasl/slad016"}],"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"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","publication_identifier":{"issn":["1745-3925","1745-3933"]},"volume":522,"date_created":"2024-09-05T13:23:29Z","publisher":"Oxford University Press","oa":1,"status":"public","author":[{"full_name":"Komossa, S","last_name":"Komossa","first_name":"S"},{"last_name":"Grupe","first_name":"D","full_name":"Grupe, D"},{"full_name":"Kraus, A","last_name":"Kraus","first_name":"A"},{"first_name":"M A","last_name":"Gurwell","full_name":"Gurwell, M A"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"first_name":"F K","last_name":"Liu","full_name":"Liu, F K"},{"full_name":"Tchekhovskoy, A","last_name":"Tchekhovskoy","first_name":"A"},{"last_name":"Gallo","first_name":"L C","full_name":"Gallo, L C"},{"last_name":"Berton","first_name":"M","full_name":"Berton, M"},{"first_name":"R","last_name":"Blandford","full_name":"Blandford, R"},{"first_name":"J L","last_name":"Gómez","full_name":"Gómez, J L"},{"full_name":"Gonzalez, A G","last_name":"Gonzalez","first_name":"A G"}],"language":[{"iso":"eng"}],"year":"2023"},{"volume":197,"publication_identifier":{"issn":["0003-486X"]},"article_type":"original","related_material":{"link":[{"url":"https://ist.ac.at/en/news/when-is-necessary-sufficient/","description":"News on IST Homepage","relation":"press_release"}]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","abstract":[{"text":"It is known that the Brauer--Manin obstruction to the Hasse principle is vacuous for smooth Fano hypersurfaces of dimension at least 3 over any number field. Moreover, for such varieties it follows from a general conjecture of Colliot-Thélène that the Brauer--Manin obstruction to the Hasse principle should be the only one, so that the Hasse principle is expected to hold. Working over the field of rational numbers and ordering Fano hypersurfaces of fixed degree and dimension by height, we prove that almost every such hypersurface satisfies the Hasse principle provided that the dimension is at least 3. This proves a conjecture of Poonen and Voloch in every case except for cubic surfaces.","lang":"eng"}],"main_file_link":[{"url":"https://arxiv.org/abs/2006.02356","open_access":"1"}],"arxiv":1,"issue":"3","oa":1,"publisher":"Princeton University","date_created":"2020-10-19T14:28:50Z","status":"public","corr_author":"1","department":[{"_id":"TiBr"}],"year":"2023","language":[{"iso":"eng"}],"author":[{"full_name":"Browning, Timothy D","orcid":"0000-0002-8314-0177","first_name":"Timothy D","last_name":"Browning","id":"35827D50-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Pierre Le","last_name":"Boudec","full_name":"Boudec, Pierre Le"},{"full_name":"Sawin, Will","last_name":"Sawin","first_name":"Will"}],"quality_controlled":"1","intvolume":"       197","month":"05","date_updated":"2024-10-21T06:01:30Z","publication_status":"published","_id":"8682","date_published":"2023-05-01T00:00:00Z","article_processing_charge":"No","doi":"10.4007/annals.2023.197.3.3","external_id":{"isi":["000966611000003"],"arxiv":["2006.02356"]},"day":"01","publication":"Annals of Mathematics","citation":{"ieee":"T. D. Browning, P. L. Boudec, and W. Sawin, “The Hasse principle for random Fano hypersurfaces,” <i>Annals of Mathematics</i>, vol. 197, no. 3. Princeton University, pp. 1115–1203, 2023.","short":"T.D. Browning, P.L. Boudec, W. Sawin, Annals of Mathematics 197 (2023) 1115–1203.","apa":"Browning, T. D., Boudec, P. L., &#38; Sawin, W. (2023). The Hasse principle for random Fano hypersurfaces. <i>Annals of Mathematics</i>. Princeton University. <a href=\"https://doi.org/10.4007/annals.2023.197.3.3\">https://doi.org/10.4007/annals.2023.197.3.3</a>","mla":"Browning, Timothy D., et al. “The Hasse Principle for Random Fano Hypersurfaces.” <i>Annals of Mathematics</i>, vol. 197, no. 3, Princeton University, 2023, pp. 1115–203, doi:<a href=\"https://doi.org/10.4007/annals.2023.197.3.3\">10.4007/annals.2023.197.3.3</a>.","ama":"Browning TD, Boudec PL, Sawin W. The Hasse principle for random Fano hypersurfaces. <i>Annals of Mathematics</i>. 2023;197(3):1115-1203. doi:<a href=\"https://doi.org/10.4007/annals.2023.197.3.3\">10.4007/annals.2023.197.3.3</a>","chicago":"Browning, Timothy D, Pierre Le Boudec, and Will Sawin. “The Hasse Principle for Random Fano Hypersurfaces.” <i>Annals of Mathematics</i>. Princeton University, 2023. <a href=\"https://doi.org/10.4007/annals.2023.197.3.3\">https://doi.org/10.4007/annals.2023.197.3.3</a>.","ista":"Browning TD, Boudec PL, Sawin W. 2023. The Hasse principle for random Fano hypersurfaces. Annals of Mathematics. 197(3), 1115–1203."},"isi":1,"oa_version":"Preprint","scopus_import":"1","page":"1115-1203","title":"The Hasse principle for random Fano hypersurfaces","type":"journal_article"},{"year":"2023","language":[{"iso":"eng"}],"author":[{"orcid":"0000-0001-7302-8256","full_name":"Wilsch, Florian Alexander","id":"560601DA-8D36-11E9-A136-7AC1E5697425","last_name":"Wilsch","first_name":"Florian Alexander"}],"department":[{"_id":"TiBr"}],"corr_author":"1","status":"public","oa":1,"publisher":"Oxford University Press","date_created":"2021-01-22T09:31:09Z","acknowledgement":"This work was supported by the German Academic Exchange Service. Parts of this article were prepared at the Institut de Mathémathiques de Jussieu—Paris Rive Gauche. I wish to thank Antoine Chambert-Loir for his remarks and the institute for its hospitality, as well as the anonymous referee for several useful remarks and suggestions for improvements.","issue":"8","arxiv":1,"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1901.08503"}],"abstract":[{"text":"We determine an asymptotic formula for the number of integral points of bounded height on a blow-up of P3 outside certain planes using universal torsors.","lang":"eng"}],"article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","volume":2023,"publication_identifier":{"eissn":["1687-0247"],"issn":["1073-7928"]},"page":"6780-6808","title":"Integral points of bounded height on a log Fano threefold","type":"journal_article","scopus_import":"1","oa_version":"Preprint","isi":1,"citation":{"apa":"Wilsch, F. A. (2023). Integral points of bounded height on a log Fano threefold. <i>International Mathematics Research Notices</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/imrn/rnac048\">https://doi.org/10.1093/imrn/rnac048</a>","short":"F.A. Wilsch, International Mathematics Research Notices 2023 (2023) 6780–6808.","ieee":"F. A. Wilsch, “Integral points of bounded height on a log Fano threefold,” <i>International Mathematics Research Notices</i>, vol. 2023, no. 8. Oxford University Press, pp. 6780–6808, 2023.","chicago":"Wilsch, Florian Alexander. “Integral Points of Bounded Height on a Log Fano Threefold.” <i>International Mathematics Research Notices</i>. Oxford University Press, 2023. <a href=\"https://doi.org/10.1093/imrn/rnac048\">https://doi.org/10.1093/imrn/rnac048</a>.","mla":"Wilsch, Florian Alexander. “Integral Points of Bounded Height on a Log Fano Threefold.” <i>International Mathematics Research Notices</i>, vol. 2023, no. 8, Oxford University Press, 2023, pp. 6780–808, doi:<a href=\"https://doi.org/10.1093/imrn/rnac048\">10.1093/imrn/rnac048</a>.","ama":"Wilsch FA. Integral points of bounded height on a log Fano threefold. <i>International Mathematics Research Notices</i>. 2023;2023(8):6780-6808. doi:<a href=\"https://doi.org/10.1093/imrn/rnac048\">10.1093/imrn/rnac048</a>","ista":"Wilsch FA. 2023. Integral points of bounded height on a log Fano threefold. International Mathematics Research Notices. 2023(8), 6780–6808."},"publication":"International Mathematics Research Notices","day":"01","external_id":{"arxiv":["1901.08503"],"isi":["000773116000001"]},"doi":"10.1093/imrn/rnac048","article_processing_charge":"No","date_published":"2023-04-01T00:00:00Z","date_updated":"2025-05-14T11:07:41Z","publication_status":"published","_id":"9034","quality_controlled":"1","month":"04","intvolume":"      2023"},{"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","volume":253,"publication_identifier":{"eissn":["1565-8511"]},"arxiv":1,"acknowledgement":"This work was done while both authors were employed at the University of Innsbruck and enjoyed the full support of Austrian Science Fund (FWF): P 30902-N35.","abstract":[{"lang":"eng","text":"In 1998 Burago and Kleiner and (independently) McMullen gave examples of separated nets in Euclidean space which are non-bilipschitz equivalent to the integer lattice. We study weaker notions of equivalence of separated nets and demonstrate that such notions also give rise to distinct equivalence classes. Put differently, we find occurrences of particularly strong divergence of separated nets from the integer lattice. Our approach generalises that of Burago and Kleiner and McMullen which takes place largely in a continuous setting. Existence of irregular separated nets is verified via the existence of non-realisable density functions ρ:[0,1]d→(0,∞). In the present work we obtain stronger types of non-realisable densities."}],"file_date_updated":"2021-07-14T07:41:50Z","date_created":"2021-07-14T07:01:28Z","publisher":"Springer Nature","oa":1,"has_accepted_license":"1","ddc":["515","516"],"status":"public","department":[{"_id":"UlWa"}],"author":[{"full_name":"Dymond, Michael","first_name":"Michael","last_name":"Dymond"},{"id":"21AE5134-9EAC-11EA-BEA2-D7BD3DDC885E","last_name":"Kaluza","first_name":"Vojtech","orcid":"0000-0002-2512-8698","full_name":"Kaluza, Vojtech"}],"language":[{"iso":"eng"}],"year":"2023","_id":"9652","date_updated":"2023-08-14T11:26:34Z","publication_status":"published","intvolume":"       253","keyword":["Lipschitz","bilipschitz","bounded displacement","modulus of continuity","separated net","non-realisable density","Burago--Kleiner construction"],"month":"03","quality_controlled":"1","date_published":"2023-03-01T00:00:00Z","article_processing_charge":"No","doi":"10.1007/s11856-022-2448-6","day":"01","publication":"Israel Journal of Mathematics","external_id":{"isi":["000904950300003"],"arxiv":["1903.05923"]},"isi":1,"file":[{"content_type":"application/pdf","date_updated":"2021-07-14T07:41:50Z","file_id":"9653","checksum":"6fa0a3207dd1d6467c309fd1bcc867d1","relation":"main_file","creator":"vkaluza","access_level":"open_access","file_name":"separated_nets.pdf","date_created":"2021-07-14T07:41:50Z","file_size":900422}],"citation":{"ieee":"M. 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Dunajova, B. Prats Mateu, P. Radler, K. Lim, D. Brandis, P. Velicky, J.G. Danzl, R.W. Wong, J. Elgeti, E.B. Hannezo, M. Loose, (2023).","ieee":"Z. Dunajova <i>et al.</i>, “Chiral and nematic phases of flexible active filaments.” Institute of Science and Technology Austria, 2023."},"oa_version":"Published Version","type":"research_data","title":"Chiral and nematic phases of flexible active filaments","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","related_material":{"record":[{"id":"13314","relation":"used_in_publication","status":"public"},{"id":"21423","status":"public","relation":"used_in_publication"}]},"acknowledged_ssus":[{"_id":"Bio"},{"_id":"LifeSc"}],"acknowledgement":"This work was supported by the European Research Council through grant ERC 2015-StG-679239 and by the Austrian Science Fund (FWF) StandAlone P34607 to M.L., B. P.M.  was also supported by the Kanazawa University WPI- NanoLSI Bio-SPM collaborative research program. Z.D. has received funding from Doctoral Programme of the Austrian Academy of Sciences (OeAW): Grant agreement 26360. We thank Jan Brugues (MPI CBG, Dresden, Germany), Andela Saric (ISTA, Klosterneuburg, Austria), Daniel Pearce (Uni Geneva, Switzerland) for valuable scientific input and comments on the manuscript. We are also thankful for the support by the Scientific Service Units (SSU) of IST Austria through resources provided by the Imaging and Optics Facility (IOF) and the Lab Support Facility (LSF). ","abstract":[{"lang":"eng","text":"The emergence of large-scale order in self-organized systems relies on local interactions between individual components. During bacterial cell division, FtsZ -- a prokaryotic homologue of the eukaryotic protein tubulin -- polymerizes into treadmilling filaments that further organize into a cytoskeletal ring. In vitro, FtsZ filaments can form dynamic chiral assemblies. However, how the active and passive properties of individual filaments relate to these large-scale self-organized structures remains poorly understood. Here, we connect single filament properties with the mesoscopic scale by combining minimal active matter simulations and biochemical reconstitution experiments. We show that density and flexibility of active chiral filaments define their global order. At intermediate densities, curved, flexible filaments organize into chiral rings and polar bands. An effectively nematic organization dominates for high densities and for straight, mutant filaments with increased rigidity. Our predicted phase diagram captures these features quantitatively, demonstrating how the flexibility, density and chirality of active filaments affect their collective behaviour. Our findings shed light on the fundamental properties of active chiral matter and explain how treadmilling FtsZ filaments organize during bacterial cell division. 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During bacterial cell division, FtsZ—a prokaryotic homologue of the eukaryotic protein tubulin—polymerizes into treadmilling filaments that further organize into a cytoskeletal ring. In vitro, FtsZ filaments can form dynamic chiral assemblies. However, how the active and passive properties of individual filaments relate to these large-scale self-organized structures remains poorly understood. Here we connect single-filament properties with the mesoscopic scale by combining minimal active matter simulations and biochemical reconstitution experiments. We show that the density and flexibility of active chiral filaments define their global order. At intermediate densities, curved, flexible filaments organize into chiral rings and polar bands. An effectively nematic organization dominates for high densities and for straight, mutant filaments with increased rigidity. Our predicted phase diagram quantitatively captures these features, demonstrating how the flexibility, density and chirality of the active filaments affect their collective behaviour. Our findings shed light on the fundamental properties of active chiral matter and explain how treadmilling FtsZ filaments organize during bacterial cell division.","lang":"eng"}],"acknowledgement":"This work was supported by the European Research Council through grant ERC 2015-StG-679239 and by the Austrian Science Fund (FWF) StandAlone P34607 to M.L., B. P.M. was also supported by the Kanazawa University WPI- NanoLSI Bio-SPM collaborative research program. Z.D. has received funding from Doctoral Programme of the Austrian Academy of Sciences (OeAW): Grant agreement 26360. We thank Jan Brugues (MPI CBG, Dresden, Germany), Andela Saric (ISTA, Klosterneuburg, Austria), Daniel Pearce (Uni Geneva, Switzerland) for valuable scientific input and comments on the manuscript. 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