--- _id: '9981' abstract: - lang: eng text: "The numerical simulation of dynamical phenomena in interacting quantum systems is a notoriously hard problem. Although a number of promising numerical methods exist, they often have limited applicability due to the growth of entanglement or the presence of the so-called sign problem. In this work, we develop an importance sampling scheme for the simulation of quantum spin dynamics, building on a recent approach mapping quantum spin systems to classical stochastic processes. The importance sampling scheme is based on identifying the classical trajectory that yields the largest contribution to a given quantum observable. An exact transformation is then carried out to preferentially sample trajectories that are close to the dominant one. We demonstrate that this approach is capable of reducing the temporal growth of fluctuations in the stochastic quantities, thus extending the range of accessible times and system sizes compared to direct sampling. We discuss advantages and limitations of the proposed approach, outlining directions\r\nfor further developments." article_number: '048' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Stefano full_name: De Nicola, Stefano id: 42832B76-F248-11E8-B48F-1D18A9856A87 last_name: De Nicola orcid: 0000-0002-4842-6671 citation: ama: De Nicola S. Importance sampling scheme for the stochastic simulation of quantum spin dynamics. SciPost Physics. 2021;11(3). doi:10.21468/scipostphys.11.3.048 apa: De Nicola, S. (2021). Importance sampling scheme for the stochastic simulation of quantum spin dynamics. SciPost Physics. SciPost Foundation. https://doi.org/10.21468/scipostphys.11.3.048 chicago: De Nicola, Stefano. “Importance Sampling Scheme for the Stochastic Simulation of Quantum Spin Dynamics.” SciPost Physics. SciPost Foundation, 2021. https://doi.org/10.21468/scipostphys.11.3.048. ieee: S. De Nicola, “Importance sampling scheme for the stochastic simulation of quantum spin dynamics,” SciPost Physics, vol. 11, no. 3. SciPost Foundation, 2021. ista: De Nicola S. 2021. Importance sampling scheme for the stochastic simulation of quantum spin dynamics. SciPost Physics. 11(3), 048. mla: De Nicola, Stefano. “Importance Sampling Scheme for the Stochastic Simulation of Quantum Spin Dynamics.” SciPost Physics, vol. 11, no. 3, 048, SciPost Foundation, 2021, doi:10.21468/scipostphys.11.3.048. short: S. De Nicola, SciPost Physics 11 (2021). date_created: 2021-09-02T11:49:47Z date_published: 2021-09-02T00:00:00Z date_updated: 2025-05-14T10:51:45Z day: '02' ddc: - '519' department: - _id: MaSe doi: 10.21468/scipostphys.11.3.048 ec_funded: 1 external_id: arxiv: - '2103.16468' isi: - '000692534200001' file: - access_level: open_access checksum: e4ec69d893e31811efc6093cb6ea8eb7 content_type: application/pdf creator: cchlebak date_created: 2021-09-02T14:05:43Z date_updated: 2021-09-02T14:05:43Z file_id: '9984' file_name: 2021_SciPostPhys_DeNicola.pdf file_size: 373833 relation: main_file success: 1 file_date_updated: 2021-09-02T14:05:43Z has_accepted_license: '1' intvolume: ' 11' isi: 1 issue: '3' keyword: - General Physics and Astronomy language: - iso: eng license: https://creativecommons.org/licenses/by/4.0/ month: '09' oa: 1 oa_version: Published Version project: - _id: 260C2330-B435-11E9-9278-68D0E5697425 call_identifier: H2020 grant_number: '754411' name: ISTplus - Postdoctoral Fellowships publication: SciPost Physics publication_identifier: eissn: - 2666-9366 issn: - 2542-4653 publication_status: published publisher: SciPost Foundation quality_controlled: '1' scopus_import: '1' status: public title: Importance sampling scheme for the stochastic simulation of quantum spin dynamics tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 11 year: '2021' ... --- _id: '9985' abstract: - lang: eng text: AMPA receptor (AMPAR) abundance and positioning at excitatory synapses regulates the strength of transmission. Changes in AMPAR localisation can enact synaptic plasticity, allowing long-term information storage, and is therefore tightly controlled. Multiple mechanisms regulating AMPAR synaptic anchoring have been described, but with limited coherence or comparison between reports, our understanding of this process is unclear. Here, combining synaptic recordings from mouse hippocampal slices and super-resolution imaging in dissociated cultures, we compare the contributions of three AMPAR interaction domains controlling transmission at hippocampal CA1 synapses. We show that the AMPAR C-termini play only a modulatory role, whereas the extracellular N-terminal domain (NTD) and PDZ interactions of the auxiliary subunit TARP γ8 are both crucial, and each is sufficient to maintain transmission. Our data support a model in which γ8 accumulates AMPARs at the postsynaptic density, where the NTD further tunes their positioning. This interplay between cytosolic (TARP γ8) and synaptic cleft (NTD) interactions provides versatility to regulate synaptic transmission and plasticity. acknowledgement: The authors are very grateful to Andrew Penn for advice and discussions on surface receptor labelling in slice tissue, dissociated culture transfection, and for providing tdTomato and BirAER expression plasmids. This work would not have been possible without support from the Biological Services teams at both the Laboratory of Molecular Biology and Ares facilities. We are also very grateful to Nick Barry and Jerome Boulanger of the LMB Light Microscopy facility for support with confocal and STORM imaging and analysis, Junichi Takagi for providing scFv-Clasp expression constructs, Veronica Chang for assistance with scFv-Clasp protein production, and Nejc Kejzar for assistance with cluster analysis. We would like to thank Teru Nakagawa and Ole Paulsen for critical reading of the manuscript and constructive feedback. This work was supported by grants from the Medical Research Council (MC_U105174197) and BBSRC (BB/N002113/1). article_number: '5083' article_processing_charge: Yes article_type: original author: - first_name: Jake full_name: Watson, Jake id: 63836096-4690-11EA-BD4E-32803DDC885E last_name: Watson orcid: 0000-0002-8698-3823 - first_name: Alexandra full_name: Pinggera, Alexandra last_name: Pinggera - first_name: Hinze full_name: Ho, Hinze last_name: Ho - first_name: Ingo H. full_name: Greger, Ingo H. last_name: Greger citation: ama: Watson J, Pinggera A, Ho H, Greger IH. AMPA receptor anchoring at CA1 synapses is determined by N-terminal domain and TARP γ8 interactions. Nature Communications. 2021;12(1). doi:10.1038/s41467-021-25281-4 apa: Watson, J., Pinggera, A., Ho, H., & Greger, I. H. (2021). AMPA receptor anchoring at CA1 synapses is determined by N-terminal domain and TARP γ8 interactions. Nature Communications. Nature Publishing Group. https://doi.org/10.1038/s41467-021-25281-4 chicago: Watson, Jake, Alexandra Pinggera, Hinze Ho, and Ingo H. Greger. “AMPA Receptor Anchoring at CA1 Synapses Is Determined by N-Terminal Domain and TARP Γ8 Interactions.” Nature Communications. Nature Publishing Group, 2021. https://doi.org/10.1038/s41467-021-25281-4. ieee: J. Watson, A. Pinggera, H. Ho, and I. H. Greger, “AMPA receptor anchoring at CA1 synapses is determined by N-terminal domain and TARP γ8 interactions,” Nature Communications, vol. 12, no. 1. Nature Publishing Group, 2021. ista: Watson J, Pinggera A, Ho H, Greger IH. 2021. AMPA receptor anchoring at CA1 synapses is determined by N-terminal domain and TARP γ8 interactions. Nature Communications. 12(1), 5083. mla: Watson, Jake, et al. “AMPA Receptor Anchoring at CA1 Synapses Is Determined by N-Terminal Domain and TARP Γ8 Interactions.” Nature Communications, vol. 12, no. 1, 5083, Nature Publishing Group, 2021, doi:10.1038/s41467-021-25281-4. short: J. Watson, A. Pinggera, H. Ho, I.H. Greger, Nature Communications 12 (2021). date_created: 2021-09-05T22:01:23Z date_published: 2021-08-23T00:00:00Z date_updated: 2023-08-11T11:07:51Z day: '23' ddc: - '612' department: - _id: PeJo doi: 10.1038/s41467-021-25281-4 external_id: isi: - '000687672000006' pmid: - '34426577 ' file: - access_level: open_access checksum: 1bf4f6a561f96bc426d754de9cb57710 content_type: application/pdf creator: cchlebak date_created: 2021-09-08T12:57:06Z date_updated: 2021-09-08T12:57:06Z file_id: '9991' file_name: 2021_NatureCommunications_Watson.pdf file_size: 18310502 relation: main_file success: 1 file_date_updated: 2021-09-08T12:57:06Z has_accepted_license: '1' intvolume: ' 12' isi: 1 issue: '1' language: - iso: eng month: '08' oa: 1 oa_version: Published Version pmid: 1 publication: Nature Communications publication_identifier: eissn: - 2041-1723 publication_status: published publisher: Nature Publishing Group quality_controlled: '1' scopus_import: '1' status: public title: AMPA receptor anchoring at CA1 synapses is determined by N-terminal domain and TARP γ8 interactions tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8 volume: 12 year: '2021' ... --- _id: '9986' abstract: - lang: eng text: Size control is a fundamental question in biology, showing incremental complexity in plants, whose cells possess a rigid cell wall. The phytohormone auxin is a vital growth regulator with central importance for differential growth control. Our results indicate that auxin-reliant growth programs affect the molecular complexity of xyloglucans, the major type of cell wall hemicellulose in eudicots. Auxin-dependent induction and repression of growth coincide with reduced and enhanced molecular complexity of xyloglucans, respectively. In agreement with a proposed function in growth control, genetic interference with xyloglucan side decorations distinctly modulates auxin-dependent differential growth rates. Our work proposes that auxin-dependent growth programs have a spatially defined effect on xyloglucan’s molecular structure, which in turn affects cell wall mechanics and specifies differential, gravitropic hypocotyl growth. acknowledgement: "We are grateful to Paul Knox, Markus Pauly, Malcom O’Neill, and Ignacio Zarra for providing published material; the BOKU-VIBT Imaging Center for access and M. Debreczeny for expertise; J.I. Thaker and Georg Seifert for critical reading.\r\n" article_number: '9222' article_processing_charge: Yes article_type: original author: - first_name: Silvia Melina full_name: Velasquez, Silvia Melina last_name: Velasquez - first_name: Xiaoyuan full_name: Guo, Xiaoyuan last_name: Guo - first_name: Marçal full_name: Gallemi, Marçal id: 460C6802-F248-11E8-B48F-1D18A9856A87 last_name: Gallemi orcid: 0000-0003-4675-6893 - first_name: Bibek full_name: Aryal, Bibek last_name: Aryal - first_name: Peter full_name: Venhuizen, Peter last_name: Venhuizen - first_name: Elke full_name: Barbez, Elke last_name: Barbez - first_name: Kai Alexander full_name: Dünser, Kai Alexander last_name: Dünser - first_name: Martin full_name: Darino, Martin last_name: Darino - first_name: Aleš full_name: Pӗnčík, Aleš last_name: Pӗnčík - first_name: Ondřej full_name: Novák, Ondřej last_name: Novák - first_name: Maria full_name: Kalyna, Maria last_name: Kalyna - first_name: Gregory full_name: Mouille, Gregory last_name: Mouille - first_name: Eva full_name: Benková, Eva id: 38F4F166-F248-11E8-B48F-1D18A9856A87 last_name: Benková orcid: 0000-0002-8510-9739 - first_name: Rishikesh P. full_name: Bhalerao, Rishikesh P. last_name: Bhalerao - first_name: Jozef full_name: Mravec, Jozef last_name: Mravec - first_name: Jürgen full_name: Kleine-Vehn, Jürgen last_name: Kleine-Vehn citation: ama: Velasquez SM, Guo X, Gallemi M, et al. Xyloglucan remodeling defines auxin-dependent differential tissue expansion in plants. International Journal of Molecular Sciences. 2021;22(17). doi:10.3390/ijms22179222 apa: Velasquez, S. M., Guo, X., Gallemi, M., Aryal, B., Venhuizen, P., Barbez, E., … Kleine-Vehn, J. (2021). Xyloglucan remodeling defines auxin-dependent differential tissue expansion in plants. International Journal of Molecular Sciences. MDPI. https://doi.org/10.3390/ijms22179222 chicago: Velasquez, Silvia Melina, Xiaoyuan Guo, Marçal Gallemi, Bibek Aryal, Peter Venhuizen, Elke Barbez, Kai Alexander Dünser, et al. “Xyloglucan Remodeling Defines Auxin-Dependent Differential Tissue Expansion in Plants.” International Journal of Molecular Sciences. MDPI, 2021. https://doi.org/10.3390/ijms22179222. ieee: S. M. Velasquez et al., “Xyloglucan remodeling defines auxin-dependent differential tissue expansion in plants,” International Journal of Molecular Sciences, vol. 22, no. 17. MDPI, 2021. ista: Velasquez SM, Guo X, Gallemi M, Aryal B, Venhuizen P, Barbez E, Dünser KA, Darino M, Pӗnčík A, Novák O, Kalyna M, Mouille G, Benková E, Bhalerao RP, Mravec J, Kleine-Vehn J. 2021. Xyloglucan remodeling defines auxin-dependent differential tissue expansion in plants. International Journal of Molecular Sciences. 22(17), 9222. mla: Velasquez, Silvia Melina, et al. “Xyloglucan Remodeling Defines Auxin-Dependent Differential Tissue Expansion in Plants.” International Journal of Molecular Sciences, vol. 22, no. 17, 9222, MDPI, 2021, doi:10.3390/ijms22179222. short: S.M. Velasquez, X. Guo, M. Gallemi, B. Aryal, P. Venhuizen, E. Barbez, K.A. Dünser, M. Darino, A. Pӗnčík, O. Novák, M. Kalyna, G. Mouille, E. Benková, R.P. Bhalerao, J. Mravec, J. Kleine-Vehn, International Journal of Molecular Sciences 22 (2021). corr_author: '1' date_created: 2021-09-05T22:01:24Z date_published: 2021-08-26T00:00:00Z date_updated: 2024-10-09T21:00:50Z day: '26' ddc: - '575' department: - _id: EvBe doi: 10.3390/ijms22179222 external_id: isi: - '000694347100001' pmid: - '34502129' file: - access_level: open_access checksum: 6b7055cf89f1b7ed8594c3fdf56f000b content_type: application/pdf creator: cchlebak date_created: 2021-09-06T12:50:19Z date_updated: 2021-09-07T09:04:53Z file_id: '9988' file_name: 2021_IntJMolecularSciences_Velasquez.pdf file_size: 2162247 relation: main_file file_date_updated: 2021-09-07T09:04:53Z has_accepted_license: '1' intvolume: ' 22' isi: 1 issue: '17' keyword: - auxin - growth - cell wall - xyloglucans - hypocotyls - gravitropism language: - iso: eng month: '08' oa: 1 oa_version: Published Version pmid: 1 publication: International Journal of Molecular Sciences publication_identifier: eissn: - 1422-0067 issn: - 1661-6596 publication_status: published publisher: MDPI quality_controlled: '1' scopus_import: '1' status: public title: Xyloglucan remodeling defines auxin-dependent differential tissue expansion in plants tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 22 year: '2021' ... --- _id: '9987' abstract: - lang: eng text: 'Stateless model checking (SMC) is one of the standard approaches to the verification of concurrent programs. As scheduling non-determinism creates exponentially large spaces of thread interleavings, SMC attempts to partition this space into equivalence classes and explore only a few representatives from each class. The efficiency of this approach depends on two factors: (a) the coarseness of the partitioning, and (b) the time to generate representatives in each class. For this reason, the search for coarse partitionings that are efficiently explorable is an active research challenge. In this work we present RVF-SMC , a new SMC algorithm that uses a novel reads-value-from (RVF) partitioning. Intuitively, two interleavings are deemed equivalent if they agree on the value obtained in each read event, and read events induce consistent causal orderings between them. The RVF partitioning is provably coarser than recent approaches based on Mazurkiewicz and “reads-from” partitionings. Our experimental evaluation reveals that RVF is quite often a very effective equivalence, as the underlying partitioning is exponentially coarser than other approaches. Moreover, RVF-SMC generates representatives very efficiently, as the reduction in the partitioning is often met with significant speed-ups in the model checking task.' acknowledgement: The research was partially funded by the ERC CoG 863818 (ForM-SMArt) and the Vienna Science and Technology Fund (WWTF) through project ICT15-003. alternative_title: - LNCS article_processing_charge: Yes arxiv: 1 author: - first_name: Pratyush full_name: Agarwal, Pratyush last_name: Agarwal - first_name: Krishnendu full_name: Chatterjee, Krishnendu id: 2E5DCA20-F248-11E8-B48F-1D18A9856A87 last_name: Chatterjee orcid: 0000-0002-4561-241X - first_name: Shreya full_name: Pathak, Shreya last_name: Pathak - first_name: Andreas full_name: Pavlogiannis, Andreas id: 49704004-F248-11E8-B48F-1D18A9856A87 last_name: Pavlogiannis orcid: 0000-0002-8943-0722 - first_name: Viktor full_name: Toman, Viktor id: 3AF3DA7C-F248-11E8-B48F-1D18A9856A87 last_name: Toman orcid: 0000-0001-9036-063X citation: ama: 'Agarwal P, Chatterjee K, Pathak S, Pavlogiannis A, Toman V. Stateless model checking under a reads-value-from equivalence. In: 33rd International Conference on Computer-Aided Verification . Vol 12759. Springer Nature; 2021:341-366. doi:10.1007/978-3-030-81685-8_16' apa: 'Agarwal, P., Chatterjee, K., Pathak, S., Pavlogiannis, A., & Toman, V. (2021). Stateless model checking under a reads-value-from equivalence. In 33rd International Conference on Computer-Aided Verification (Vol. 12759, pp. 341–366). Virtual: Springer Nature. https://doi.org/10.1007/978-3-030-81685-8_16' chicago: Agarwal, Pratyush, Krishnendu Chatterjee, Shreya Pathak, Andreas Pavlogiannis, and Viktor Toman. “Stateless Model Checking under a Reads-Value-from Equivalence.” In 33rd International Conference on Computer-Aided Verification , 12759:341–66. Springer Nature, 2021. https://doi.org/10.1007/978-3-030-81685-8_16. ieee: P. Agarwal, K. Chatterjee, S. Pathak, A. Pavlogiannis, and V. Toman, “Stateless model checking under a reads-value-from equivalence,” in 33rd International Conference on Computer-Aided Verification , Virtual, 2021, vol. 12759, pp. 341–366. ista: 'Agarwal P, Chatterjee K, Pathak S, Pavlogiannis A, Toman V. 2021. Stateless model checking under a reads-value-from equivalence. 33rd International Conference on Computer-Aided Verification . CAV: Computer Aided Verification , LNCS, vol. 12759, 341–366.' mla: Agarwal, Pratyush, et al. “Stateless Model Checking under a Reads-Value-from Equivalence.” 33rd International Conference on Computer-Aided Verification , vol. 12759, Springer Nature, 2021, pp. 341–66, doi:10.1007/978-3-030-81685-8_16. short: P. Agarwal, K. Chatterjee, S. Pathak, A. Pavlogiannis, V. Toman, in:, 33rd International Conference on Computer-Aided Verification , Springer Nature, 2021, pp. 341–366. conference: end_date: 2021-07-23 location: Virtual name: 'CAV: Computer Aided Verification ' start_date: 2021-07-20 corr_author: '1' date_created: 2021-09-05T22:01:24Z date_published: 2021-07-15T00:00:00Z date_updated: 2026-04-08T07:00:30Z day: '15' ddc: - '000' department: - _id: KrCh doi: 10.1007/978-3-030-81685-8_16 ec_funded: 1 external_id: arxiv: - '2105.06424' isi: - '000698732400016' file: - access_level: open_access checksum: 4b346e5fbaa8b9bdf107819c7b2aadee content_type: application/pdf creator: dernst date_created: 2022-05-13T07:00:20Z date_updated: 2022-05-13T07:00:20Z file_id: '11368' file_name: 2021_LNCS_Agarwal.pdf file_size: 1516756 relation: main_file success: 1 file_date_updated: 2022-05-13T07:00:20Z has_accepted_license: '1' isi: 1 language: - iso: eng month: '07' oa: 1 oa_version: Published Version page: 341-366 project: - _id: 25892FC0-B435-11E9-9278-68D0E5697425 grant_number: ICT15-003 name: Efficient Algorithms for Computer Aided Verification - _id: 0599E47C-7A3F-11EA-A408-12923DDC885E call_identifier: H2020 grant_number: '863818' name: 'Formal Methods for Stochastic Models: Algorithms and Applications' publication: '33rd International Conference on Computer-Aided Verification ' publication_identifier: eisbn: - 978-3-030-81685-8 eissn: - 1611-3349 isbn: - 978-3-030-81684-1 issn: - 0302-9743 publication_status: published publisher: Springer Nature quality_controlled: '1' related_material: record: - id: '10199' relation: dissertation_contains status: public scopus_import: '1' status: public title: Stateless model checking under a reads-value-from equivalence tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: conference user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8 volume: '12759 ' year: '2021' ... --- _id: '9998' abstract: - lang: eng text: We define quantum equivariant K-theory of Nakajima quiver varieties. We discuss type A in detail as well as its connections with quantum XXZ spin chains and trigonometric Ruijsenaars-Schneider models. Finally we study a limit which produces a K-theoretic version of results of Givental and Kim, connecting quantum geometry of flag varieties and Toda lattice. acknowledgement: 'First of all we would like to thank Andrei Okounkov for invaluable discussions, advises and sharing with us his fantastic viewpoint on modern quantum geometry. We are also grateful to D. Korb and Z. Zhou for their interest and comments. The work of A. Smirnov was supported in part by RFBR Grants under Numbers 15-02-04175 and 15-01-04217 and in part by NSF Grant DMS–2054527. The work of P. Koroteev, A.M. Zeitlin and A. Smirnov is supported in part by AMS Simons travel Grant. A. M. Zeitlin is partially supported by Simons Collaboration Grant, Award ID: 578501. Open access funding provided by Institute of Science and Technology (IST Austria).' article_number: '87' article_processing_charge: Yes (via OA deal) article_type: original author: - first_name: Peter full_name: Koroteev, Peter last_name: Koroteev - first_name: Petr full_name: Pushkar, Petr id: 151DCEB6-9EC3-11E9-8480-ABECE5697425 last_name: Pushkar - first_name: Andrey V. full_name: Smirnov, Andrey V. last_name: Smirnov - first_name: Anton M. full_name: Zeitlin, Anton M. last_name: Zeitlin citation: ama: Koroteev P, Pushkar P, Smirnov AV, Zeitlin AM. Quantum K-theory of quiver varieties and many-body systems. Selecta Mathematica. 2021;27(5). doi:10.1007/s00029-021-00698-3 apa: Koroteev, P., Pushkar, P., Smirnov, A. V., & Zeitlin, A. M. (2021). Quantum K-theory of quiver varieties and many-body systems. Selecta Mathematica. Springer Nature. https://doi.org/10.1007/s00029-021-00698-3 chicago: Koroteev, Peter, Petr Pushkar, Andrey V. Smirnov, and Anton M. Zeitlin. “Quantum K-Theory of Quiver Varieties and Many-Body Systems.” Selecta Mathematica. Springer Nature, 2021. https://doi.org/10.1007/s00029-021-00698-3. ieee: P. Koroteev, P. Pushkar, A. V. Smirnov, and A. M. Zeitlin, “Quantum K-theory of quiver varieties and many-body systems,” Selecta Mathematica, vol. 27, no. 5. Springer Nature, 2021. ista: Koroteev P, Pushkar P, Smirnov AV, Zeitlin AM. 2021. Quantum K-theory of quiver varieties and many-body systems. Selecta Mathematica. 27(5), 87. mla: Koroteev, Peter, et al. “Quantum K-Theory of Quiver Varieties and Many-Body Systems.” Selecta Mathematica, vol. 27, no. 5, 87, Springer Nature, 2021, doi:10.1007/s00029-021-00698-3. short: P. Koroteev, P. Pushkar, A.V. Smirnov, A.M. Zeitlin, Selecta Mathematica 27 (2021). date_created: 2021-09-12T22:01:22Z date_published: 2021-08-30T00:00:00Z date_updated: 2025-04-15T06:53:09Z day: '30' ddc: - '530' department: - _id: TaHa doi: 10.1007/s00029-021-00698-3 external_id: isi: - '000692795200001' file: - access_level: open_access checksum: beadc5a722ffb48190e1e63ee2dbfee5 content_type: application/pdf creator: cchlebak date_created: 2021-09-13T11:31:34Z date_updated: 2021-09-13T11:31:34Z file_id: '10010' file_name: 2021_SelectaMath_Koroteev.pdf file_size: 584648 relation: main_file success: 1 file_date_updated: 2021-09-13T11:31:34Z has_accepted_license: '1' intvolume: ' 27' isi: 1 issue: '5' language: - iso: eng month: '08' oa: 1 oa_version: Published Version project: - _id: B67AFEDC-15C9-11EA-A837-991A96BB2854 name: IST Austria Open Access Fund publication: Selecta Mathematica publication_identifier: eissn: - 1420-9020 issn: - 1022-1824 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Quantum K-theory of quiver varieties and many-body systems tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8 volume: 27 year: '2021' ... --- _id: '9999' abstract: - lang: eng text: 'The developmental strategies used by progenitor cells to endure a safe journey from their induction place towards the site of terminal differentiation are still poorly understood. Here we uncovered a progenitor cell allocation mechanism that stems from an incomplete process of epithelial delamination that allows progenitors to coordinate their movement with adjacent extra-embryonic tissues. Progenitors of the zebrafish laterality organ originate from the surface epithelial enveloping layer by an apical constriction process of cell delamination. During this process, progenitors retain long-term apical contacts that enable the epithelial layer to pull a subset of progenitors along their way towards the vegetal pole. The remaining delaminated progenitors follow apically-attached progenitors’ movement by a co-attraction mechanism, avoiding sequestration by the adjacent endoderm, ensuring their fate and collective allocation at the differentiation site. Thus, we reveal that incomplete delamination serves as a cellular platform for coordinated tissue movements during development. Impact Statement: Incomplete delamination serves as a cellular platform for coordinated tissue movements during development, guiding newly formed progenitor cell groups to the differentiation site.' article_number: e66483 article_processing_charge: Yes article_type: original author: - first_name: Eduardo full_name: Pulgar, Eduardo last_name: Pulgar - first_name: Cornelia full_name: Schwayer, Cornelia id: 3436488C-F248-11E8-B48F-1D18A9856A87 last_name: Schwayer orcid: 0000-0001-5130-2226 - first_name: Néstor full_name: Guerrero, Néstor last_name: Guerrero - first_name: Loreto full_name: López, Loreto last_name: López - first_name: Susana full_name: Márquez, Susana last_name: Márquez - first_name: Steffen full_name: Härtel, Steffen last_name: Härtel - first_name: Rodrigo full_name: Soto, Rodrigo last_name: Soto - first_name: Carl Philipp full_name: Heisenberg, Carl Philipp last_name: Heisenberg - first_name: Miguel L. full_name: Concha, Miguel L. last_name: Concha citation: ama: Pulgar E, Schwayer C, Guerrero N, et al. Apical contacts stemming from incomplete delamination guide progenitor cell allocation through a dragging mechanism. eLife. 2021;10. doi:10.7554/eLife.66483 apa: Pulgar, E., Schwayer, C., Guerrero, N., López, L., Márquez, S., Härtel, S., … Concha, M. L. (2021). Apical contacts stemming from incomplete delamination guide progenitor cell allocation through a dragging mechanism. ELife. eLife Sciences Publications. https://doi.org/10.7554/eLife.66483 chicago: Pulgar, Eduardo, Cornelia Schwayer, Néstor Guerrero, Loreto López, Susana Márquez, Steffen Härtel, Rodrigo Soto, Carl Philipp Heisenberg, and Miguel L. Concha. “Apical Contacts Stemming from Incomplete Delamination Guide Progenitor Cell Allocation through a Dragging Mechanism.” ELife. eLife Sciences Publications, 2021. https://doi.org/10.7554/eLife.66483. ieee: E. Pulgar et al., “Apical contacts stemming from incomplete delamination guide progenitor cell allocation through a dragging mechanism,” eLife, vol. 10. eLife Sciences Publications, 2021. ista: Pulgar E, Schwayer C, Guerrero N, López L, Márquez S, Härtel S, Soto R, Heisenberg CP, Concha ML. 2021. Apical contacts stemming from incomplete delamination guide progenitor cell allocation through a dragging mechanism. eLife. 10, e66483. mla: Pulgar, Eduardo, et al. “Apical Contacts Stemming from Incomplete Delamination Guide Progenitor Cell Allocation through a Dragging Mechanism.” ELife, vol. 10, e66483, eLife Sciences Publications, 2021, doi:10.7554/eLife.66483. short: E. Pulgar, C. Schwayer, N. Guerrero, L. López, S. Márquez, S. Härtel, R. Soto, C.P. Heisenberg, M.L. Concha, ELife 10 (2021). date_created: 2021-09-12T22:01:23Z date_published: 2021-08-27T00:00:00Z date_updated: 2025-04-14T07:46:58Z day: '27' ddc: - '570' department: - _id: CaHe doi: 10.7554/eLife.66483 ec_funded: 1 external_id: isi: - '000700428500001' pmid: - '34448451' file: - access_level: open_access checksum: a3f82b0499cc822ac1eab48a01f3f57e content_type: application/pdf creator: dernst date_created: 2022-05-13T08:03:37Z date_updated: 2022-05-13T08:03:37Z file_id: '11371' file_name: 2021_eLife_Pulgar.pdf file_size: 9010446 relation: main_file success: 1 file_date_updated: 2022-05-13T08:03:37Z has_accepted_license: '1' intvolume: ' 10' isi: 1 keyword: - cell delamination - apical constriction - dragging - mechanical forces - collective 18 locomotion - dorsal forerunner cells - zebrafish language: - iso: eng month: '08' oa: 1 oa_version: Published Version pmid: 1 project: - _id: 260F1432-B435-11E9-9278-68D0E5697425 call_identifier: H2020 grant_number: '742573' name: Interaction and feedback between cell mechanics and fate specification in vertebrate gastrulation publication: eLife publication_identifier: eissn: - 2050-084X publication_status: published publisher: eLife Sciences Publications quality_controlled: '1' scopus_import: '1' status: public title: Apical contacts stemming from incomplete delamination guide progenitor cell allocation through a dragging mechanism tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8 volume: 10 year: '2021' ... --- _id: '17384' abstract: - lang: eng text: Basket weaving is a traditional craft for creating curved surfaces as an interwoven array of thin, flexible, and initially straight ribbons. The three-dimensional shape of a woven structure emerges through a complex interplay of the elastic bending behavior of the ribbons and the contact forces at their crossings. Curvature can be injected by carefully placing topological singularities in the otherwise regular weaving pattern. However, shape control through topology is highly non-trivial and inherently discrete, which severely limits the range of attainable woven geometries. Here, we demonstrate how to construct arbitrary smooth free-form surface geometries by weaving carefully optimized curved ribbons. We present an optimization-based approach to solving the inverse design problem for such woven structures. Our algorithm computes the ribbons' planar geometry such that their interwoven assembly closely approximates a given target design surface in equilibrium. We systematically validate our approach through a series of physical prototypes to show a broad range of new woven geometries that is not achievable by existing methods. We anticipate our computational approach to significantly enhance the capabilities for the design of new woven structures. Facilitated by modern digital fabrication technology, we see potential applications in material science, bio- and mechanical engineering, art, design, and architecture. article_processing_charge: No article_type: original author: - first_name: Yingying full_name: Ren, Yingying id: 93d68d10-3540-11ef-a265-f748a50dba3d last_name: Ren - first_name: Julian full_name: Panetta, Julian last_name: Panetta - first_name: Tian full_name: Chen, Tian last_name: Chen - first_name: Florin full_name: Isvoranu, Florin last_name: Isvoranu - first_name: Samuel full_name: Poincloux, Samuel last_name: Poincloux - first_name: Christopher full_name: Brandt, Christopher last_name: Brandt - first_name: Alison full_name: Martin, Alison last_name: Martin - first_name: Mark full_name: Pauly, Mark last_name: Pauly citation: ama: Ren Y, Panetta J, Chen T, et al. 3D weaving with curved ribbons. ACM Transactions on Graphics. 2021;40(4):1-15. doi:10.1145/3450626.3459788 apa: Ren, Y., Panetta, J., Chen, T., Isvoranu, F., Poincloux, S., Brandt, C., … Pauly, M. (2021). 3D weaving with curved ribbons. ACM Transactions on Graphics. Association for Computing Machinery. https://doi.org/10.1145/3450626.3459788 chicago: Ren, Yingying, Julian Panetta, Tian Chen, Florin Isvoranu, Samuel Poincloux, Christopher Brandt, Alison Martin, and Mark Pauly. “3D Weaving with Curved Ribbons.” ACM Transactions on Graphics. Association for Computing Machinery, 2021. https://doi.org/10.1145/3450626.3459788. ieee: Y. Ren et al., “3D weaving with curved ribbons,” ACM Transactions on Graphics, vol. 40, no. 4. Association for Computing Machinery, pp. 1–15, 2021. ista: Ren Y, Panetta J, Chen T, Isvoranu F, Poincloux S, Brandt C, Martin A, Pauly M. 2021. 3D weaving with curved ribbons. ACM Transactions on Graphics. 40(4), 1–15. mla: Ren, Yingying, et al. “3D Weaving with Curved Ribbons.” ACM Transactions on Graphics, vol. 40, no. 4, Association for Computing Machinery, 2021, pp. 1–15, doi:10.1145/3450626.3459788. short: Y. Ren, J. Panetta, T. Chen, F. Isvoranu, S. Poincloux, C. Brandt, A. Martin, M. Pauly, ACM Transactions on Graphics 40 (2021) 1–15. date_created: 2024-08-05T06:30:27Z date_published: 2021-08-01T00:00:00Z date_updated: 2024-08-12T09:38:19Z day: '01' doi: 10.1145/3450626.3459788 extern: '1' intvolume: ' 40' issue: '4' language: - iso: eng month: '08' oa_version: None page: 1-15 publication: ACM Transactions on Graphics publication_identifier: eissn: - 1557-7368 issn: - 0730-0301 publication_status: published publisher: Association for Computing Machinery quality_controlled: '1' scopus_import: '1' status: public title: 3D weaving with curved ribbons type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 40 year: '2021' ... --- _id: '17422' abstract: - lang: eng text: Inspired by motion patterns of some commercially available mobile robots, we investigate the power of robots that move forward in straight lines until colliding with an environment boundary, at which point they can rotate in place and move forward again; we visualize this as the robot “bouncing” off boundaries. We define bounce rules governing how the robot should reorient after reaching a boundary, such as reorienting relative to its heading prior to collision, or relative to the normal of the boundary. We then generate plans as sequences of rules, using the bounce visibility graph generated from a polygonal environment definition, while assuming we have unavoidable non-determinism in our actuation. Our planner can be queried to determine the feasibility of tasks such as reaching goal sets and patrolling (repeatedly visiting a sequence of goals). If the task is found feasible, the planner provides a sequence of non-deterministic interaction rules, which also provide information on how precisely the robot must execute the plan to succeed. We also show how to compute stable cyclic trajectories and use these to limit uncertainty in the robot’s position. article_processing_charge: No article_type: original author: - first_name: Alexandra Q full_name: Nilles, Alexandra Q last_name: Nilles - first_name: Yingying full_name: Ren, Yingying id: 93d68d10-3540-11ef-a265-f748a50dba3d last_name: Ren - first_name: Israel full_name: Becerra, Israel last_name: Becerra - first_name: Steven M full_name: LaValle, Steven M last_name: LaValle citation: ama: Nilles AQ, Ren Y, Becerra I, LaValle SM. A visibility-based approach to computing non-deterministic bouncing strategies. The International Journal of Robotics Research. 2021;40(10-11):1196-1211. doi:10.1177/0278364921992788 apa: Nilles, A. Q., Ren, Y., Becerra, I., & LaValle, S. M. (2021). A visibility-based approach to computing non-deterministic bouncing strategies. The International Journal of Robotics Research. SAGE Publications. https://doi.org/10.1177/0278364921992788 chicago: Nilles, Alexandra Q, Yingying Ren, Israel Becerra, and Steven M LaValle. “A Visibility-Based Approach to Computing Non-Deterministic Bouncing Strategies.” The International Journal of Robotics Research. SAGE Publications, 2021. https://doi.org/10.1177/0278364921992788. ieee: A. Q. Nilles, Y. Ren, I. Becerra, and S. M. LaValle, “A visibility-based approach to computing non-deterministic bouncing strategies,” The International Journal of Robotics Research, vol. 40, no. 10–11. SAGE Publications, pp. 1196–1211, 2021. ista: Nilles AQ, Ren Y, Becerra I, LaValle SM. 2021. A visibility-based approach to computing non-deterministic bouncing strategies. The International Journal of Robotics Research. 40(10–11), 1196–1211. mla: Nilles, Alexandra Q., et al. “A Visibility-Based Approach to Computing Non-Deterministic Bouncing Strategies.” The International Journal of Robotics Research, vol. 40, no. 10–11, SAGE Publications, 2021, pp. 1196–211, doi:10.1177/0278364921992788. short: A.Q. Nilles, Y. Ren, I. Becerra, S.M. LaValle, The International Journal of Robotics Research 40 (2021) 1196–1211. date_created: 2024-08-12T10:01:27Z date_published: 2021-09-01T00:00:00Z date_updated: 2024-08-12T10:15:14Z day: '01' doi: 10.1177/0278364921992788 extern: '1' intvolume: ' 40' issue: 10-11 language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1177/0278364921992788 month: '09' oa: 1 oa_version: Published Version page: 1196-1211 publication: The International Journal of Robotics Research publication_identifier: eissn: - 1741-3176 issn: - 0278-3649 publication_status: published publisher: SAGE Publications quality_controlled: '1' scopus_import: '1' status: public title: A visibility-based approach to computing non-deterministic bouncing strategies type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 40 year: '2021' ... --- _id: '17505' abstract: - lang: eng text: "Given the central role that C continues to play in systems software, and the difficulty of writing safe and correct C code, it remains a grand challenge to develop effective formal methods for verifying C programs. In this paper, we propose a new approach to this problem: a type system we call RefinedC, which combines ownership types (for modular reasoning about shared state and concurrency) with refinement types (for encoding precise invariants on C data types and Hoare-style specifications for C functions).\r\nRefinedC is both automated (requiring minimal user intervention) and foundational (producing a proof of program correctness in Coq), while at the same time handling a range of low-level programming idioms such as pointer arithmetic. In particular, following the approach of RustBelt, the soundness of the RefinedC type system is justified semantically by interpretation into the Coq-based Iris framework for higher-order concurrent separation logic. However, the typing rules of RefinedC are also designed to be encodable in a new “separation logic programming” language we call Lithium. By restricting to a carefully chosen (yet expressive) fragment of separation logic, Lithium supports predictable, automatic, goal-directed proof search without backtracking. We demonstrate the effectiveness of RefinedC on a range of representative examples of C code." article_processing_charge: No author: - first_name: Michael Joachim full_name: Sammler, Michael Joachim id: 510d3901-2a03-11ee-914d-d9ae9011f0a7 last_name: Sammler - first_name: Rodolphe full_name: Lepigre, Rodolphe last_name: Lepigre - first_name: Robbert full_name: Krebbers, Robbert last_name: Krebbers - first_name: Kayvan full_name: Memarian, Kayvan last_name: Memarian - first_name: Derek full_name: Dreyer, Derek last_name: Dreyer - first_name: Deepak full_name: Garg, Deepak last_name: Garg citation: ama: 'Sammler MJ, Lepigre R, Krebbers R, Memarian K, Dreyer D, Garg D. RefinedC: Automating the foundational verification of C code with refined ownership types. In: Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation. Association for Computing Machinery; 2021:158-174. doi:10.1145/3453483.3454036' apa: 'Sammler, M. J., Lepigre, R., Krebbers, R., Memarian, K., Dreyer, D., & Garg, D. (2021). RefinedC: Automating the foundational verification of C code with refined ownership types. In Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation (pp. 158–174). virtual: Association for Computing Machinery. https://doi.org/10.1145/3453483.3454036' chicago: 'Sammler, Michael Joachim, Rodolphe Lepigre, Robbert Krebbers, Kayvan Memarian, Derek Dreyer, and Deepak Garg. “RefinedC: Automating the Foundational Verification of C Code with Refined Ownership Types.” In Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation, 158–74. Association for Computing Machinery, 2021. https://doi.org/10.1145/3453483.3454036.' ieee: 'M. J. Sammler, R. Lepigre, R. Krebbers, K. Memarian, D. Dreyer, and D. Garg, “RefinedC: Automating the foundational verification of C code with refined ownership types,” in Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation, virtual, 2021, pp. 158–174.' ista: 'Sammler MJ, Lepigre R, Krebbers R, Memarian K, Dreyer D, Garg D. 2021. RefinedC: Automating the foundational verification of C code with refined ownership types. Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation. PLDI: Conference on Programming Language Design and Implementation, 158–174.' mla: 'Sammler, Michael Joachim, et al. “RefinedC: Automating the Foundational Verification of C Code with Refined Ownership Types.” Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation, Association for Computing Machinery, 2021, pp. 158–74, doi:10.1145/3453483.3454036.' short: M.J. Sammler, R. Lepigre, R. Krebbers, K. Memarian, D. Dreyer, D. Garg, in:, Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation, Association for Computing Machinery, 2021, pp. 158–174. conference: end_date: 2021-06-25 location: virtual name: 'PLDI: Conference on Programming Language Design and Implementation' start_date: 2021-06-20 date_created: 2024-09-05T08:34:50Z date_published: 2021-06-18T00:00:00Z date_updated: 2024-09-10T11:54:22Z day: '18' doi: 10.1145/3453483.3454036 extern: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1145/3453483.3454036 month: '06' oa: 1 oa_version: Published Version page: 158-174 publication: Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation publication_status: published publisher: Association for Computing Machinery quality_controlled: '1' scopus_import: '1' status: public title: 'RefinedC: Automating the foundational verification of C code with refined ownership types' type: conference user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 year: '2021' ... --- _id: '17508' abstract: - lang: eng text: "This paper presents the ESA Voyage 2050 White Paper for a concept of TeraHertz Exploration and Zooming-in for Astrophysics (THEZA). It addresses the science case and some implementation issues of a space-borne radio interferometric system for ultra-sharp imaging of celestial radio sources at the level of angular resolution down to (sub-) microarcseconds. THEZA focuses at millimetre and sub-millimetre wavelengths (frequencies above \r\n300 GHz), but allows for science operations at longer wavelengths too. The THEZA concept science rationale is focused on the physics of spacetime in the vicinity of supermassive black holes as the leading science driver. The main aim of the concept is to facilitate a major leap by providing researchers with orders of magnitude improvements in the resolution and dynamic range in direct imaging studies of the most exotic objects in the Universe, black holes. The concept will open up a sizeable range of hitherto unreachable parameters of observational astrophysics. It unifies two major lines of development of space-borne radio astronomy of the past decades: Space VLBI (Very Long Baseline Interferometry) and mm- and sub-mm astrophysical studies with “single dish” instruments. It also builds upon the recent success of the Earth-based Event Horizon Telescope (EHT) – the first-ever direct image of a shadow of the super-massive black hole in the centre of the galaxy M87. As an amalgam of these three major areas of modern observational astrophysics, THEZA aims at facilitating a breakthrough in high-resolution high image quality studies in the millimetre and sub-millimetre domain of the electromagnetic spectrum." alternative_title: - An ESA Voyage 2050 White Paper article_processing_charge: No article_type: original author: - first_name: Leonid I. full_name: Gurvits, Leonid I. last_name: Gurvits - first_name: Zsolt full_name: Paragi, Zsolt last_name: Paragi - first_name: Viviana full_name: Casasola, Viviana last_name: Casasola - first_name: John full_name: Conway, John last_name: Conway - first_name: Jordy full_name: Davelaar, Jordy last_name: Davelaar - first_name: Heino full_name: Falcke, Heino last_name: Falcke - first_name: Rob full_name: Fender, Rob last_name: Fender - first_name: Sándor full_name: Frey, Sándor last_name: Frey - first_name: Christian M. full_name: Fromm, Christian M. last_name: Fromm - first_name: Cristina García full_name: Miró, Cristina García last_name: Miró - first_name: Michael A. full_name: Garrett, Michael A. last_name: Garrett - first_name: Marcello full_name: Giroletti, Marcello last_name: Giroletti - first_name: Ciriaco full_name: Goddi, Ciriaco last_name: Goddi - first_name: José-Luis full_name: Gómez, José-Luis last_name: Gómez - first_name: Jeffrey full_name: van der Gucht, Jeffrey last_name: van der Gucht - first_name: José Carlos full_name: Guirado, José Carlos last_name: Guirado - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Frank full_name: Helmich, Frank last_name: Helmich - first_name: Elizabeth full_name: Humphreys, Elizabeth last_name: Humphreys - first_name: Violette full_name: Impellizzeri, Violette last_name: Impellizzeri - first_name: Michael full_name: Kramer, Michael last_name: Kramer - first_name: Michael full_name: Lindqvist, Michael last_name: Lindqvist - first_name: Hendrik full_name: Linz, Hendrik last_name: Linz - first_name: Elisabetta full_name: Liuzzo, Elisabetta last_name: Liuzzo - first_name: Andrei P. full_name: Lobanov, Andrei P. last_name: Lobanov - first_name: Yosuke full_name: Mizuno, Yosuke last_name: Mizuno - first_name: Luciano full_name: Rezzolla, Luciano last_name: Rezzolla - first_name: Freek full_name: Roelofs, Freek last_name: Roelofs - first_name: Eduardo full_name: Ros, Eduardo last_name: Ros - first_name: Kazi L.J. full_name: Rygl, Kazi L.J. last_name: Rygl - first_name: Tuomas full_name: Savolainen, Tuomas last_name: Savolainen - first_name: Karl full_name: Schuster, Karl last_name: Schuster - first_name: Tiziana full_name: Venturi, Tiziana last_name: Venturi - first_name: Martina C. full_name: Wiedner, Martina C. last_name: Wiedner - first_name: J. Anton full_name: Zensus, J. Anton last_name: Zensus citation: ama: 'Gurvits LI, Paragi Z, Casasola V, et al. THEZA: TeraHertz exploration and zooming-in for astrophysics. Experimental Astronomy. 2021;51(3):559-594. doi:10.1007/s10686-021-09714-y' apa: 'Gurvits, L. I., Paragi, Z., Casasola, V., Conway, J., Davelaar, J., Falcke, H., … Zensus, J. A. (2021). THEZA: TeraHertz exploration and zooming-in for astrophysics. Experimental Astronomy. Springer Science and Business Media LLC. https://doi.org/10.1007/s10686-021-09714-y' chicago: 'Gurvits, Leonid I., Zsolt Paragi, Viviana Casasola, John Conway, Jordy Davelaar, Heino Falcke, Rob Fender, et al. “THEZA: TeraHertz Exploration and Zooming-in for Astrophysics.” Experimental Astronomy. Springer Science and Business Media LLC, 2021. https://doi.org/10.1007/s10686-021-09714-y.' ieee: 'L. I. Gurvits et al., “THEZA: TeraHertz exploration and zooming-in for astrophysics,” Experimental Astronomy, vol. 51, no. 3. Springer Science and Business Media LLC, pp. 559–594, 2021.' ista: 'Gurvits LI, Paragi Z, Casasola V, Conway J, Davelaar J, Falcke H, Fender R, Frey S, Fromm CM, Miró CG, Garrett MA, Giroletti M, Goddi C, Gómez J-L, van der Gucht J, Guirado JC, Haiman Z, Helmich F, Humphreys E, Impellizzeri V, Kramer M, Lindqvist M, Linz H, Liuzzo E, Lobanov AP, Mizuno Y, Rezzolla L, Roelofs F, Ros E, Rygl KLJ, Savolainen T, Schuster K, Venturi T, Wiedner MC, Zensus JA. 2021. THEZA: TeraHertz exploration and zooming-in for astrophysics. Experimental Astronomy. 51(3), 559–594.' mla: 'Gurvits, Leonid I., et al. “THEZA: TeraHertz Exploration and Zooming-in for Astrophysics.” Experimental Astronomy, vol. 51, no. 3, Springer Science and Business Media LLC, 2021, pp. 559–94, doi:10.1007/s10686-021-09714-y.' short: L.I. Gurvits, Z. Paragi, V. Casasola, J. Conway, J. Davelaar, H. Falcke, R. Fender, S. Frey, C.M. Fromm, C.G. Miró, M.A. Garrett, M. Giroletti, C. Goddi, J.-L. Gómez, J. van der Gucht, J.C. Guirado, Z. Haiman, F. Helmich, E. Humphreys, V. Impellizzeri, M. Kramer, M. Lindqvist, H. Linz, E. Liuzzo, A.P. Lobanov, Y. Mizuno, L. Rezzolla, F. Roelofs, E. Ros, K.L.J. Rygl, T. Savolainen, K. Schuster, T. Venturi, M.C. Wiedner, J.A. Zensus, Experimental Astronomy 51 (2021) 559–594. date_created: 2024-09-05T08:46:17Z date_published: 2021-05-27T00:00:00Z date_updated: 2024-09-10T12:15:42Z day: '27' doi: 10.1007/s10686-021-09714-y extern: '1' intvolume: ' 51' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1007/s10686-021-09714-y month: '05' oa: 1 oa_version: Published Version page: 559-594 publication: Experimental Astronomy publication_identifier: issn: - 0922-6435 - 1572-9508 publication_status: published publisher: Springer Science and Business Media LLC quality_controlled: '1' scopus_import: '1' status: public title: 'THEZA: TeraHertz exploration and zooming-in for astrophysics' type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 51 year: '2021' ... --- _id: '17509' abstract: - lang: eng text: The recently discovered gravitational wave sources GW190521 and GW190814 have shown evidence of BH mergers with masses and spins outside of the range expected from isolated stellar evolution. These merging objects could have undergone previous mergers. Such hierarchical mergers are predicted to be frequent in active galactic nuclei (AGNs) disks, where binaries form and evolve efficiently by dynamical interactions and gaseous dissipation. Here we compare the properties of these observed events to the theoretical models of mergers in AGN disks, which are obtained by performing one-dimensional N-body simulations combined with semi-analytical prescriptions. The high BH masses in GW190521 are consistent with mergers of high-generation (high-g) BHs where the initial progenitor stars had high metallicity, 2g BHs if the original progenitors were metal-poor, or 1g BHs that had gained mass via super-Eddington accretion. Other measured properties related to spin parameters in GW190521 are also consistent with mergers in AGN disks. Furthermore, mergers in the lower mass gap or those with low mass ratio as found in GW190814 and GW190412 are also reproduced by mergers of 2g–1g or 1g–1g objects with significant accretion in AGN disks. Finally, due to gas accretion, the massive neutron star merger reported in GW190425 can be produced in an AGN disk. article_number: '194' article_processing_charge: No article_type: original author: - first_name: Hiromichi full_name: Tagawa, Hiromichi last_name: Tagawa - first_name: Bence full_name: Kocsis, Bence last_name: Kocsis - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Imre full_name: Bartos, Imre last_name: Bartos - first_name: Kazuyuki full_name: Omukai, Kazuyuki last_name: Omukai - first_name: Johan full_name: Samsing, Johan last_name: Samsing citation: ama: Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. Mass-gap mergers in active galactic nuclei. The Astrophysical Journal. 2021;908(2). doi:10.3847/1538-4357/abd555 apa: Tagawa, H., Kocsis, B., Haiman, Z., Bartos, I., Omukai, K., & Samsing, J. (2021). Mass-gap mergers in active galactic nuclei. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/abd555 chicago: Tagawa, Hiromichi, Bence Kocsis, Zoltán Haiman, Imre Bartos, Kazuyuki Omukai, and Johan Samsing. “Mass-Gap Mergers in Active Galactic Nuclei.” The Astrophysical Journal. American Astronomical Society, 2021. https://doi.org/10.3847/1538-4357/abd555. ieee: H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, and J. Samsing, “Mass-gap mergers in active galactic nuclei,” The Astrophysical Journal, vol. 908, no. 2. American Astronomical Society, 2021. ista: Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. 2021. Mass-gap mergers in active galactic nuclei. The Astrophysical Journal. 908(2), 194. mla: Tagawa, Hiromichi, et al. “Mass-Gap Mergers in Active Galactic Nuclei.” The Astrophysical Journal, vol. 908, no. 2, 194, American Astronomical Society, 2021, doi:10.3847/1538-4357/abd555. short: H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, J. Samsing, The Astrophysical Journal 908 (2021). date_created: 2024-09-05T08:47:46Z date_published: 2021-02-24T00:00:00Z date_updated: 2024-09-10T12:36:17Z day: '24' doi: 10.3847/1538-4357/abd555 extern: '1' intvolume: ' 908' issue: '2' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3847/1538-4357/abd555 month: '02' oa: 1 oa_version: Published Version publication: The Astrophysical Journal publication_identifier: issn: - 0004-637X - 1538-4357 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: Mass-gap mergers in active galactic nuclei type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 908 year: '2021' ... --- _id: '17515' abstract: - lang: eng text: 'The disks of active galactic nuclei (AGNs) have emerged as a rich environment for the evolution of stars and their compact remnants. The very dense medium favors rapid accretion, while torques and migration traps enhance binary formation and mergers. Both long and short gamma-ray bursts are hence expected. We show that AGN disks constitute an ideal environment for another interesting phenomenon: the accretion-induced collapse (AIC) of neutron stars (NSs) to black holes (BHs). Rapid accretion in the dense disks can cause NSs to grow to the point of exceeding the maximum mass allowed by their equation of state. General relativistic magnetohydrodynamical simulations have shown that electromagnetic signatures are expected if the NS is surrounded by a minidisk prior to collapse, which then rapidly accretes onto the BH, and/or if the NS is highly magnetized, from reconnection of the magnetosphere during collapse. Here we compute the rates of AICs and their locations within the disks for both isolated NSs and for (initially stable) NSs formed from NS-NS mergers. We find that the global AIC rates are ∼0.07–20 Gpc−3 yr−1, and we discuss their observable prospects and signatures as they emerge from the dense disk environments.' article_number: '10' article_processing_charge: No article_type: original author: - first_name: Rosalba full_name: Perna, Rosalba last_name: Perna - first_name: Hiromichi full_name: Tagawa, Hiromichi last_name: Tagawa - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Imre full_name: Bartos, Imre last_name: Bartos citation: ama: Perna R, Tagawa H, Haiman Z, Bartos I. Accretion-induced collapse of neutron stars in the disks of active galactic nuclei. The Astrophysical Journal. 2021;915(1). doi:10.3847/1538-4357/abfdb4 apa: Perna, R., Tagawa, H., Haiman, Z., & Bartos, I. (2021). Accretion-induced collapse of neutron stars in the disks of active galactic nuclei. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/abfdb4 chicago: Perna, Rosalba, Hiromichi Tagawa, Zoltán Haiman, and Imre Bartos. “Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei.” The Astrophysical Journal. American Astronomical Society, 2021. https://doi.org/10.3847/1538-4357/abfdb4. ieee: R. Perna, H. Tagawa, Z. Haiman, and I. Bartos, “Accretion-induced collapse of neutron stars in the disks of active galactic nuclei,” The Astrophysical Journal, vol. 915, no. 1. American Astronomical Society, 2021. ista: Perna R, Tagawa H, Haiman Z, Bartos I. 2021. Accretion-induced collapse of neutron stars in the disks of active galactic nuclei. The Astrophysical Journal. 915(1), 10. mla: Perna, Rosalba, et al. “Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei.” The Astrophysical Journal, vol. 915, no. 1, 10, American Astronomical Society, 2021, doi:10.3847/1538-4357/abfdb4. short: R. Perna, H. Tagawa, Z. Haiman, I. Bartos, The Astrophysical Journal 915 (2021). date_created: 2024-09-05T08:55:06Z date_published: 2021-06-28T00:00:00Z date_updated: 2024-09-10T13:47:31Z day: '28' doi: 10.3847/1538-4357/abfdb4 extern: '1' intvolume: ' 915' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3847/1538-4357/abfdb4 month: '06' oa: 1 oa_version: Published Version publication: The Astrophysical Journal publication_identifier: issn: - 0004-637X - 1538-4357 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: Accretion-induced collapse of neutron stars in the disks of active galactic nuclei type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 915 year: '2021' ... --- _id: '17516' abstract: - lang: eng text: We study the effect of baryonic processes on weak lensing (WL) observables with a suite of mock WL maps, the κTNG, based on the cosmological hydrodynamic simulations IllustrisTNG. We quantify the baryonic effects on the WL angular power spectrum, one-point probability distribution function (PDF), and number counts of peaks and minima. We also show the redshift evolution of the effects, which is a key to distinguish the effect of baryons from fundamental physics such as dark energy, dark matter, and massive neutrinos. We find that baryonic processes reduce the small-scale power, suppress the tails of the PDF, peak and minimum counts, and change the total number of peaks and minima. We compare our results to existing semi-analytical models and hydrodynamic simulations, and discuss the source of discrepancies. The κTNG suite includes 10 000 realizations of $5 \times 5 \, \mathrm{deg}^2$ maps for 40 source redshifts up to zs = 2.6, well covering the range of interest for existing and upcoming WL surveys. We also produce the κTNG-Dark suite of maps, generated based on the corresponding dark matter-only IllustrisTNG simulations. Our mock maps are not only suitable for developing analytical models that incorporate the effect of baryons, but also particularly useful for studies that rely on mass maps, such as non-Gaussian statistics and machine learning with convolutional neural networks. The suite of mock maps is publicly available at Columbia Lensing (http://columbialensing.org). article_processing_charge: No article_type: original author: - first_name: Ken full_name: Osato, Ken last_name: Osato - first_name: Jia full_name: Liu, Jia last_name: Liu - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: 'Osato K, Liu J, Haiman Z. κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations. Monthly Notices of the Royal Astronomical Society. 2021;502(4):5593-5602. doi:10.1093/mnras/stab395' apa: 'Osato, K., Liu, J., & Haiman, Z. (2021). κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stab395' chicago: 'Osato, Ken, Jia Liu, and Zoltán Haiman. “ΚTNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2021. https://doi.org/10.1093/mnras/stab395.' ieee: 'K. Osato, J. Liu, and Z. Haiman, “κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations,” Monthly Notices of the Royal Astronomical Society, vol. 502, no. 4. Oxford University Press, pp. 5593–5602, 2021.' ista: 'Osato K, Liu J, Haiman Z. 2021. κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations. Monthly Notices of the Royal Astronomical Society. 502(4), 5593–5602.' mla: 'Osato, Ken, et al. “ΚTNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations.” Monthly Notices of the Royal Astronomical Society, vol. 502, no. 4, Oxford University Press, 2021, pp. 5593–602, doi:10.1093/mnras/stab395.' short: K. Osato, J. Liu, Z. Haiman, Monthly Notices of the Royal Astronomical Society 502 (2021) 5593–5602. date_created: 2024-09-05T08:56:14Z date_published: 2021-02-11T00:00:00Z date_updated: 2024-09-10T13:53:06Z day: '11' doi: 10.1093/mnras/stab395 extern: '1' intvolume: ' 502' issue: '4' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stab395 month: '02' oa: 1 oa_version: Published Version page: 5593-5602 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: 'κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations' type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 502 year: '2021' ... --- _id: '17525' abstract: - lang: eng text: Since the very beginning of astronomy the location of objects on the sky has been a fundamental observational quantity that has been taken for granted. While precise two dimensional positional information is easy to obtain for observations in the electromagnetic spectrum, the positional accuracy of current and near future gravitational wave detectors is limited to between tens and hundreds of square degrees, which makes it extremely challenging to identify the host galaxies of gravitational wave events or to detect any electromagnetic counterparts. Gravitational wave observations provide information on source properties that is complementary to the information in any associated electromagnetic emission. Observing systems with multiple messengers thus has scientific potential much greater than the sum of its parts. A gravitational wave detector with higher angular resolution would significantly increase the prospects for finding the hosts of gravitational wave sources and triggering a multi-messenger follow-up campaign. An observatory with arcminute precision or better could be realised within the Voyage 2050 programme by creating a large baseline interferometer array in space and would have transformative scientific potential. Precise positional information of standard sirens would enable precision measurements of cosmological parameters and offer new insights on structure formation; a high angular resolution gravitational wave observatory would allow the detection of a stochastic background and resolution of the anisotropies within it; it would also allow the study of accretion processes around black holes; and it would have tremendous potential for tests of modified gravity and the discovery of physics beyond the Standard Model. article_processing_charge: No article_type: original author: - first_name: John full_name: Baker, John last_name: Baker - first_name: Tessa full_name: Baker, Tessa last_name: Baker - first_name: Carmelita full_name: Carbone, Carmelita last_name: Carbone - first_name: Giuseppe full_name: Congedo, Giuseppe last_name: Congedo - first_name: Carlo full_name: Contaldi, Carlo last_name: Contaldi - first_name: Irina full_name: Dvorkin, Irina last_name: Dvorkin - first_name: Jonathan full_name: Gair, Jonathan last_name: Gair - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: David F. full_name: Mota, David F. last_name: Mota - first_name: Arianna full_name: Renzini, Arianna last_name: Renzini - first_name: Ernst-Jan full_name: Buis, Ernst-Jan last_name: Buis - first_name: Giulia full_name: Cusin, Giulia last_name: Cusin - first_name: Jose Maria full_name: Ezquiaga, Jose Maria last_name: Ezquiaga - first_name: Guido full_name: Mueller, Guido last_name: Mueller - first_name: Mauro full_name: Pieroni, Mauro last_name: Pieroni - first_name: John full_name: Quenby, John last_name: Quenby - first_name: Angelo full_name: Ricciardone, Angelo last_name: Ricciardone - first_name: Ippocratis D. full_name: Saltas, Ippocratis D. last_name: Saltas - first_name: Lijing full_name: Shao, Lijing last_name: Shao - first_name: Nicola full_name: Tamanini, Nicola last_name: Tamanini - first_name: Gianmassimo full_name: Tasinato, Gianmassimo last_name: Tasinato - first_name: Miguel full_name: Zumalacárregui, Miguel last_name: Zumalacárregui citation: ama: Baker J, Baker T, Carbone C, et al. High angular resolution gravitational wave astronomy. Experimental Astronomy. 2021;51(3):1441-1470. doi:10.1007/s10686-021-09712-0 apa: Baker, J., Baker, T., Carbone, C., Congedo, G., Contaldi, C., Dvorkin, I., … Zumalacárregui, M. (2021). High angular resolution gravitational wave astronomy. Experimental Astronomy. Springer Science and Business Media LLC. https://doi.org/10.1007/s10686-021-09712-0 chicago: Baker, John, Tessa Baker, Carmelita Carbone, Giuseppe Congedo, Carlo Contaldi, Irina Dvorkin, Jonathan Gair, et al. “High Angular Resolution Gravitational Wave Astronomy.” Experimental Astronomy. Springer Science and Business Media LLC, 2021. https://doi.org/10.1007/s10686-021-09712-0. ieee: J. Baker et al., “High angular resolution gravitational wave astronomy,” Experimental Astronomy, vol. 51, no. 3. Springer Science and Business Media LLC, pp. 1441–1470, 2021. ista: Baker J, Baker T, Carbone C, Congedo G, Contaldi C, Dvorkin I, Gair J, Haiman Z, Mota DF, Renzini A, Buis E-J, Cusin G, Ezquiaga JM, Mueller G, Pieroni M, Quenby J, Ricciardone A, Saltas ID, Shao L, Tamanini N, Tasinato G, Zumalacárregui M. 2021. High angular resolution gravitational wave astronomy. Experimental Astronomy. 51(3), 1441–1470. mla: Baker, John, et al. “High Angular Resolution Gravitational Wave Astronomy.” Experimental Astronomy, vol. 51, no. 3, Springer Science and Business Media LLC, 2021, pp. 1441–70, doi:10.1007/s10686-021-09712-0. short: J. Baker, T. Baker, C. Carbone, G. Congedo, C. Contaldi, I. Dvorkin, J. Gair, Z. Haiman, D.F. Mota, A. Renzini, E.-J. Buis, G. Cusin, J.M. Ezquiaga, G. Mueller, M. Pieroni, J. Quenby, A. Ricciardone, I.D. Saltas, L. Shao, N. Tamanini, G. Tasinato, M. Zumalacárregui, Experimental Astronomy 51 (2021) 1441–1470. date_created: 2024-09-05T09:28:30Z date_published: 2021-05-04T00:00:00Z date_updated: 2024-09-11T08:17:16Z day: '04' doi: 10.1007/s10686-021-09712-0 extern: '1' intvolume: ' 51' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1007/s10686-021-09712-0 month: '05' oa: 1 oa_version: Published Version page: 1441-1470 publication: Experimental Astronomy publication_identifier: issn: - 0922-6435 - 1572-9508 publication_status: published publisher: Springer Science and Business Media LLC quality_controlled: '1' scopus_import: '1' status: public title: High angular resolution gravitational wave astronomy type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 51 year: '2021' ... --- _id: '17534' abstract: - lang: eng text: We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a μ-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe. article_processing_charge: No article_type: original author: - first_name: Alberto full_name: Sesana, Alberto last_name: Sesana - first_name: Natalia full_name: Korsakova, Natalia last_name: Korsakova - first_name: Manuel Arca full_name: Sedda, Manuel Arca last_name: Sedda - first_name: Vishal full_name: Baibhav, Vishal last_name: Baibhav - first_name: Enrico full_name: Barausse, Enrico last_name: Barausse - first_name: Simon full_name: Barke, Simon last_name: Barke - first_name: Emanuele full_name: Berti, Emanuele last_name: Berti - first_name: Matteo full_name: Bonetti, Matteo last_name: Bonetti - first_name: Pedro R. full_name: Capelo, Pedro R. last_name: Capelo - first_name: Chiara full_name: Caprini, Chiara last_name: Caprini - first_name: Juan full_name: Garcia-Bellido, Juan last_name: Garcia-Bellido - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Karan full_name: Jani, Karan last_name: Jani - first_name: Oliver full_name: Jennrich, Oliver last_name: Jennrich - first_name: Peter H. full_name: Johansson, Peter H. last_name: Johansson - first_name: Fazeel Mahmood full_name: Khan, Fazeel Mahmood last_name: Khan - first_name: Valeriya full_name: Korol, Valeriya last_name: Korol - first_name: Astrid full_name: Lamberts, Astrid last_name: Lamberts - first_name: Alessandro full_name: Lupi, Alessandro last_name: Lupi - first_name: Alberto full_name: Mangiagli, Alberto last_name: Mangiagli - first_name: Lucio full_name: Mayer, Lucio last_name: Mayer - first_name: Germano full_name: Nardini, Germano last_name: Nardini - first_name: Fabio full_name: Pacucci, Fabio last_name: Pacucci - first_name: Antoine full_name: Petiteau, Antoine last_name: Petiteau - first_name: Alvise full_name: Raccanelli, Alvise last_name: Raccanelli - first_name: Surjeet full_name: Rajendran, Surjeet last_name: Rajendran - first_name: John full_name: Regan, John last_name: Regan - first_name: Lijing full_name: Shao, Lijing last_name: Shao - first_name: Alessandro full_name: Spallicci, Alessandro last_name: Spallicci - first_name: Nicola full_name: Tamanini, Nicola last_name: Tamanini - first_name: Marta full_name: Volonteri, Marta last_name: Volonteri - first_name: Niels full_name: Warburton, Niels last_name: Warburton - first_name: Kaze full_name: Wong, Kaze last_name: Wong - first_name: Miguel full_name: Zumalacarregui, Miguel last_name: Zumalacarregui citation: ama: Sesana A, Korsakova N, Sedda MA, et al. Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy. 2021;51(3):1333-1383. doi:10.1007/s10686-021-09709-9 apa: Sesana, A., Korsakova, N., Sedda, M. A., Baibhav, V., Barausse, E., Barke, S., … Zumalacarregui, M. (2021). Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy. Springer Science and Business Media LLC. https://doi.org/10.1007/s10686-021-09709-9 chicago: Sesana, Alberto, Natalia Korsakova, Manuel Arca Sedda, Vishal Baibhav, Enrico Barausse, Simon Barke, Emanuele Berti, et al. “Unveiling the Gravitational Universe at μ-Hz Frequencies.” Experimental Astronomy. Springer Science and Business Media LLC, 2021. https://doi.org/10.1007/s10686-021-09709-9. ieee: A. Sesana et al., “Unveiling the gravitational universe at μ-Hz frequencies,” Experimental Astronomy, vol. 51, no. 3. Springer Science and Business Media LLC, pp. 1333–1383, 2021. ista: Sesana A, Korsakova N, Sedda MA, Baibhav V, Barausse E, Barke S, Berti E, Bonetti M, Capelo PR, Caprini C, Garcia-Bellido J, Haiman Z, Jani K, Jennrich O, Johansson PH, Khan FM, Korol V, Lamberts A, Lupi A, Mangiagli A, Mayer L, Nardini G, Pacucci F, Petiteau A, Raccanelli A, Rajendran S, Regan J, Shao L, Spallicci A, Tamanini N, Volonteri M, Warburton N, Wong K, Zumalacarregui M. 2021. Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy. 51(3), 1333–1383. mla: Sesana, Alberto, et al. “Unveiling the Gravitational Universe at μ-Hz Frequencies.” Experimental Astronomy, vol. 51, no. 3, Springer Science and Business Media LLC, 2021, pp. 1333–83, doi:10.1007/s10686-021-09709-9. short: A. Sesana, N. Korsakova, M.A. Sedda, V. Baibhav, E. Barausse, S. Barke, E. Berti, M. Bonetti, P.R. Capelo, C. Caprini, J. Garcia-Bellido, Z. Haiman, K. Jani, O. Jennrich, P.H. Johansson, F.M. Khan, V. Korol, A. Lamberts, A. Lupi, A. Mangiagli, L. Mayer, G. Nardini, F. Pacucci, A. Petiteau, A. Raccanelli, S. Rajendran, J. Regan, L. Shao, A. Spallicci, N. Tamanini, M. Volonteri, N. Warburton, K. Wong, M. Zumalacarregui, Experimental Astronomy 51 (2021) 1333–1383. date_created: 2024-09-05T09:42:29Z date_published: 2021-09-04T00:00:00Z date_updated: 2024-09-11T14:53:17Z day: '04' doi: 10.1007/s10686-021-09709-9 extern: '1' intvolume: ' 51' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1007/s10686-021-09709-9 month: '09' oa: 1 oa_version: Published Version page: 1333-1383 publication: Experimental Astronomy publication_identifier: issn: - 0922-6435 - 1572-9508 publication_status: published publisher: Springer Science and Business Media LLC quality_controlled: '1' scopus_import: '1' status: public title: Unveiling the gravitational universe at μ-Hz frequencies type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 51 year: '2021' ... --- _id: '17574' abstract: - lang: eng text: As weak lensing surveys are becoming deeper and cover larger areas, information will be available on small angular scales down to the arcmin level. To extract this extra information, accurate modelling of baryonic effects is necessary. In this work, we adopt a baryonic correction model, which includes gas both bound inside and ejected from dark matter (DM) haloes, a central galaxy, and changes in the DM profile induced by baryons. We use this model to incorporate baryons into a large suite of DM-only N-body simulations, covering a grid of 75 cosmologies in the Ωm–σ8 parameter space. We investigate how baryons affect Gaussian and non-Gaussian weak lensing statistics and the cosmological parameter inferences from these statistics. Our results show that marginalizing over baryonic parameters degrades the constraints in Ωm–σ8 space by a factor of 2–5 compared to those with baryonic parameters fixed. We also find that combining the lensing power spectrum and peak counts can break the degeneracy between cosmological and baryonic parameters and mitigate the impact of the uncertainty in baryonic physics. article_processing_charge: No article_type: original author: - first_name: Tianhuan full_name: Lu, Tianhuan last_name: Lu - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: Lu T, Haiman Z. The impact of baryons on cosmological inference from weak lensing statistics. Monthly Notices of the Royal Astronomical Society. 2021;506(3):3406-3417. doi:10.1093/mnras/stab1978 apa: Lu, T., & Haiman, Z. (2021). The impact of baryons on cosmological inference from weak lensing statistics. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stab1978 chicago: Lu, Tianhuan, and Zoltán Haiman. “The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2021. https://doi.org/10.1093/mnras/stab1978. ieee: T. Lu and Z. Haiman, “The impact of baryons on cosmological inference from weak lensing statistics,” Monthly Notices of the Royal Astronomical Society, vol. 506, no. 3. Oxford University Press, pp. 3406–3417, 2021. ista: Lu T, Haiman Z. 2021. The impact of baryons on cosmological inference from weak lensing statistics. Monthly Notices of the Royal Astronomical Society. 506(3), 3406–3417. mla: Lu, Tianhuan, and Zoltán Haiman. “The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics.” Monthly Notices of the Royal Astronomical Society, vol. 506, no. 3, Oxford University Press, 2021, pp. 3406–17, doi:10.1093/mnras/stab1978. short: T. Lu, Z. Haiman, Monthly Notices of the Royal Astronomical Society 506 (2021) 3406–3417. date_created: 2024-09-05T12:17:24Z date_published: 2021-07-10T00:00:00Z date_updated: 2024-09-19T07:43:16Z day: '10' doi: 10.1093/mnras/stab1978 extern: '1' intvolume: ' 506' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stab1978 month: '07' oa: 1 oa_version: Published Version page: 3406-3417 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: The impact of baryons on cosmological inference from weak lensing statistics type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 506 year: '2021' ... --- _id: '17577' abstract: - lang: eng text: 'The Legacy Survey of Space and Time (LSST) by the Vera C. Rubin Observatory is expected to discover tens of millions of quasars. A significant fraction of these could be powered by coalescing massive black hole (MBH) binaries, since many quasars are believed to be triggered by mergers. We show that under plausible assumptions about the luminosity functions, lifetimes, and binary fractions of quasars, we expect the full LSST quasar catalogue to contain between 20 and 100 million compact MBH binaries with masses M = 105–9M⊙, redshifts z = 0–6, and orbital periods P = 1–70 d. Their light-curves are expected to be distinctly periodic, which can be confidently distinguished from stochastic red-noise variability, because LSST will cover dozens, or even hundreds of cycles. A very small subset of 10–150 ultracompact (P ≲ 1 d) binary quasars among these will, over ∼5–15 yr, evolve into the mHz gravitational-wave frequency band and can be detected by LISA. They can therefore be regarded as ‘LISA verification binaries’, analogous to short-period Galactic compact-object binaries. The practical question is how to find these handful of ‘needles in the haystack’ among the large number of quasars: this will likely require a tailored co-adding analysis optimized for this purpose.' article_processing_charge: No article_type: original author: - first_name: Chengcheng full_name: Xin, Chengcheng last_name: Xin - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: Xin C, Haiman Z. Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries.’ Monthly Notices of the Royal Astronomical Society. 2021;506(2):2408-2417. doi:10.1093/mnras/stab1856 apa: Xin, C., & Haiman, Z. (2021). Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries.’ Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stab1856 chicago: Xin, Chengcheng, and Zoltán Haiman. “Ultra-Short-Period Massive Black Hole Binary Candidates in LSST as LISA ‘Verification Binaries.’” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2021. https://doi.org/10.1093/mnras/stab1856. ieee: C. Xin and Z. Haiman, “Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries,’” Monthly Notices of the Royal Astronomical Society, vol. 506, no. 2. Oxford University Press, pp. 2408–2417, 2021. ista: Xin C, Haiman Z. 2021. Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries’. Monthly Notices of the Royal Astronomical Society. 506(2), 2408–2417. mla: Xin, Chengcheng, and Zoltán Haiman. “Ultra-Short-Period Massive Black Hole Binary Candidates in LSST as LISA ‘Verification Binaries.’” Monthly Notices of the Royal Astronomical Society, vol. 506, no. 2, Oxford University Press, 2021, pp. 2408–17, doi:10.1093/mnras/stab1856. short: C. Xin, Z. Haiman, Monthly Notices of the Royal Astronomical Society 506 (2021) 2408–2417. date_created: 2024-09-05T12:19:58Z date_published: 2021-07-05T00:00:00Z date_updated: 2024-09-19T08:07:41Z day: '05' doi: 10.1093/mnras/stab1856 extern: '1' intvolume: ' 506' issue: '2' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stab1856 month: '07' oa: 1 oa_version: Published Version page: 2408-2417 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries’ type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 506 year: '2021' ... --- _id: '17578' abstract: - lang: eng text: "If primordial black holes (PBHs) seeded the supermassive black holes (SMBHs) at the centers of high-redshift quasars, then the gas surrounding these black holes may reveal nucleosynthetic clues to their primordial origins. We present predictions of altered primordial abundances around PBHs massive enough to seed SMBHs at \U0001D467≈6–7.5. We find that if PBHs with initial masses of ∼105  M⊙ are responsible for such SMBHs, they may produce primordial deuterium and Helium fractions enhanced by ≥10%, and lithium abundance depleted by ≥10%, at distances of up to ≈ a comoving kiloparsec away from the black hole after decoupling. We estimate that ∼108  M⊙ of gas is enhanced (or depleted) by at least one percent. Evidence of these modified primordial deuterium, helium, and lithium abundances could still be present if this circum-PBH gas remains unaccreted by the SMBH and in or near the host galaxies of high-redshift quasars. Measuring the abundance anomalies will be challenging, but could offer a novel way to reveal the primordial origin of such SMBH seeds." article_number: '103022' article_processing_charge: No article_type: original author: - first_name: Phoebe Upton full_name: Sanderbeck, Phoebe Upton last_name: Sanderbeck - first_name: Simeon full_name: Bird, Simeon last_name: Bird - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: Sanderbeck PU, Bird S, Haiman Z. Nucleosynthetic signatures of primordial origin around supermassive black holes. Physical Review D. 2021;104(10). doi:10.1103/physrevd.104.103022 apa: Sanderbeck, P. U., Bird, S., & Haiman, Z. (2021). Nucleosynthetic signatures of primordial origin around supermassive black holes. Physical Review D. American Physical Society. https://doi.org/10.1103/physrevd.104.103022 chicago: Sanderbeck, Phoebe Upton, Simeon Bird, and Zoltán Haiman. “Nucleosynthetic Signatures of Primordial Origin around Supermassive Black Holes.” Physical Review D. American Physical Society, 2021. https://doi.org/10.1103/physrevd.104.103022. ieee: P. U. Sanderbeck, S. Bird, and Z. Haiman, “Nucleosynthetic signatures of primordial origin around supermassive black holes,” Physical Review D, vol. 104, no. 10. American Physical Society, 2021. ista: Sanderbeck PU, Bird S, Haiman Z. 2021. Nucleosynthetic signatures of primordial origin around supermassive black holes. Physical Review D. 104(10), 103022. mla: Sanderbeck, Phoebe Upton, et al. “Nucleosynthetic Signatures of Primordial Origin around Supermassive Black Holes.” Physical Review D, vol. 104, no. 10, 103022, American Physical Society, 2021, doi:10.1103/physrevd.104.103022. short: P.U. Sanderbeck, S. Bird, Z. Haiman, Physical Review D 104 (2021). date_created: 2024-09-05T12:20:50Z date_published: 2021-11-17T00:00:00Z date_updated: 2024-09-19T08:12:35Z day: '17' doi: 10.1103/physrevd.104.103022 extern: '1' intvolume: ' 104' issue: '10' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1103/physrevd.104.103022 month: '11' oa: 1 oa_version: Published Version publication: Physical Review D publication_identifier: issn: - 2470-0010 - 2470-0029 publication_status: published publisher: American Physical Society quality_controlled: '1' scopus_import: '1' status: public title: Nucleosynthetic signatures of primordial origin around supermassive black holes type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 104 year: '2021' ... --- _id: '17583' abstract: - lang: eng text: The astrophysical origin of gravitational wave transients is a timely open question in the wake of discoveries by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo. In active galactic nuclei (AGNs), binaries form and evolve efficiently by interaction with a dense population of stars and the gaseous AGN disk. Previous studies have shown that stellar-mass black hole (BH) mergers in such environments can explain the merger rate and the number of suspected hierarchical mergers observed by LIGO/Virgo. The binary eccentricity distribution can provide further information to distinguish between astrophysical models. Here we derive the eccentricity distribution of BH mergers in AGN disks. We find that eccentricity is mainly due to binary–single (BS) interactions, which lead to most BH mergers in AGN disks having a significant eccentricity at 0.01 Hz, detectable by the Laser Interferometer Space Antenna. If BS interactions occur in isotropic-3D directions, then 8%–30% of the mergers in AGN disks will have eccentricities at 10 Hz above e10 Hz ≳ 0.03, detectable by LIGO/Virgo/Kamioka Gravitational Wave Detector, while 5%–17% of mergers have e10 Hz ≥ 0.3. On the other hand, if BS interactions are confined to the AGN–disk plane due to torques from the disk, with 1–20 intermediate binary states during each interaction, or if BHs can migrate to ≲ 10−3 pc from the central supermassive BH, then 10%–70% of the mergers will be highly eccentric (e10 Hz ≥ 0.3), consistent with the possible high eccentricity in GW190521. article_number: L20 article_processing_charge: No article_type: original author: - first_name: Hiromichi full_name: Tagawa, Hiromichi last_name: Tagawa - first_name: Bence full_name: Kocsis, Bence last_name: Kocsis - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Imre full_name: Bartos, Imre last_name: Bartos - first_name: Kazuyuki full_name: Omukai, Kazuyuki last_name: Omukai - first_name: Johan full_name: Samsing, Johan last_name: Samsing citation: ama: Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. Eccentric black hole mergers in active galactic nuclei. The Astrophysical Journal Letters. 2021;907(1). doi:10.3847/2041-8213/abd4d3 apa: Tagawa, H., Kocsis, B., Haiman, Z., Bartos, I., Omukai, K., & Samsing, J. (2021). Eccentric black hole mergers in active galactic nuclei. The Astrophysical Journal Letters. American Astronomical Society. https://doi.org/10.3847/2041-8213/abd4d3 chicago: Tagawa, Hiromichi, Bence Kocsis, Zoltán Haiman, Imre Bartos, Kazuyuki Omukai, and Johan Samsing. “Eccentric Black Hole Mergers in Active Galactic Nuclei.” The Astrophysical Journal Letters. American Astronomical Society, 2021. https://doi.org/10.3847/2041-8213/abd4d3. ieee: H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, and J. Samsing, “Eccentric black hole mergers in active galactic nuclei,” The Astrophysical Journal Letters, vol. 907, no. 1. American Astronomical Society, 2021. ista: Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. 2021. Eccentric black hole mergers in active galactic nuclei. The Astrophysical Journal Letters. 907(1), L20. mla: Tagawa, Hiromichi, et al. “Eccentric Black Hole Mergers in Active Galactic Nuclei.” The Astrophysical Journal Letters, vol. 907, no. 1, L20, American Astronomical Society, 2021, doi:10.3847/2041-8213/abd4d3. short: H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, J. Samsing, The Astrophysical Journal Letters 907 (2021). date_created: 2024-09-05T12:27:07Z date_published: 2021-01-21T00:00:00Z date_updated: 2024-09-19T11:41:11Z day: '21' doi: 10.3847/2041-8213/abd4d3 extern: '1' intvolume: ' 907' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3847/2041-8213/abd4d3 month: '01' oa: 1 oa_version: Published Version publication: The Astrophysical Journal Letters publication_identifier: issn: - 2041-8205 - 2041-8213 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: Eccentric black hole mergers in active galactic nuclei type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 907 year: '2021' ... --- _id: '17585' abstract: - lang: eng text: Recent gravitational wave (GW) observations by LIGO/Virgo show evidence for hierarchical mergers, where the merging BHs are the remnants of previous BH merger events. These events may carry important clues about the astrophysical host environments of the GW sources. In this paper, we present the distributions of the effective spin parameter (χeff), the precession spin parameter (χp), and the chirp mass (mchirp) expected in hierarchical mergers. Under a wide range of assumptions, hierarchical mergers produce (i) a monotonic increase of the average of the typical total spin for merging binaries, which we characterize with χ¯typ≡(χ2eff+χ2p)1/2¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯¯, up to roughly the maximum mchirp among first-generation (1g) BHs, and (ii) a plateau at χ¯typ∼0.6 at higher mchirp. We suggest that the maximum mass and typical spin magnitudes for 1g BHs can be estimated from χ¯typ as a function of mchirp. The GW data observed in LIGO/Virgo O1--O3a prefers an increase in χ¯typ at low mchirp, which is consistent with the growth of the BH spin magnitude by hierarchical mergers, at ∼2σ confidence. A Bayesian analysis suggests that 1g BHs have the maximum mass of ∼15--30M⊙ if the majority of mergers are of high-generation BHs (not among 1g-1g BHs), which is consistent with mergers in active galactic nucleus disks and/or nuclear star clusters, while if mergers mainly originate from globular clusters, 1g BHs are favored to have non-zero spin magnitudes of ∼0.3. We also forecast that signatures for hierarchical mergers in the χ¯typ distribution can be confidently recovered once the number of GW events increases to ≳O(100). article_processing_charge: No article_type: original author: - first_name: Hiromichi full_name: Tagawa, Hiromichi last_name: Tagawa - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Imre full_name: Bartos, Imre last_name: Bartos - first_name: Bence full_name: Kocsis, Bence last_name: Kocsis - first_name: Kazuyuki full_name: Omukai, Kazuyuki last_name: Omukai citation: ama: Tagawa H, Haiman Z, Bartos I, Kocsis B, Omukai K. Signatures of hierarchical mergers in black hole spin and mass distribution. Monthly Notices of the Royal Astronomical Society. 2021;507(3):3362-3380. doi:10.1093/mnras/stab2315 apa: Tagawa, H., Haiman, Z., Bartos, I., Kocsis, B., & Omukai, K. (2021). Signatures of hierarchical mergers in black hole spin and mass distribution. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stab2315 chicago: Tagawa, Hiromichi, Zoltán Haiman, Imre Bartos, Bence Kocsis, and Kazuyuki Omukai. “Signatures of Hierarchical Mergers in Black Hole Spin and Mass Distribution.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2021. https://doi.org/10.1093/mnras/stab2315. ieee: H. Tagawa, Z. Haiman, I. Bartos, B. Kocsis, and K. Omukai, “Signatures of hierarchical mergers in black hole spin and mass distribution,” Monthly Notices of the Royal Astronomical Society, vol. 507, no. 3. Oxford University Press, pp. 3362–3380, 2021. ista: Tagawa H, Haiman Z, Bartos I, Kocsis B, Omukai K. 2021. Signatures of hierarchical mergers in black hole spin and mass distribution. Monthly Notices of the Royal Astronomical Society. 507(3), 3362–3380. mla: Tagawa, Hiromichi, et al. “Signatures of Hierarchical Mergers in Black Hole Spin and Mass Distribution.” Monthly Notices of the Royal Astronomical Society, vol. 507, no. 3, Oxford University Press, 2021, pp. 3362–80, doi:10.1093/mnras/stab2315. short: H. Tagawa, Z. Haiman, I. Bartos, B. Kocsis, K. Omukai, Monthly Notices of the Royal Astronomical Society 507 (2021) 3362–3380. date_created: 2024-09-05T12:30:08Z date_published: 2021-08-13T00:00:00Z date_updated: 2024-09-19T11:50:46Z day: '13' doi: 10.1093/mnras/stab2315 extern: '1' intvolume: ' 507' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stab2315 month: '08' oa: 1 oa_version: Published Version page: 3362-3380 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: Signatures of hierarchical mergers in black hole spin and mass distribution type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 507 year: '2021' ...