TY - JOUR A1 - Roelofs, Freek A1 - Blackburn, Lindy A1 - Lindahl, Greg A1 - Doeleman, Sheperd S. A1 - Johnson, Michael D. A1 - Arras, Philipp A1 - Chatterjee, Koushik A1 - Emami, Razieh A1 - Fromm, Christian A1 - Fuentes, Antonio A1 - Knollmüller, Jakob A1 - Kosogorov, Nikita A1 - Müller, Hendrik A1 - Patel, Nimesh A1 - Raymond, Alexander A1 - Tiede, Paul A1 - Traianou, Efthalia A1 - Vega, Justin T1 - The ngEHT analysis challenges JF - Galaxies N2 - The next-generation Event Horizon Telescope (ngEHT) will be a significant enhancement of the Event Horizon Telescope (EHT) array, with ∼10 new antennas and instrumental upgrades of existing antennas. The increased uv-coverage, sensitivity, and frequency coverage allow a wide range of new science opportunities to be explored. The ngEHT Analysis Challenges have been launched to inform the development of the ngEHT array design, science objectives, and analysis pathways. For each challenge, synthetic EHT and ngEHT datasets are generated from theoretical source models and released to the challenge participants, who analyze the datasets using image reconstruction and other methods. The submitted analysis results are evaluated with quantitative metrics. In this work, we report on the first two ngEHT Analysis Challenges. These have focused on static and dynamical models of M87* and Sgr A* and shown that high-quality movies of the extended jet structure of M87* and near-horizon hourly timescale variability of Sgr A* can be reconstructed by the reference ngEHT array in realistic observing conditions using current analysis algorithms. We identify areas where there is still room for improvement of these algorithms and analysis strategies. Other science cases and arrays will be explored in future challenges. KW - very long baseline interferometry KW - black holes KW - active galactic nuclei KW - radio astronomy KW - imaging KW - instrument design KW - telescopes KW - algorithms KW - data analysis Y1 - 2023 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-304976 SN - 2075-4434 VL - 11 IS - 1 ER - TY - JOUR A1 - Majounie, Elisa A1 - Renton, Alan E. A1 - Mok, Kin A1 - Dopper, Elise G. P. A1 - Waite, Adrian A1 - Rollinson, Sara A1 - Chiò, Adriano A1 - Restagno, Gabriella A1 - Nicolaou, Nayia A1 - Simon-Sanchez, Javier A1 - van Swieten, John C. A1 - Abramzon, Yevgeniya A1 - Johnson, Janel O. A1 - Sendtner, Michael A1 - Pamphlett, Roger A1 - Orrell, Richard W. A1 - Mead, Simon A1 - Sidle, Katie C. A1 - Houlden, Henry A1 - Rohrer, Jonathan D. A1 - Morrison, Karen E. A1 - Pall, Hardev A1 - Talbot, Kevin A1 - Ansorge, Olaf A1 - Hernandez, Dena G. A1 - Arepalli, Sampath A1 - Sabatelli, Mario A1 - Mora, Gabriele A1 - Corbo, Massimo A1 - Giannini, Fabio A1 - Calvo, Andrea A1 - Englund, Elisabet A1 - Borghero, Giuseppe A1 - Floris, Gian Luca A1 - Remes, Anne M. A1 - Laaksovirta, Hannu A1 - McCluskey, Leo A1 - Trojanowski, John Q. A1 - Van Deerlin, Vivianna M. A1 - Schellenberg, Gerard D. A1 - Nalls, Michael A. A1 - Drory, Vivian E. A1 - Lu, Chin-Song A1 - Yeh, Tu-Hsueh A1 - Ishiura, Hiroyuki A1 - Takahashi, Yuji A1 - Tsuji, Shoji A1 - Le Ber, Isabelle A1 - Brice, Alexis A1 - Drepper, Carsten A1 - Williams, Nigel A1 - Kirby, Janine A1 - Shaw, Pamela A1 - Hardy, John A1 - Tienari, Pentti J. A1 - Heutink, Peter A1 - Morris, Huw R. A1 - Pickering-Brown, Stuart A1 - Traynor, Bryan J. T1 - Frequency of the C9orf72 hexanucleotide repeat expansion in patients with amyotrophic lateral sclerosis and frontotemporal dementia: a cross-sectional study JF - The Lancet Neurology N2 - Background We aimed to accurately estimate the frequency of a hexanucleotide repeat expansion in C9orf72 that has been associated with a large proportion of cases of amyotrophic lateral sclerosis (ALS) and frontotemporal dementia (FTD). Methods We screened 4448 patients diagnosed with ALS (El Escorial criteria) and 1425 patients with FTD (Lund-Manchester criteria) from 17 regions worldwide for the GGGGCC hexanucleotide expansion using a repeat-primed PCR assay. We assessed familial disease status on the basis of self-reported family history of similar neurodegenerative diseases at the time of sample collection. We compared haplotype data for 262 patients carrying the expansion with the known Finnish founder risk haplotype across the chromosomal locus. We calculated age-related penetrance using the Kaplan-Meier method with data for 603 individuals with the expansion. Findings In patients with sporadic ALS, we identified the repeat expansion in 236 (7·0%) of 3377 white individuals from the USA, Europe, and Australia, two (4·1%) of 49 black individuals from the USA, and six (8·3%) of 72 Hispanic individuals from the USA. The mutation was present in 217 (39·3%) of 552 white individuals with familial ALS from Europe and the USA. 59 (6·0%) of 981 white Europeans with sporadic FTD had the mutation, as did 99 (24·8%) of 400 white Europeans with familial FTD. Data for other ethnic groups were sparse, but we identified one Asian patient with familial ALS (from 20 assessed) and two with familial FTD (from three assessed) who carried the mutation. The mutation was not carried by the three Native Americans or 360 patients from Asia or the Pacific Islands with sporadic ALS who were tested, or by 41 Asian patients with sporadic FTD. All patients with the repeat expansion had (partly or fully) the founder haplotype, suggesting a one-off expansion occurring about 1500 years ago. The pathogenic expansion was non-penetrant in individuals younger than 35 years, 50% penetrant by 58 years, and almost fully penetrant by 80 years. Interpretation A common Mendelian genetic lesion in C9orf72 is implicated in many cases of sporadic and familial ALS and FTD. Testing for this pathogenic expansion should be considered in the management and genetic counselling of patients with these fatal neurodegenerative diseases. KW - DNA repeat expansion KW - C9orf72 KW - amyotrophic lateral sclerosis KW - frontotemporal dementia KW - cross-sectional studies Y1 - 2012 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-154644 VL - 11 SP - 323 EP - 330 ER - TY - JOUR A1 - Johnson, Michael D. A1 - Akiyama, Kazunori A1 - Blackburn, Lindy A1 - Bouman, Katherine L. A1 - Broderick, Avery E. A1 - Cardoso, Vitor A1 - Fender, Rob P. A1 - Fromm, Christian M. A1 - Galison, Peter A1 - Gómez, José L. A1 - Haggard, Daryl A1 - Lister, Matthew L. A1 - Lobanov, Andrei P. A1 - Markoff, Sera A1 - Narayan, Ramesh A1 - Natarajan, Priyamvada A1 - Nichols, Tiffany A1 - Pesce, Dominic W. A1 - Younsi, Ziri A1 - Chael, Andrew A1 - Chatterjee, Koushik A1 - Chaves, Ryan A1 - Doboszewski, Juliusz A1 - Dodson, Richard A1 - Doeleman, Sheperd S. A1 - Elder, Jamee A1 - Fitzpatrick, Garret A1 - Haworth, Kari A1 - Houston, Janice A1 - Issaoun, Sara A1 - Kovalev, Yuri Y. A1 - Levis, Aviad A1 - Lico, Rocco A1 - Marcoci, Alexandru A1 - Martens, Niels C. M. A1 - Nagar, Neil M. A1 - Oppenheimer, Aaron A1 - Palumbo, Daniel C. M. A1 - Ricarte, Angelo A1 - Rioja, María  J. A1 - Roelofs, Freek A1 - Thresher, Ann C. A1 - Tiede, Paul A1 - Weintroub, Jonathan A1 - Wielgus, Maciek T1 - Key science goals for the next-generation Event Horizon Telescope JF - Galaxies N2 - The Event Horizon Telescope (EHT) has led to the first images of a supermassive black hole, revealing the central compact objects in the elliptical galaxy M87 and the Milky Way. Proposed upgrades to this array through the next-generation EHT (ngEHT) program would sharply improve the angular resolution, dynamic range, and temporal coverage of the existing EHT observations. These improvements will uniquely enable a wealth of transformative new discoveries related to black hole science, extending from event-horizon-scale studies of strong gravity to studies of explosive transients to the cosmological growth and influence of supermassive black holes. Here, we present the key science goals for the ngEHT and their associated instrument requirements, both of which have been formulated through a multi-year international effort involving hundreds of scientists worldwide. KW - black holes KW - general relativity KW - interferometry KW - accretion KW - relativistic jets KW - very-long-baseline interferometry KW - EHT KW - ngEHT Y1 - 2023 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-313525 SN - 2075-4434 VL - 11 IS - 3 ER - TY - JOUR A1 - Chatterjee, Koushik A1 - Chael, Andrew A1 - Tiede, Paul A1 - Mizuno, Yosuke A1 - Emami, Razieh A1 - Fromm, Christian A1 - Ricarte, Angelo A1 - Blackburn, Lindy A1 - Roelofs, Freek A1 - Johnson, Michael D. A1 - Doeleman, Sheperd S. A1 - Arras, Philipp A1 - Fuentes, Antonio A1 - Knollmüller, Jakob A1 - Kosogorov, Nikita A1 - Lindahl, Greg A1 - Müller, Hendrik A1 - Patel, Nimesh A1 - Raymond, Alexander A1 - Traianou, Efthalia A1 - Vega, Justin T1 - Accretion flow morphology in numerical simulations of black holes from the ngEHT model library: the impact of radiation physics JF - Galaxies N2 - In the past few years, the Event Horizon Telescope (EHT) has provided the first-ever event horizon-scale images of the supermassive black holes (BHs) M87* and Sagittarius A* (Sgr A*). The next-generation EHT project is an extension of the EHT array that promises larger angular resolution and higher sensitivity to the dim, extended flux around the central ring-like structure, possibly connecting the accretion flow and the jet. The ngEHT Analysis Challenges aim to understand the science extractability from synthetic images and movies to inform the ngEHT array design and analysis algorithm development. In this work, we compare the accretion flow structure and dynamics in numerical fluid simulations that specifically target M87* and Sgr A*, and were used to construct the source models in the challenge set. We consider (1) a steady-state axisymmetric radiatively inefficient accretion flow model with a time-dependent shearing hotspot, (2) two time-dependent single fluid general relativistic magnetohydrodynamic (GRMHD) simulations from the H-AMR code, (3) a two-temperature GRMHD simulation from the BHAC code, and (4) a two-temperature radiative GRMHD simulation from the KORAL code. We find that the different models exhibit remarkably similar temporal and spatial properties, except for the electron temperature, since radiative losses substantially cool down electrons near the BH and the jet sheath, signaling the importance of radiative cooling even for slowly accreting BHs such as M87*. We restrict ourselves to standard torus accretion flows, and leave larger explorations of alternate accretion models to future work. KW - black holes KW - general relativity KW - accretion KW - relativistic jets KW - very-long-baseline interferometry Y1 - 2023 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-304084 SN - 2075-4434 VL - 11 IS - 2 ER -