5 research outputs found
NILAI-NILAI MODERASI BERAGAMA DALAM PEMBENTUKAN KARAKTER SISWA DI SEKOLAH DASAR: Penelitian Kualitatif Deskriptif di Sekolah Dasar Islam Al-isro Muhammadiyah 7 Daerah Khusus Jakarta
Get PDFPengimplementasian moderasi beragama di sekolah sebenarnya sudah diterapakan sejak lama, namun banyak orang tidak menyadari bahwa kegiatan dalam kehidupan sehari-hari sudah termasuk ke dalam nilai-nilai moderasi beragama. Penelitian ini dilaksanakan di Sekolah Dasar Islam Al-Isro Muhammadiyah 7 untuk menganalisis sejauh mana sekolah tersebut sudah melakukan pengimplementasian nilai-nilai moderasi beragama. Penelitian ini juga menelaah bagaimana proses, apa yang menjadi faktor pendukung dan penghambat. serta dampak dalam pembentukan karakter siswa dalam pengimplementasian moderasi beragama. Pada penelitian ini menggunakan pendeketan kualitatif dan menggunakan metode deskriptif. Untuk mendapatkan hasil penelitian, pada penelitian ini mengumpulkan dengan menggunakan wawancara, observasi, dan dokumentasi. Hasil penelitian menunjukkan bahwa nilai-nilai moderasi beragama di Sekolah Dasar Islam Al-Isro Muhammadiyah 7 sudah terimplementasi dengan baik sehingga dapat hasil yang positif dalam pembentukan karakter siswa-siswi.
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The implementation of religious moderation in schools has actually been implemented for a long time, but many people do not realize that activities in daily life are included in the values of religious moderation. This research was conducted at Al-Isro Muhammadiyah 7 Islamic Elementary School to analyze the extent to which the school has implemented the values of religious moderation. This study also examines how the process, what are the supporting and inhibiting factors, and the impact on student character building in implementing religious moderation. This research uses a qualitative approach and uses descriptive methods. To get the research results, this research collects by using interviews, observations, and documentation. The results showed that the values of religious moderation at Al-Isro Muhammadiyah 7 Islamic Elementary School have been implemented well so that it can have positive results in the formation of student character
Evaluasi Program Pembelajaran PTM Terbatas
Get PDFCovid-19 sudah memberikan banyak dampak terhadap berbagai bidang, salah satunya bidang pendidikan. Pembelajaran Tatap Muka terbatas merupakan solusi yang diberikan oleh KEMENDIKBUD melalui surat Keputusan Bersama Menteri Pendidikan dan Kebudayaan, Menteri Agama, Menteri Kesehatan, dan Menteri Dalam Negeri Nomor 03/KB/2021, Nomor 384 Tahun 2021, Nomor HK.01.08/MENNKES/4242/2021, Nomor 440-717 Tahun 2021 tentang Panduan Pembelajaran di Masa Pandemi Coronavirus Disease 2019 (Covid-19) atau yang disebut sebagai Surat Keputusan Bersama (SKB) Empat Menteri. Tujuan dari penelitian ini antara lain untuk melihata bagaimana pelaksanaan dari PTM terbatas. Penulis dalam penulisannya menggunakan penelitian kualitatif metode deskriptif. Prosedur Penelitian dilakukan dengan cara penyebaran angket terhadap responden. Berdasarkan hasil penelitian, penulis mendapatkan bahwa tidak semua sekolah melaksanakan PTM terbatas. Didalam pelaksanaan PTM terbatas masih terdapat kekurangan seperti kurangnya fasilitas protokol kesehatan. Serta terdapat beberapa sekolah yang masih belum bisa memenuhi syarat yang sudah ditentukan oleh KEMENDIKBUD. PTM terbatas memiliki kekurangan serta kelebihan. Adapun siswa lebih banyak merasakan ketidakefektivan dalam belajar dikarenakan oleh beberapa fakto
Pendidikan Anak Dalam Perspektif HAM dan Hukum Islam
Get PDFDapat diketahui bahwasanya pendidikan bagi anak itu sangat penting. penulisan ini bertujuan untuk menyadarkan orang tua, bahwa pendidikan merupakan bagian dari Hak Asasi Manusia yang harus dipenuhi pada anak. serta memberitahu bahwasanya pendidikan terdapat pada Hukum Islam. Metode yang dilakukan oleh peneliti yaitu menyebarkan angket menggunakan Google-form yang disebarkan kepada masyarakat umum khususnya orang tua. Hasil yang diterima penulis dari penyebaran angket yaitu: masih banyak orang tua mengatakan bahwa pendidikan pada anak itu sangat penting. tapi ada beberapa yang orang tua tidak memenuhi hak asasi manusia dalam pendidikan anak. Dikarenakan beberapa faktor, seperti faktor ekonomi, faktor keluarga, serta faktor lingkung tempat tinggal.dengan adanya penulisan ini semoga bisa menjadi bahan analisa mengenai pendidikan dalam tingkat sekolah dasar dan terpenuhinya HAM anak dalam pendidikan. serta diharapkan bahwasanya kepada orang tua bisa menyadari bahwa pendidikan bagi anak itu penting baik pendidikan dunia maupun akhirat. Supaya kelak anak kita semua bisa bermanfaat bagi dirinya sendiri serta lingkungannya
Broadband multi-wavelength properties of M87 during the 2018 EHT campaign including a very high energy flaring episode
No full textAlgaba, Juan-Carlos et al.-- Full list of authors: Algaba, J. C.; Baloković, M.; Chandra, S.; Cheong, W. -Y.; Cui, Y. -Z.; D'Ammando, F.; Falcone, A. D.; Ford, N. M.; Giroletti, M.; Goddi, C.; Gurwell, M. A.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Kerby, S.; Kim, J. -Y.; Kino, M.; Kravchenko, E. V.; Lee, S. -S.; Lu, R. -S.; Markoff, S.; Michail, J.; Neilsen, J.; Nowak, M. A.; Principe, G.; Ramakrishnan, V.; Ripperda, B.; Sasada, M.; Savchenko, S. S.; Sheridan, C.; Akiyama, K.; Alberdi, A.; Alef, W.; Anantua, R.; Asada, K.; Azulay, R.; Bach, U.; Baczko, A. -K.; Ball, D.; Bandyopadhyay, B.; Barrett, J.; Bauböck, M.; Benson, B. A.; Bintley, D.; lackburn, L.; Blundell, R.; Bouman, K. L.; Bower, G. C.; Boyce, H.; Bremer, M.; Brissenden, R.; Britzen, S.; Broderick, A. E.; Broguiere, D.; Bronzwaer, T.; Bustamante, S.; Carlstrom, J. E.; Chael, A.; Chan, C. -k.; Chang, D. O.; Chatterjee, K.; Chatterjee, S.; Chen, M. -T.; Chen, Y.; Cheng, X.; Cho, I.; Christian, P.; Conroy, N. S.; Conway, J. E.; Crawford, T. M.; Crew, G. B.; Cruz-Osorio, A.; Dahale, R.; Davelaar, J.; De Laurentis, M.; Deane, R.; Dempsey, J.; Desvignes, G.; Dexter, J.; Dhruv, V.; Dihingia, I. K.; Doeleman, S. S.; Dzib, S. A.; Eatough, R. P.; Emami, R.; Falcke, H.; Farah, J.; Fish, V. L.; Fomalont, E.; Ford, H. A.; Foschi, M.; Fraga-Encinas, R.; Freeman, W. T.; Friberg, P.; Fromm, C. M.; Fuentes, A.; Galison, P.; Gammie, C. F.; García, R.; Gentaz, O.; Georgiev, B.; Gold, R.; Gómez-Ruiz, A. I.; Gómez, J. L.; Gu, M.; Hesper, R.; Heumann, D.; Ho, L. C.; Ho, P.; Honma, M.; Huang, C. -W. L.; Huang, L.; Hughes, D. H.; Ikeda, S.; Impellizzeri, C. M. V.; Inoue, M.; Issaoun, S.; James, D. J.; Jannuzi, B. T.; Janssen, M.; Jeter, B.; Jiang, W.; Jiménez-Rosales, A.; Johnson, M. D.; Jones, A. C.; Joshi, A. V.; Jung, T.; Karuppusamy, R.; Keating, G. K.; Kettenis, M.; Kim, D. -J.; Kim, J.; Kim, J.; Koay, J. Y.; Kocherlakota, P.; Kofuji, Y.; Koch, P. M.; Koyama, S.; Kramer, C.; Kramer, J. A.; Kramer, M.; Krichbaum, T. P.; Kuo, C. -Y.; La Bella, N.; Levis, A.; Li, Z.; Lico, R.; Lindahl, G.; Lindqvist, M.; Lisakov, M.; Liu, J.; Liu, K.; Liuzzo, E.; Lo, W. -P.; Lobanov, A. P.; Loinard, L.; Lonsdale, C. J.; Lowitz, A. E.; MacDonald, N. R.; Mao, J.; Marchili, N.; Marrone, D. P.; Marscher, A. P.; Martí-Vidal, I.; Matsushita, S.; Matthews, L. D.; Medeiros, L.; Menten, K. M.; Mizuno, I.; Mizuno, Y.; Montgomery, J.; Moran, J. M.; Moriyama, K.; Moscibrodzka, M.; Mulaudzi, W.; Müller, C.; Müller, H.; Mus, A.; Musoke, G.; Myserlis, I.; Nagai, H.; Nagar, N. M.; Nair, D. G.; Nakamura, M.; Narayanan, G.; Natarajan, I.; Nathanail, A.; Navarro Fuentes, S.; Ni, C.; Oh, J.; Okino, H.; Olivares, H.; Oyama, T.; Özel, F.; Palumbo, D. C. M.; Filippos Paraschos, G.; Park, J.; Parsons, H.; Patel, N.; Pen, U. -L.; Pesce, D. W.; Piétu, V.; PopStefanija, A.; Porth, O.; Prather, B.; Psaltis, D.; Pu, H. -Y.; Rao, R.; Rawlings, M. G.; Raymond, A. W.; Rezzolla, L.; Ricarte, A.; Roelofs, F.; Romero-Cañizales, C.; Ros, E.; Roshanineshat, A.; Rottmann, H.; Roy, A. L.; Ruiz, I.; Ruszczyk, C.; Rygl, K. L. J.; Sánchez, S.; Sánchez-Argüelles, D.; Sánchez-Portal, M.; Satapathy, K.; Savolainen, T.; Schloerb, F. P.; Schonfeld, J.; Schuster, K. -F.; Shao, L.; Shen, Z.; Small, D.; Sohn, B. W.; SooHoo, J.; Sosapanta Salas, L. D.; Souccar, K.; Stanway, J. S.; Sun, H.; Tazaki, F.; Tetarenko, A. J.; Tiede, P.; Tilanus, R. P. J.; Titus, M.; Toma, K.; Torne, P.; Toscano, T.; Traianou, E.; Trent, T.; Trippe, S.; Turk, M.; van Bemmel, I.; van Langevelde, H. J.; van Rossum, D. R.; Vos, J.; Wagner, J.; Ward-Thompson, D.; Wardle, J.; Washington, J. E.; Weintroub, J.; Wharton, R.; Wielgus, M.; Wiik, K.; Witzel, G.; Wondrak, M. F.; Wong, G. N.; Wu, Q.; Yadlapalli, N.; Yamaguchi, P.; Yfantis, A.; Yoon, D.; Young, A.; Younsi, Z.; Yu, W.; Yuan, F.; Yuan, Y. -F.; Zensus, J. A.; Zhang, S.; Zhao, G. -Y.; Zhao, S. -S.; Bellazzini, R.; Berenji, B.; Bissaldi, E.; Blandford, R. D.; Bonino, R.; Bruel, P.; Cameron, R. A.; Caraveo, P. A.; Cavazzuti, E.; Cheung, C. C.; Ciprini, S.; Cristarella Orestano, P.; Cutini, S.; Di Lalla, N.; Dinesh, A.; Di Venere, L.; Domínguez, A.; Fegan, S. J.; Franckowiak, A.; Fukazawa, Y.; Fusco, P.; Gargano, F.; Gasbarra, C.; Germani, S.; Giliberti, M.; Grenier, I. A.; Hays, E.; Horan, D.; Kuss, M.; Larsson, S.; Liodakis, I.; Longo, F.; Loparco, F.; Lovellette, M. N.; Maldera, S.; Mazziotta, M. N.; Mereu, I.; Michelson, P. F.; Mirabal, N.; Mizuno, T.; Monzani, M. E.; Morselli, A.; Negro, M.; Omodei, N.; Orlando, E.; Persic, M.; Rainò, S.; Rani, B.; Reimer, A.; Reimer, O.; Sánchez-Conde, M.; Saz Parkinson, P. M.; Sgrò, C.; Siskind, E. J.; Spinelli, P.; Suson, D. J.; Tajima, H.; Torres, D. F.; Zaharijas, G.; Aharonian, F.; Ait Benkhali, F.; Aschersleben, J.; Ashkar, H.; Backes, M.; Barbosa Martins, V.; Batzofin, R.; Becherini, Y.; Berge, D.; Böttcher, M.; Boisson, C.; Bolmont, J.; de Bony de Lavergne, M.; Borowska, J.; Bouyahiaoui, M.; Bradascio, F.; Brose, R.; Brown, A.; Bruno, B.; Bulik, T.; Burger-Scheidlin, C.; Casanova, S.; Cecil, R.; Celic, J.; Cerruti, M.; Chand, T.; Chen, A.; Chibueze, J.; Chibueze, O.; Cotter, G.; Damascene Mbarubucyeye, J.; Devin, J.; Djuvsland, J.; Dmytriiev, A.; Einecke, S.; Ernenwein, J. -P.; Feijen, K.; Fontaine, G.; Funk, S.; Gabici, S.; Glawion, D.; Glicenstein, J. F.; Goswami, P.; Grolleron, G.; Haerer, L.; Heß, B.; Holch, T. L.; Holler, M.; Horns, D.; Huang, Zhiqiu; Jamrozy, M.; Jankowsky, F.; Jung-Richardt, I.; Kasai, E.; Katarzyński, K.; Khatoon, R.; Khélifi, B.; Kluźniak, W.; Komin, Nu.; Kosack, K.; Kundu, A.; Lang, R. G.; Le Stum, S.; Leitl, F.; Lemière, A.; Lemoine-Goumard, M.; Lenain, J. -P.; Leuschner, F.; Luashvili, A.; Mackey, J.; Malyshev, D.; Martí-Devesa, G.; Marx, R.; Meyer, M.; Mitchell, A.; Moderski, R.; Moghadam, M. O.; Mohrmann, L.; Montanari, A.; Moulin, E.; de Naurois, M.; Niemiec, J.; O'Brien, P.; Ohm, S.; de Ona Wilhelmi, E.; Ostrowski, M.; Panny, S.; Panter, M.; Pensec, U.; Pita, S.; Pühlhofer, G.; Quirrenbach, A.; Ravikularaman, S.; Reimer, A.; Reimer, O.; Reville, B.; Reis, I.; Ren, H.; Rieger, F.; Roellinghoff, G.; Rudak, B.; Ruiz-Velasco, E.; Sabri, K.; Sahakian, V.; Salzmann, H.; Santangelo, A.; Sasaki, M.; Schäfer, J.; Schüssler, F.; Schutte, H. M.; Shapopi, J. N. S.; Sharma, A.; Sol, H.; Spencer, S.; Stawarz, Ł.; Steppa, C.; Streil, K.; Suzuki, H.; Takahashi, T.; Tanaka, T.; Taylor, A. M.; Terrier, R.; Tluczykont, M.; Tsirou, M.; van Eldik, C.; Vecchi, M.; Wach, T.; Wagner, S. J.; Wierzcholska, A.; Zacharias, M.; Zdziarski, A. A.; Zech, A.; Żywucka, N.; Abe, S.; Abhir, J.; Abhishek, A.; Acciari, V. A.; Aguasca-Cabot, A.; Agudo, I.; Aniello, T.; Ansoldi, S.; Antonelli, L. A.; Arbet Engels, A.; Arcaro, C.; Artero, M.; Asano, K.; Babić, A.; Barres de Almeida, U.; Barrio, J. A.; Batković, I.; Bautista, A.; Baxter, J.; Becerra González, J.; Bednarek, W.; Bernardini, E.; Bernete, J.; Berti, A.; Besenrieder, J.; Bigongiari, C.; Biland, A.; Blanch, O.; Bonnoli, G.; Bošnjak, Ž.; Bronzini, E.; Burelli, I.; Busetto, G.; Campoy-Ordaz, A.; Carosi, A.; Carosi, R.; Carretero-Castrillo, M.; Castro-Tirado, A. J.; Cerasole, D.; Ceribella, G.; Chai, Y.; Cifuentes, A.; Colombo, E.; Contreras, J. L.; Cortina, J.; Covino, S.; D'Amico, G.; D'Elia, V.; Da Vela, P.; Dazzi, F.; De Angelis, A.; De Lotto, B.; de Menezes, R.; Delfino, M.; Delgado, J.; Delgado Mendez, C.; Di Pierro, F.; Di Tria, R.; Di Venere, L.; Dominis Prester, D.; Donini, A.; Dorner, D.; Doro, M.; Elsaesser, D.; Escudero, J.; Fariña, L.; Fattorini, A.; Foffano, L.; Font, L.; Fröse, S.; Fukami, S.; Fukazawa, Y.; García López, R. J.; Garczarczyk, M.; Gasparyan, S.; Gaug, M.; Giesbrecht Paiva, J. G.; Giglietto, N.; Giordano, F.; Gliwny, P.; Godinović, N.; Gradetzke, T.; Grau, R.; Green, D.; Green, J. G.; Günther, P.; Hadasch, D.; Hahn, A.; Hassan, T.; Heckmann, L.; Herrera Llorente, J.; Hrupec, D.; Imazawa, R.; Ishio, K.; Jiménez Martínez, I.; Jormanainen, J.; Kayanoki, T.; Kerszberg, D.; Kluge, G. W.; Kobayashi, Y.; Kouch, P. M.; Kubo, H.; Kushida, J.; Láinez, M.; Lamastra, A.; Leone, F.; Lindfors, E.; Lombardi, S.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Lorini, A.; Lyard, E.; Machado de Oliveira Fraga, B.; Majumdar, P.; Makariev, M.; Maneva, G.; Manganaro, M.; Mangano, S.; Mannheim, K.; Mariotti, M.; Martínez, M.; Martínez-Chicharro, M.; Mas-Aguilar, A.; Mazin, D.; Menchiari, S.; Mender, S.; Miceli, D.; Miener, T.; Miranda, J. M.; Mirzoyan, R.; Molero González, M.; Molina, E.; Mondal, H. A.; Moralejo, A.; Morcuende, D.; Nakamori, T.; Nanci, C.; Neustroev, V.; Nickel, L.; Nievas Rosillo, M.; Nigro, C.; Nikolić, L.; Nilsson, K.; Nishijima, K.; Njoh Ekoume, T.; Noda, K.; Nozaki, S.; Ohtani, Y.; Okumura, A.; Otero-Santos, J.; Paiano, S.; Paneque, D.; Paoletti, R.; Paredes, J. M.; Peresano, M.; Persic, M.; Pihet, M.; Pirola, G.; Podobnik, F.; Prada Moroni, P. G.; Prandini, E.; Priyadarshi, C.; Ribó, M.; Rico, J.; Righi, C.; Sahakyan, N.; Saito, T.; Saturni, F. G.; Schmidt, K.; Schmuckermaier, F.; Schubert, J. L.; Schweizer, T.; Sciaccaluga, A.; Silvestri, G.; Sitarek, J.; Sliusar, V.; Sobczynska, D.; Spolon, A.; Stamerra, A.; Strišković, J.; Strom, D.; Strzys, M.; Suda, Y.; Suutarinen, S.; Tajima, H.; Takahashi, M.; Takeishi, R.; Tavecchio, F.; Temnikov, P.; Terauchi, K.; Terzić, T.; Teshima, M.; Truzzi, S.; Tutone, A.; Ubach, S.; van Scherpenberg, J.; Vazquez Acosta, M.; Ventura, S.; Verna, G.; Viale, I.; Vigorito, C. F.; Vitale, V.; Vovk, I.; Walter, R.; Will, M.; Wunderlich, C.; Yamamoto, T.; Acharyya, A.; Adams, C. B.; Bangale, P.; Bartkoske, J. T.; Benbow, W.; Christiansen, J. L.; Duerr, A.; Errando, M.; Feng, Q.; Foote, J.; Fortson, L.; Furniss, A.; Hanlon, W.; Hervet, O.; Hinrichs, C. E.; Holder, J.; Humensky, T. B.; Jin, W.; Johnson, M. N.; Kaaret, P.; Kertzman, M.; Kieda, D.; Kleiner, T. K.; Korzoun, N.; Krennrich, F.; Kumar, S.; Lang, M. J.; Lundy, M.; Maier, G.; McGrath, C. E.; Millard, M. J.; Mooney, C. L.; Moriarty, P.; Mukherjee, R.; Ning, W.; O'Brien, S.; Ong, R. A.; Pohl, M.; Pueschel, E.; Quinn, J.; Ragan, K.; Reynolds, P. T.; Ribeiro, D.; Roache, E.; Ryan, J. L.; Sadeh, I.; Saha, L.; Santander, M.; Sembroski, G. H.; Shang, R.; Splettstoesser, M.; Talluri, A. K.; Tucci, J. V.; Valverde, J.; Vassiliev, V. V.; Williams, D. A.; Wong, S. L.; Chen, Z.; Cui, L.; Hirota, T.; Li, B.; Li, G.; Liu, Q.; Liu, X.; Liu, Z.; Ma, J.; Niinuma, K.; Ro, H.; Sakai, N.; Sawada-Satoh, S.; Wajima, K.; Wang, J.; Wang, N.; Xia, B.; Yan, H.; Yonekura, Y.; Zhang, H.; Zhao, R.; Zhong, W.Context. The nearby elliptical galaxy M87 contains one of only two supermassive black holes whose emission surrounding the event horizon has been imaged by the Event Horizon Telescope (EHT). In 2018, more than two dozen multi-wavelength (MWL) facilities (from radio to γ-ray energies) took part in the second M87 EHT campaign.Aims. The goal of this extensive MWL campaign was to better understand the physics of the accreting black hole M87*, the relationship between the inflow and inner jets, and the high-energy particle acceleration. Understanding the complex astrophysics is also a necessary first step towards performing further tests of general relativity.Methods. The MWL campaign took place in April 2018, overlapping with the EHT M87* observations. We present a new, contemporaneous spectral energy distribution (SED) ranging from radio to very high-energy (VHE) γ-rays as well as details of the individual observations and light curves. We also conducted phenomenological modelling to investigate the basic source properties.Results. We present the first VHE γ-ray flare from M87 detected since 2010. The flux above 350 GeV more than doubled within a period of ≈36 hours. We find that the X-ray flux is enhanced by about a factor of two compared to 2017, while the radio and millimetre core fluxes are consistent between 2017 and 2018. We detect evidence for a monotonically increasing jet position angle that corresponds to variations in the bright spot of the EHT image.Conclusions. Our results show the value of continued MWL monitoring together with precision imaging for addressing the origins of high-energy particle acceleration. While we cannot currently pinpoint the precise location where such acceleration takes place, the new VHE γ-ray flare already presents a challenge to simple one-zone leptonic emission model approaches, and it emphasises the need for combined image and spectral modelling. © The Authors 2024The Event Horizon Telescope Collaboration thanks the following organisations and programs: the Academia Sinica;
the Academy of Finland (projects 274477, 284495, 312496,
315721); the Agencia Nacional de Investigación y Desarrollo
(ANID), Chile via NCN19_058 (TITANs), Fondecyt 1221421
and BASAL FB210003; the Alexander von Humboldt Stiftung;
an Alfred P. Sloan Research Fellowship; Allegro, the European
ALMA Regional Centre node in the Netherlands, the NL astronomy research network NOVA and the astronomy institutes of
the University of Amsterdam, Leiden University, and Radboud
University; the ALMA North America Development Fund; the
Astrophysics and High Energy Physics programme by MCIN
(with funding from European Union NextGenerationEU, PRTRC17I1); the Black Hole Initiative, that is funded by grants from
the John Templeton Foundation (60477, 61497, 62286) and the
Gordon and Betty Moore Foundation (Grant GBMF-8273) -
although the opinions expressed in this work are those of the
author and do not necessarily reflect the views of these Foundations; the Brinson Foundation; “la Caixa” Foundation (ID
100010434) through fellowship codes LCF/BQ/DI22/11940027
and LCF/BQ/DI22/11940030; Chandra DD7-18089X and
TM6-17006X; the China Scholarship Council; the China
Postdoctoral Science Foundation fellowships (2020M671266,
2022M712084); Consejo Nacional de Humanidades, Ciencia
y Tecnología (CONAHCYT, Mexico, projects U0004-246083,
U0004-259839, F0003-272050, M0037-279006, F0003-
281692, 104497, 275201, 263356); the Colfuturo Scholarship;
the Consejería de Economía, Conocimiento, Empresas y
Universidad of the Junta de Andalucía (grant P18-FR-1769),
the Consejo Superior de Investigaciones Científicas (grant
2019AEP112); the Delaney Family via the Delaney Family
John A. Wheeler Chair at Perimeter Institute; Dirección General
de Asuntos del Personal Académico-Universidad Nacional
Autónoma de México (DGAPA-UNAM, projects IN112820
and IN108324); the Dutch Organization for Scientific Research
(NWO) for the VICI award (grant 639.043.513), the grant
OCENW.KLEIN.113, and the Dutch Black Hole Consortium
(with project No. NWA 1292.19.202) of the research programme
the National Science Agenda; the Dutch National Supercomputers, Cartesius and Snellius (NWO grant 2021.013); the EACOA
Fellowship awarded by the East Asia Core Observatories
Association, which consists of the Academia Sinica Institute
of Astronomy and Astrophysics, the National Astronomical
Observatory of Japan, Center for Astronomical Mega-Science,
Chinese Academy of Sciences, and the Korea Astronomy and
Space Science Institute; the European Research Council (ERC)
Synergy Grant “BlackHoleCam: Imaging the Event Horizon of
Black Holes" (grant 610058); the European Union Horizon 2020
research and innovation programme under grant agreements
RadioNet (No. 730562) and M2FINDERS (No. 101018682);
the European Research Council for advanced grant ‘JETSET:
Launching, propagation and emission of relativistic jets from
binary mergers and across mass scales’ (grant No. 884631); the
Horizon ERC Grants 2021 programme under grant agreement
No. 101040021; the FAPESP (Fundação de Amparo á Pesquisa
do Estado de São Paulo) under grant 2021/01183-8; the Fondo
CAS-ANID folio CAS220010; the Generalitat Valenciana
(grants APOSTD/2018/177 and ASFAE/2022/018) and GenT
Program (project CIDEGENT/2018/021); the Gordon and Betty
Moore Foundation (GBMF-3561, GBMF-5278, GBMF-10423);
the Institute for Advanced Study; the Istituto Nazionale di
Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche
TEONGRAV; the International Max Planck Research School
for Astronomy and Astrophysics at the Universities of Bonn
and Cologne; DFG research grant “Jet physics on horizon scales
and beyond” (grant No. 443220636); Joint Columbia/Flatiron
Postdoctoral Fellowship (research at the Flatiron Institute is
supported by the Simons Foundation); the Japan Ministry of
Education, Culture, Sports, Science and Technology (MEXT;
grant JPMXP1020200109); the Japan Society for the Promotion
of Science (JSPS) Grant-in-Aid for JSPS Research Fellowship
(JP17J08829); the Joint Institute for Computational Fundamental Science, Japan; the Key Research Program of Frontier
Sciences, Chinese Academy of Sciences (CAS, grants QYZDJSSW-SLH057, QYZDJSSW-SYS008, ZDBS-LY-SLH011);
the Leverhulme Trust Early Career Research Fellowship; the
Max-Planck-Gesellschaft (MPG); the Max Planck Partner
Group of the MPG and the CAS; the MEXT/JSPS KAKENHI
(grants 18KK0090, JP21H01137, JP18H03721, JP18K13594,
18K03709, JP19K14761, 18H01245, 25120007, 19H01943,
21H01137, 21H04488, 22H00157, 23K03453); the MICINN
Research Project PID2019-108995GB-C22; the MIT International Science and Technology Initiatives (MISTI) Funds;
the Ministry of Science and Technology (MOST) of Taiwan
(103-2119-M-001-010-MY2, 105-2112-M-001-025-MY3, 105-
2119-M-001-042, 106-2112-M-001-011, 106-2119-M-001-013,
106-2119-M-001-027, 106-2923-M-001-005, 107-2119-
M-001-017, 107-2119-M-001-020, 107-2119-M-001-041,
107-2119-M-110-005, 107-2923-M-001-009, 108-2112-M001-048, 108-2112-M-001-051, 108-2923-M-001-002, 109-
2112-M-001-025, 109-2124-M-001-005, 109-2923-M-001-001,
110-2112-M-001-033, 110-2124-M-001-007, 110-2923-M-001-
001, and 112-2112-M-003-010-MY3); the National Science and
Technology Council (NSTC) of Taiwan (111-2124-M-001-005,
112-2124-M-001-014); the Ministry of Education (MoE) of
Taiwan Yushan Young Scholar Program; the Physics Division, National Center for Theoretical Sciences of Taiwan; the
National Aeronautics and Space Administration (NASA, Fermi
Guest Investigator grant 80NSSC23K1508, NASA Astrophysics
Theory Program grant 80NSSC20K0527, NASA NuSTAR
award 80NSSC20K0645); NASA Hubble Fellowship grants
HST-HF2-51431.001-A, HST-HF2-51482.001-A awarded by
the Space Telescope Science Institute, which is operated by
the Association of Universities for Research in Astronomy,
Inc., for NASA, under contract NAS5-26555; the National
Institute of Natural Sciences (NINS) of Japan; the National
Key Research and Development Program of China (grant
2016YFA0400704, 2017YFA0402703, 2016YFA0400702); the
National Science and Technology Council (NSTC, grants NSTC
111-2112-M-001 -041, NSTC 111-2124-M-001-005, NSTC
112-2124-M-001-014); the US National Science Foundation
(NSF, grants AST-0096454, AST-0352953, AST-0521233,
AST-0705062, AST-0905844, AST-0922984, AST-1126433,
OIA-1126433, AST-1140030, DGE-1144085, AST-1207704,
AST-1207730, AST-1207752, MRI-1228509, OPP-1248097,
AST-1310896, AST-1440254, AST-1555365, AST-1614868,
AST-1615796, AST-1715061, AST-1716327, AST-1726637,
OISE-1743747, AST-1743747, AST-1816420, AST-1935980,
AST-1952099, AST-2034306, AST-2205908, AST-2307887);
NSF Astronomy and Astrophysics Postdoctoral Fellowship
(AST-1903847); the Natural Science Foundation of China
(grants 11650110427, 10625314, 11721303, 11725312,
11873028, 11933007, 11991052, 11991053, 12192220,
12192223, 12273022, 12325302); the Natural Sciences and
Engineering Research Council of Canada (NSERC, including
a Discovery Grant and the NSERC Alexander Graham Bell
Canada Graduate Scholarships-Doctoral Program); the National
Research Foundation of Korea (the Global PhD Fellowship
Grant: grants NRF-2015H1A2A1033752, the Korea Research
Fellowship Program: NRF-2015H1D3A1066561, Brain Pool
Program: 2019H1D3A1A01102564, Basic Research Support Grant 2019R1F1A1059721, 2021R1A6A3A01086420,
2022R1C1C1005255, 2022R1F1A1075115); Netherlands
Research School for Astronomy (NOVA) Virtual Institute of
Accretion (VIA) postdoctoral fellowships; NOIRLab, which
is managed by the Association of Universities for Research
in Astronomy (AURA) under a cooperative agreement with
the National Science Foundation; Onsala Space Observatory
(OSO) national infrastructure, for the provisioning of its
facilities/observational support (OSO receives funding through
the Swedish Research Council under grant 2017-00648);
the Perimeter Institute for Theoretical Physics (research at
Perimeter Institute is supported by the Government of Canada
through the Department of Innovation, Science and Economic
Development and by the Province of Ontario through the
Ministry of Research, Innovation and Science); the Princeton
Gravity Initiative; the Spanish Ministerio de Ciencia e Innovación (grants PGC2018-098915-B-C21, AYA2016-80889-P,
PID2019-108995GB-C21, PID2020-117404GB-C21); the
University of Pretoria for financial aid in the provision of
the new Cluster Server nodes and SuperMicro (USA) for a
SEEDING GRANT approved toward these nodes in 2020; the
Shanghai Municipality orientation program of basic research for
international scientists (grant no. 22JC1410600); the Shanghai
Pilot Program for Basic Research, Chinese Academy of Science,
Shanghai Branch (JCYJ-SHFY-2021-013); the State Agency
for Research of the Spanish MCIU through the “Center of
Excellence Severo Ochoa” award for the Instituto de Astrofísica
de Andalucía (SEV-2017- 0709); the Spanish Ministry for
Science and Innovation grant CEX2021-001131-S funded by
MCIN/AEI/10.13039/501100011033; the Spinoza Prize SPI
78-409; the South African Research Chairs Initiative, through
the South African Radio Astronomy Observatory (SARAO,
grant ID 77948), which
