Bibliografisk note

Funding Information:
The Legacy Surveys consist of three individual and complementary projects: the Dark Energy Camera Legacy Survey (DECaLS; Proposal ID 2014B-0404; PIs David Schlegel and Arjun Dey), the Beijing–Arizona Sky Survey (BASS; Proposal ID 2015A-0801; PIs Zhou Xu and Xiaohui Fan), and the Mayall z-band Legacy Survey (MzLS; Proposal 2016A-0453; PI Arjun Dey). DECaLS, BASS, and MzLS together include data obtained (respectively) at the Blanco telescope, Cerro Tololo Inter-American Observatory, NSF’s NOIRLab; the Bok telescope, Steward Observatory, the University of Arizona; and the Mayall telescope, Kitt Peak National Observatory, NOIRLab. Pipeline processing and analyses of data were supported by NOIRLab and the Lawrence Berkeley National Laboratory (LBNL). The Legacy Surveys project is honored to be permitted to conduct astronomical research on Iolkam Du’ag (Kitt Peak), a mountain with particular significance to the Tohono O’odham Nation. NOIRLab is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NSF. LBNL is managed by the Regents of the University of California under contract to the U.S. Department of Energy.

Funding Information:
The UCSC team is supported in part by National Aeronautics and Space Administration (NASA) grant number 80NSSC20K0953, National Science Foundation (NSF) grant number AST-1815935, the Gordon & Betty Moore Foundation, the Heising–Simons Foundation, and by a fellowship from the David and Lucile Packard Foundation to RJF. CRA was supported by a VILLUM FONDEN Young Investigator grant (project number 25501). The DARK team was supported in part by a VILLUM FONDEN Investigator grant (project number 16599). DAC acknowledges support from the NSF Graduate Research Fellowship under grant number DGE-1339067. DOJ is supported by NASA through Hubble Fellowship grant HF2-51462.001 awarded by the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5–26555. PLK acknowledges support through NSF grant AST-1908823. The Las Cumbres group is supported by AST–1911151 and AST–1911225. MRS is supported by the STScI Postdoctoral Fellowship. CRB acknowledges the financial support from National Council for Scientific and Technological Development (CNPq) (316072/2021-4) and from Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ) (grants 201.456/2022 and 210.330/2022). Support for AVF’s group at U.C. Berkeley is provided by the Christopher R. Redlich Fund and many individual donors. LG acknowledges financial support from the Spanish Ministerio de Ciencia e Innovación (MCIN), the Agencia Estatal de Investigación (AEI) 10.13039/501100011033, and the European Social Fund (ESF) ‘Investing in your future’ under the 2019 Ramón y Cajal program RYC2019-027683-I and the PID2020-115253GA-I00 HOSTFLOWS project, from Centro Superior de Investigaciones Científicas (CSIC) under the PIE project 20215AT016, and the program Unidad de Excelencia María de Maeztu CEX2020-001058-M. FRH acknowledges funding from São Paulo Research Foundation (FAPESP) grants 2018/21661-9 and 2021/11345-5. CG is supported by a VILLUM FONDEN Young Investigator Grant (project number 25501). CL is supported by the NSF Graduate Research Fellowship under grant number DGE–2233066.

Funding Information:
A major upgrade of the Kast spectrograph on the Shane 3 m telescope at the Lick Observatory was made possible through generous gifts from the Heising–Simons Foundation as well as William and Marina Kast. Research at the Lick Observatory is partially supported by a generous gift from Google.

Funding Information:
This project used data obtained with the Dark Energy Camera (DECam), which was constructed by the Dark Energy Survey (DES) collaboration. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. NSF, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundacao Carlos Chagas Filho de Amparo, Financiadora de Estudos e Projetos, Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico and the Ministerio da Ciencia, Tecnologia e Inovacao, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are the Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid, the University of Chicago, the University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenossische Technische Hochschule (ETH) Zurich, the Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l’Espai (IEEC/CSIC), the Institut de Fisica d’Altes Energies, the Lawrence Berkeley National Laboratory, the Ludwig Maximilians Universitat Munchen and the associated Excellence Cluster Universe, the University of Michigan, NSF’s NOIRLab, the University of Nottingham, the Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, and Texas A&M University.

Funding Information:
A subset of the data presented herein were obtained at the W. M. Keck Observatory. NASA Keck time is administered by the NASA Exoplanet Science Institute. Data presented herein were obtained at the W. M. Keck Observatory from telescope time allocated to the National Aeronautics and Space Administration through the agency’s scientific partnership with the California Institute of Technology and the University of California. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.

Funding Information:
The UCSC team is supported in part by National Aeronautics and Space Administration (NASA) grant number 80NSSC20K0953, National Science Foundation (NSF) grant number AST-1815935, the Gordon & Betty Moore Foundation, the Heising-Simons Foundation, and by a fellowship from the David and Lucile Packard Foundation to RJF. CRA was supported by a VILLUM FONDEN Young Investigator grant (project number 25501). The DARK team was supported in part by a VILLUM FONDEN Investigator grant (project number 16599). DAC acknowledges support from the NSF Graduate Research Fellowship under grant number DGE- 1339067. DOJ is supported by NASA through Hubble Fellowship grant HF2-51462.001 awarded by the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. PLK acknowledges support through NSF grant AST1908823. The Las Cumbres group is supported by AST-1911151 and AST-1911225. MRS is supported by the STScI Postdoctoral Fellowship. CRB acknowledges the financial support from National Council for Scientific and Technological Development (CNPq) (316072/2021-4) and from Fundação de Amparo a Pesquisa do Estado do Rio de Janeiro (FAPERJ) (grants 201.456/2022 and 210.330/2022). Supportfor AVF's group at U.C.Berkeley is provided by the Christopher R. Redlich Fund and many individual donors. LG acknowledges financial support from the Spanish Ministerio de Ciencia e Innovacion (MCIN), the Agencia Estatal de Investigacion (AEI) 10.13039/501100011033, and the European Social Fund (ESF) 'Investing in your future' under the 2019 Ramon y Cajal program RYC2019-027683-I and the PID2020-115253GAI00 HOSTFLOWS project, from Centro Superior de Investigaciones Científicas (CSIC) under the PIE project 20215AT016, and the program Unidad de Excelencia María de Maeztu CEX2020-001058- M. FRH acknowledgesfunding from São Paulo Research Foundation (FAPESP) grants 2018/21661-9 and 2021/11345-5. CG is supported by a VILLUM FONDEN Young Investigator Grant (project number 25501). CL is supported by the NSF Graduate Research Fellowship under grant number DGE-2233066.

Funding Information:
This work has made use of data from the Asteroid Terrestrial-impact Last Alert System (ATLAS) project. The Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near-Earth objects (NEOs) through NASA grant numbers NN12AR55G, 80NSSC18K0284, and 80NSSC18K1575; byproducts of the NEO search include images and catalogs from the survey area. This work was partially funded by the Kepler/K2 grant J1944/80NSSC19K0112 and HST GO-15889, and STFC grants ST/T000198/1 and ST/S006109/1. The ATLAS science products have been made possible through the contributions of the University of Hawaii’s Institute for Astronomy, the Queen’s University Belfast, the Space Telescope Science Institute, the South African Astronomical Observatory, and the Millennium Institute of Astrophysics (MAS), Chile.

Funding Information:
Based in part on observations obtained at the Southern Astrophysical Research (SOAR) telescope [program 2021A-0242 (SOAR2022A-001); PI Dimitriadis], which is a joint project of the Ministério da Ciência, Tecnologia e Inovações (MCTI/LNA) do Brasil, the US NSF’s NOIRLab, the University of North Carolina at Chapel Hill (UNC), and the Michigan State University (MSU). Based in part on observations obtained at the international Gemini Observatory (program LP-204; PI Jacobson-Galan), a program of NSF’s NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NSF on behalf of the Gemini Observatory partnership: the NSF (United States), the National Research Council (Canada), the Agencia Nacional de Investigación y Desarrollo (Chile), the Ministerio de Ciencia, Tecnología e Innovación (Argentina), the Ministério da Ciência, Tecnologia, Inovações e Comunicações (Brazil), and the Korea Astronomy and Space Science Institute (Republic of Korea).

Funding Information:
The Young Supernova Experiment (YSE) and its research infrastructure is supported by the European Research Council under the European Union’s Horizon 2020 research and innovation programme (ERC grant agreement number 101002652, PI K. Mandel), the Heising–Simons Foundation (2018-0913, PI R. Foley; 2018–0911, PI R. Margutti), NASA (NNG17PX03C, PI R. Foley), NSF (AST-1720756, AST-1815935, PI R. Foley; AST-1909796, AST-1944985, PI R. Margutti), the David & Lucille Packard Foundation (PI R. Foley), VILLUM FONDEN (project 16599, PI J. Hjorth), and the Center for AstroPhysical Surveys (CAPS) at the National Center for Supercomputing Applications (NCSA) and the University of Illinois Urbana-Champaign.

Funding Information:
This work makes use of data from the Las Cumbres Observatory network. This publication has made use of data collected at the Lulin Observatory, partly supported by MoST grant number 108-2112-M-008-001. The S-PLUS project, including the T80-South robotic telescope and the S-PLUS scientific survey, was founded as a partnership between the Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), the Observatório Nacional (ON), the Federal University of Sergipe (UFS), and the Federal University of Santa Catarina (UFSC), with important financial and practical contributions from other collaborating institutes in Brazil, Chile (Universidad de La Serena), and Spain (Centro de Estudios de Física del Cosmos de Aragón, CEFCA). We further acknowledge financial support from the São Paulo Research Foundation (FAPESP), the Brazilian National Research Council (CNPq), the Coordination for the Improvement of Higher Education Personnel (CAPES), the Carlos Chagas Filho Rio de Janeiro State Research Foundation (FAPERJ), and the Brazilian Innovation Agency (FINEP).

Publisher Copyright:
© 2023 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.