The Outbursting YSOs Catalogue (OYCAT)
Carlos Contreras Peña, Jeong‐Eun Lee, G. J. Herczeg, Doug Johnstone, P. Ábrahám, S. Antoniucci, M. Audard, Muhammad Ashraf, Giseon Baek, A. Caratti o Garatti, Airton Torres Carvalho, Lucas A. Cieza, Fernando Cruz-Sáenz de Miera, J. Eislöffel, D. Froebrich, T. Giannini, J. Green, Arindam Ghosh, Zhe Guo, L. Hillenbrand, K. W. Hodapp, H. Jheonn, J. José, Yongman Kim, Á. Kóspál, Hyung-Ik Lee, P. W. Lucas, T. Yu. Magakian, Z. Nagy, T. Naylor, Joe P. Ninan, S. Peneva, Bo Reipurth, A. Scholz, E. Semkov, A. Sicilia-Aguilar, Krishna Kant Singh, M. Siwak, B. Stecklum, Zsófia Marianna Szabó, V. Wolf, Sehyoun Yoon
Abstract
Funding: C.C.P. was supported by the National Research Foundation of Korea (NRF) grant funded by the Korean government (MEST) (No. 2019R1A6A1A10073437). J.E.L. was supported by the New Faculty Startup Fund from Seoul National University and the NRF grant funded by the Korean government (MSIT) (grant number 2021R1A2C1011718 and RS-2024-00416859). GJH is supported by the National Key R&D program of China 2022YFA1603102 and by general grant 12173003 from the National Natural Science Foundation of China. D.J. is supported by NRC Canada and by an NSERC Discovery Grant. A.K. was supported by the NKFIH excellence grant TKP2021-NKTA-64. Zs.N. acknowledges the Hungarian National Research, Development and Innovation Office grant OTKA FK 146023. Zs.N. was supported by the János Bolyai Research Scholarship of the Hungarian Academy of Sciences. Zs.N. acknowledges support from the ESA PRODEX contract No. 4000132054. Zs.M.Sz. acknowledges funding from a St. Leonards scholarship from the University of St. Andrews. Zs.M.Sz. is a member of the International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne. A.C.G. acknowledges support from PRIN-MUR 2022 20228JPA3A “The path to star and planet formation in the JWST era (PATH)” funded by NextGeneration EU and by INAF-GoG 2022 “NIR-dark Accretion Outbursts in Massive Young stellar objects (NAOMY)” and Large Grant INAF 2022 “YSOs Outflows, Disks and Accretion: towards a global framework for the evolution of planet forming systems (YODA)”. F.C.S.M. received financial support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (ERC Starting Grant “Chemtrip”, grant agreement No 949278). G.B was supported by Basic Science Research Program through the National Research Foundation ofKorea(NRF) funded by the Ministry of Education(grant number RS-2023-00247790). Z.G. is funded by ANID, Millennium Science Initiative, AIM23-001. Z.G. is supported by the China-Chile Joint Research Fund (CCJRF No.2301) and Chinese Academy of Science South America Center for Astronomy (CASSACA) Key Research Project E52H540301. This work was also supported by the NKFIHNKKPgrantADVANCED149943. Project no.149943 has been implemented with the support provided by the Ministry of Culture and Innovation of Hungary from the National Research, Development and Innovation Fund, financed under the NKKP ADVANCED funding scheme.