The Outbursting YSOs Catalogue (OYCAT)

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.

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Publication Details

Journal
Kent Academic Repository (University of Kent)
Published
2025-09-29
DOI
https://doi.org/10.5303/jkas.2025.58.2.209
Citations
4
Primary Topic
Geophysics and Gravity Measurements
Type
article
Field-Weighted Citation Impact
7.17

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article

The Outbursting YSOs Catalogue (OYCAT)

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4 citations
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The Outbursting YSOs Catalogue (OYCAT)

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article en
4 citations

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.

Kent Academic Repository (University of Kent)
National Aeronautics and Space Administration, California Institute of Technology, Chinese Academy of Sciences South America Center for Astronomy, International Max Planck Research School for Environmental, Cellular and Molecular Microbiology, University of St Andrews, European Commission, National Research Foundation, National Natural Science Foundation of China, Seoul National University, Hungarian Scientific Research Fund, National Research Foundation of Korea, Magyar Tudományos Akadémia, Nemzeti Kutatási Fejlesztési és Innovációs Hivatal, International Max Planck Research School for Advanced Methods in Process and Systems Engineering, Ministry of Science and ICT, South Korea, Agencia Nacional de Investigación y Desarrollo, Jet Propulsion Laboratory, University of California, Los Angeles, Natural Sciences and Engineering Research Council of Canada, Nemzeti Kutatási, Fejlesztési és Innovaciós Alap, National Research, Development and Innovation Office
Openalex Percentile: Top 3%
Geophysics and Gravity Measurements
7.17
DOIOpen Access PDFOpenAlex
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