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The research leading to these results has received funding from the LP2018-7 Lendulet grant of the Hungarian Academy of Sciences.; Funding for the SDSS-IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. 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The observed sample of such events is still low, and their nature is still under debate. Such SNe are similar to SN 2005cs, a well-observed LL Type II-P event, having low expansion velocit...", "source" : { "otype" : "PlainSource", "mtid" : 148, "link" : "/api/publicationsource/148", "label" : "ADS", "type" : { "otype" : "PublicationSourceType", "mtid" : 10003, "link" : "/api/publicationsourcetype/10003", "label" : "Indexelő adatbázis", "mayHaveOa" : false, "published" : true, "snippet" : true }, "name" : "ADS", "nameEng" : "ADS", "linkPattern" : "http://adsabs.harvard.edu/abs/@@@", "publiclyVisible" : true, "published" : true, "oldId" : 148, "snippet" : true }, "validState" : "IDENTICAL", "idValue" : "2020MNRAS.496.3725J luminosity Type II-P supernova (LL SN IIP). The observed sample of such events is still low, and their nature is still under debate. Such SNe are similar to SN 2005cs, a well-observed LL Type II-P event, having low expansion velocities, and small ejected 56Ni mass. 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