Home › Core › ISCC-IDs › 28CrWDEgCzNyd

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Core Data

28CrWDEgCzNyd
ISCC-ID - digital asset identifier
CCdd2qsQ2sbzY-CTYHpYSdzsgWy-CDWDBNQ7e9oZf-CRPbLGW9aUxRB
ISCC-CODE - digital asset descriptor
2QTa5N4aeSrCB2MLoPdPF4AsTjstJgcLTnd
PUBLIC-KEY or WALLET-ADDRESS of DECLARING PARTY
0
Number of times updated

Seed Metadata (Immutable)

can stellar mass black holes be quark stars

Ledger Reference

coblo
Source Ledger/Blockchain
515304
N-th ISCC Decleration on source ledger
248d115dcc35abedf91d26e235f678539e8d0af91b978eaa272ad69e2ebb2c51
Hash of block that includes the ISCC-DECLARATION
965e5b3b8a343c94a12a5c15da75288df3f265629a69028129bd539564a4721f
Hash of transaction that includes the ISCC-DECLERATION
0
Output index that includes ISCC-DECLERATION (UTXO based chains)

Mutable Metadata

[{"data": {"name": "Can stellar mass black holes be quark stars?", "@type": "ScholarlyArticle", "genre": "journal-article", "author": [{"name": "Z. Kov\u00c3\u00a1cs", "@type": "Person"}, {"name": "K. S. Cheng", "@type": "Person"}, {"name": "T. Harko", "@type": "Person"}], "@context": "http://schema.org/", "encoding": [{"@type": "MediaObject", "contentUrl": "https://academic.oup.com/mnras/article-pdf/400/3/1632/2852793/mnras0400-1632.pdf", "encodingFormat": "application/pdf"}], "publisher": {"name": "Oxford University Press (OUP)", "@type": "Organization"}, "identifier": [{"@type": "PropertyValue", "value": "10.1111/j.1365-2966.2009.15571.x", "propertyID": "DOI"}, {"@type": "PropertyValue", "value": "CCdd2qsQ2sbzY-CTYHpYSdzsgWy-CDWDBNQ7e9oZf-CRPbLGW9aUxRB", "propertyID": "ISCC"}], "datePublished": "2009-12-11"}, "schema": "schema.org", "mediatype": "application/ld+json"}]
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