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Hubble resolved-star catalogues

Dataset

No article has been written for this page yet; it is generated from the knowledge graph.
  • Faint stellar structure detection Key work
    It starts from resolved-star catalogues from the Hubble Space Telescope for the galaxies M81 and M82: Prepare the catalogues, keeping each telescope field's geometry so every star can be traced back to its source.
  • KIWIS Jul 2026
    The first ledger, KWS–ASTRO–001, documents how resolved-star catalogues from the Hubble Space Telescope become evidence for faint structure around the galaxies M81 and M82.
  • Figure archive
    It covers resolved stellar populations and faint substructure around two contrasting nearby galaxies, from the overlapping fields of the Hubble Space Telescope surveys of M81 and M82, through duplicate removal, density maps and substructure detection, to validation.

In the knowledge graph

Hubble resolved-star catalogues and the 3 things it is linked to. Open any dot for its page, or explore it in the full graph.

As data

Everything on this page is read from triples in the knowledge graph. These are the 3 it states about Hubble resolved-star catalogues, and 1 more its ontology implies; the console runs SPARQL over the whole graph, here in your browser.

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@prefix id: <https://ask.chaipat.cc/id/> .
@prefix rdf: <http://www.w3.org/1999/02/22-rdf-syntax-ns#> .
@prefix cj: <https://ask.chaipat.cc/ns#> .
@prefix rdfs: <http://www.w3.org/2000/01/rdf-schema#> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .

id:HSTCatalogs
    a cj:Dataset ;
    rdfs:label "Hubble resolved-star catalogues" ;
    skos:altLabel "Hubble Space Telescope" .