{"paper":{"title":"Galaxy morphology to I=25 mag in the Hubble Deep Field","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. X. Santiago, K. Glazebrook, N. R. Tanvir, R. G. Abraham, R. S. Ellis, S. van den Bergh","submitted_at":"1996-02-09T02:23:57Z","abstract_excerpt":"The morphological properties of galaxies between $21 {\\rm~mag} < I < 25 {\\rm~mag}$ in the {\\em Hubble Deep Field} are investigated using a quantitative classification system based on measurements of the central concentration and asymmetry of galaxian light. The class distribution of objects in the {\\em Hubble Deep Field} is strongly skewed towards highly asymmetric objects, relative to distributions from both the {\\em HST Medium Deep Survey} at $I < 22 {\\rm~mag}$ and an artificially redshifted sample of local galaxies. The steeply rising number count-magnitude relation for irregular/peculiar/m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9602044","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}