{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:62NUPUPWNCQSVFXXPFN45OUWQJ","short_pith_number":"pith:62NUPUPW","schema_version":"1.0","canonical_sha256":"f69b47d1f668a12a96f7795bceba96825b5044efca2914de5ed500a48800b934","source":{"kind":"arxiv","id":"1804.05820","version":1},"attestation_state":"computed","paper":{"title":"GHASP: an H$\\alpha$ kinematical survey of spiral galaxies - XI. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using WISE photometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Benoit Epinat, Claude Carignan, Marie Korsaga, Philippe Amram, Tom Jarrett","submitted_at":"2018-04-16T17:43:47Z","abstract_excerpt":"We present the mass distribution of a sample of 121 nearby galaxies with high quality optical velocity fields and available infra-red $\\it{WISE}$ 3.4 $\\mu$m data. Contrary to previous studies, this sample covers all morphological types and is not biased toward late-type galaxies. These galaxies are part of the Fabry-Perot kinematical $\\it{GHASP}$ survey of spirals and irregular nearby galaxies. Combining the kinematical data to the $\\it{WISE}$ surface brightness data probing the emission from the old stellar population, we derive mass models allowing us to compare the luminous to the dark matt"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1804.05820","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-04-16T17:43:47Z","cross_cats_sorted":[],"title_canon_sha256":"c757d1e8f6b485aa8b468e483bccea4e97decbf6e05c7e8cfc182ac3ddfd81ef","abstract_canon_sha256":"c555d15bdb570c586136a2dff162a112903e2bbcc6b336818f999bc303cbe4b0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:17:03.143925Z","signature_b64":"SHGRao7+K2rv+eHArCEfZMLS9gUt3Gj01F4hUA/keURqlZoCWUa6D/scMHyroZJKaTOx12y6yw3Nom195OerDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f69b47d1f668a12a96f7795bceba96825b5044efca2914de5ed500a48800b934","last_reissued_at":"2026-05-18T00:17:03.143392Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:17:03.143392Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GHASP: an H$\\alpha$ kinematical survey of spiral galaxies - XI. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using WISE photometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Benoit Epinat, Claude Carignan, Marie Korsaga, Philippe Amram, Tom Jarrett","submitted_at":"2018-04-16T17:43:47Z","abstract_excerpt":"We present the mass distribution of a sample of 121 nearby galaxies with high quality optical velocity fields and available infra-red $\\it{WISE}$ 3.4 $\\mu$m data. Contrary to previous studies, this sample covers all morphological types and is not biased toward late-type galaxies. These galaxies are part of the Fabry-Perot kinematical $\\it{GHASP}$ survey of spirals and irregular nearby galaxies. Combining the kinematical data to the $\\it{WISE}$ surface brightness data probing the emission from the old stellar population, we derive mass models allowing us to compare the luminous to the dark matt"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.05820","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1804.05820","created_at":"2026-05-18T00:17:03.143484+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.05820v1","created_at":"2026-05-18T00:17:03.143484+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.05820","created_at":"2026-05-18T00:17:03.143484+00:00"},{"alias_kind":"pith_short_12","alias_value":"62NUPUPWNCQS","created_at":"2026-05-18T12:32:08.215937+00:00"},{"alias_kind":"pith_short_16","alias_value":"62NUPUPWNCQSVFXX","created_at":"2026-05-18T12:32:08.215937+00:00"},{"alias_kind":"pith_short_8","alias_value":"62NUPUPW","created_at":"2026-05-18T12:32:08.215937+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ","json":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ.json","graph_json":"https://pith.science/api/pith-number/62NUPUPWNCQSVFXXPFN45OUWQJ/graph.json","events_json":"https://pith.science/api/pith-number/62NUPUPWNCQSVFXXPFN45OUWQJ/events.json","paper":"https://pith.science/paper/62NUPUPW"},"agent_actions":{"view_html":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ","download_json":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ.json","view_paper":"https://pith.science/paper/62NUPUPW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.05820&json=true","fetch_graph":"https://pith.science/api/pith-number/62NUPUPWNCQSVFXXPFN45OUWQJ/graph.json","fetch_events":"https://pith.science/api/pith-number/62NUPUPWNCQSVFXXPFN45OUWQJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ/action/storage_attestation","attest_author":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ/action/author_attestation","sign_citation":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ/action/citation_signature","submit_replication":"https://pith.science/pith/62NUPUPWNCQSVFXXPFN45OUWQJ/action/replication_record"}},"created_at":"2026-05-18T00:17:03.143484+00:00","updated_at":"2026-05-18T00:17:03.143484+00:00"}