{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:4GCHUDILCG3IV4A44IHCNP3FK5","short_pith_number":"pith:4GCHUDIL","schema_version":"1.0","canonical_sha256":"e1847a0d0b11b68af01ce20e26bf65577fad872fde3c7ae9fc6beffa6b12f144","source":{"kind":"arxiv","id":"1302.1379","version":1},"attestation_state":"computed","paper":{"title":"GAMA/H-ATLAS: The Dust Opacity - Stellar Mass Surface Density Relation for Spiral Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cooray, A. Dariush, A.M. Hopkins, A.S.G. Robotham, A.W. Graham, B.F. Madore, B. Pastrav, C.C. Popescu, D.J.B. Smith, D. Thomas, E. Andrae, E.N. Taylor, E. Valiante, G. de Zotti, H. Gomez, H.R. Parkinson, I.K. Baldry, J. Liske, J. Loveday, L. Dunne, L.S. Kelvin, M. Baes, M. Gunawardhana, M. Jarvis, M.J. Micha{\\l}owski, M. Prescott, M. Seibert, M.W. Grootes, N. Bourne, P. Norberg, R. Hopwood, R.J. Tuffs, S. Brough, S. Maddox, S.P. Driver","submitted_at":"2013-02-06T14:17:16Z","abstract_excerpt":"We report the discovery of a well-defined correlation between B-band face-on central optical depth due to dust, \\tau^f_B, and the stellar mass surface density, \\mu_{*}, of nearby (z < 0.13) spiral galaxies: log(\\tau^f_B) = 1.12(+-0.11)log(\\mu_{*}/M_sol kpc^2)-8.6(+-0.8). This relation was derived from a sample of spiral galaxies taken from the Galaxy and Mass Assembly (GAMA) survey and detected in the FIR/submm in the Herschel-ATLAS survey. Using a quantitative analysis of the NUV attenuation-inclination relation for complete samples of GAMA spirals categorized according to \\mu_{*} we demonstr"},"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":"1302.1379","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-06T14:17:16Z","cross_cats_sorted":[],"title_canon_sha256":"71407a0a87a07a486fa699f0e9426782f24144edd9476bf6bbaab7b8ae6d4f14","abstract_canon_sha256":"53e18827bfb7833cf76875d49cfa562d00c85e8557403630641e4692dc3ce205"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:49.816506Z","signature_b64":"45C1WknxeOOYBTk6gFbO6FRpPyVzKbojwjOtcqSv7pVwWo34ZubYdr3kPxv5mpJdpHMGMOT0R9IuFd+7GoyzBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e1847a0d0b11b68af01ce20e26bf65577fad872fde3c7ae9fc6beffa6b12f144","last_reissued_at":"2026-05-18T01:51:49.815919Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:49.815919Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GAMA/H-ATLAS: The Dust Opacity - Stellar Mass Surface Density Relation for Spiral Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cooray, A. Dariush, A.M. Hopkins, A.S.G. Robotham, A.W. Graham, B.F. Madore, B. Pastrav, C.C. Popescu, D.J.B. Smith, D. Thomas, E. Andrae, E.N. Taylor, E. Valiante, G. de Zotti, H. Gomez, H.R. Parkinson, I.K. Baldry, J. Liske, J. Loveday, L. Dunne, L.S. Kelvin, M. Baes, M. Gunawardhana, M. Jarvis, M.J. Micha{\\l}owski, M. Prescott, M. Seibert, M.W. Grootes, N. Bourne, P. Norberg, R. Hopwood, R.J. Tuffs, S. Brough, S. Maddox, S.P. Driver","submitted_at":"2013-02-06T14:17:16Z","abstract_excerpt":"We report the discovery of a well-defined correlation between B-band face-on central optical depth due to dust, \\tau^f_B, and the stellar mass surface density, \\mu_{*}, of nearby (z < 0.13) spiral galaxies: log(\\tau^f_B) = 1.12(+-0.11)log(\\mu_{*}/M_sol kpc^2)-8.6(+-0.8). This relation was derived from a sample of spiral galaxies taken from the Galaxy and Mass Assembly (GAMA) survey and detected in the FIR/submm in the Herschel-ATLAS survey. Using a quantitative analysis of the NUV attenuation-inclination relation for complete samples of GAMA spirals categorized according to \\mu_{*} we demonstr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.1379","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":"1302.1379","created_at":"2026-05-18T01:51:49.815990+00:00"},{"alias_kind":"arxiv_version","alias_value":"1302.1379v1","created_at":"2026-05-18T01:51:49.815990+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.1379","created_at":"2026-05-18T01:51:49.815990+00:00"},{"alias_kind":"pith_short_12","alias_value":"4GCHUDILCG3I","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"4GCHUDILCG3IV4A4","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"4GCHUDIL","created_at":"2026-05-18T12:27:34.582898+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/4GCHUDILCG3IV4A44IHCNP3FK5","json":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5.json","graph_json":"https://pith.science/api/pith-number/4GCHUDILCG3IV4A44IHCNP3FK5/graph.json","events_json":"https://pith.science/api/pith-number/4GCHUDILCG3IV4A44IHCNP3FK5/events.json","paper":"https://pith.science/paper/4GCHUDIL"},"agent_actions":{"view_html":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5","download_json":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5.json","view_paper":"https://pith.science/paper/4GCHUDIL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1302.1379&json=true","fetch_graph":"https://pith.science/api/pith-number/4GCHUDILCG3IV4A44IHCNP3FK5/graph.json","fetch_events":"https://pith.science/api/pith-number/4GCHUDILCG3IV4A44IHCNP3FK5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5/action/storage_attestation","attest_author":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5/action/author_attestation","sign_citation":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5/action/citation_signature","submit_replication":"https://pith.science/pith/4GCHUDILCG3IV4A44IHCNP3FK5/action/replication_record"}},"created_at":"2026-05-18T01:51:49.815990+00:00","updated_at":"2026-05-18T01:51:49.815990+00:00"}