{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:N5DDBEJVQ3MNVOGYT3FNKSZ5EA","short_pith_number":"pith:N5DDBEJV","schema_version":"1.0","canonical_sha256":"6f4630913586d8dab8d89ecad54b3d202f9ba6dcda7283e6eeb7fc114ecd73b2","source":{"kind":"arxiv","id":"1810.01208","version":1},"attestation_state":"computed","paper":{"title":"The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Nersesian, A. P. Jones, A. Tr\\v{c}ka, A. V. Mosenkov, C. J. R. Clark, E. M. Xilouris, F. Galliano, I. De Looze, J. I. Davies, L. P. Cassar\\`a, M. Baes, M. Galametz, P. De Vis, S. Bianchi, S. C. Madden, S. Lianou, S. Viaene, V. Casasola, W. Dobbels","submitted_at":"2018-10-02T12:45:36Z","abstract_excerpt":"We study the fraction of stellar radiation absorbed by dust, f_abs, in 814 galaxies of different morphological types. The targets constitute the vast majority (93%) of the DustPedia sample, including almost all large (optical diameter larger than 1'), nearby (v <= 3000 km/s) galaxies observed with the Herschel Space Observatory. For each object, we model the spectral energy distribution from the ultraviolet to the sub-millimetre using the dedicated, aperture-matched DustPedia photometry and the fitting code CIGALE. The value of f_abs is obtained from the total luminosity emitted by dust and fr"},"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":"1810.01208","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-10-02T12:45:36Z","cross_cats_sorted":[],"title_canon_sha256":"a9b47d53d9cd66e6f146f184d84e73e5b6974043a2d7adf02d01d27e87813cd0","abstract_canon_sha256":"d9b98ce47904db64c0b9750ac3aca9729354f0a4d66b0e4874e80652723b2239"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:37.384146Z","signature_b64":"m8VNVBo7xg7GOg+u21Y3J+HrFOh0jr2HdiWeTmqjBtRKdGaTgQhWzIjnnns63UN5z65aNrV4Sx9JfoOu13geAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6f4630913586d8dab8d89ecad54b3d202f9ba6dcda7283e6eeb7fc114ecd73b2","last_reissued_at":"2026-05-17T23:58:37.383439Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:37.383439Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Nersesian, A. P. Jones, A. Tr\\v{c}ka, A. V. Mosenkov, C. J. R. Clark, E. M. Xilouris, F. Galliano, I. De Looze, J. I. Davies, L. P. Cassar\\`a, M. Baes, M. Galametz, P. De Vis, S. Bianchi, S. C. Madden, S. Lianou, S. Viaene, V. Casasola, W. Dobbels","submitted_at":"2018-10-02T12:45:36Z","abstract_excerpt":"We study the fraction of stellar radiation absorbed by dust, f_abs, in 814 galaxies of different morphological types. The targets constitute the vast majority (93%) of the DustPedia sample, including almost all large (optical diameter larger than 1'), nearby (v <= 3000 km/s) galaxies observed with the Herschel Space Observatory. For each object, we model the spectral energy distribution from the ultraviolet to the sub-millimetre using the dedicated, aperture-matched DustPedia photometry and the fitting code CIGALE. The value of f_abs is obtained from the total luminosity emitted by dust and fr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.01208","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":"1810.01208","created_at":"2026-05-17T23:58:37.383558+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.01208v1","created_at":"2026-05-17T23:58:37.383558+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.01208","created_at":"2026-05-17T23:58:37.383558+00:00"},{"alias_kind":"pith_short_12","alias_value":"N5DDBEJVQ3MN","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_16","alias_value":"N5DDBEJVQ3MNVOGY","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_8","alias_value":"N5DDBEJV","created_at":"2026-05-18T12:32:40.477152+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/N5DDBEJVQ3MNVOGYT3FNKSZ5EA","json":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA.json","graph_json":"https://pith.science/api/pith-number/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/graph.json","events_json":"https://pith.science/api/pith-number/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/events.json","paper":"https://pith.science/paper/N5DDBEJV"},"agent_actions":{"view_html":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA","download_json":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA.json","view_paper":"https://pith.science/paper/N5DDBEJV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.01208&json=true","fetch_graph":"https://pith.science/api/pith-number/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/graph.json","fetch_events":"https://pith.science/api/pith-number/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/action/storage_attestation","attest_author":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/action/author_attestation","sign_citation":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/action/citation_signature","submit_replication":"https://pith.science/pith/N5DDBEJVQ3MNVOGYT3FNKSZ5EA/action/replication_record"}},"created_at":"2026-05-17T23:58:37.383558+00:00","updated_at":"2026-05-17T23:58:37.383558+00:00"}