{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:EGSJPVOUQCFWUPEQCE5WVXFB7H","short_pith_number":"pith:EGSJPVOU","schema_version":"1.0","canonical_sha256":"21a497d5d4808b6a3c90113b6adca1f9c6dbfa4a2ace77a5e62669c801e21a9c","source":{"kind":"arxiv","id":"1403.7527","version":1},"attestation_state":"computed","paper":{"title":"The distribution of interstellar dust in CALIFA edge-on galaxies via oligochromatic radiative transfer fitting","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Gert De Geyter, Gianfranco Gentile, Ilse De Looze, Jacopo Fritz, Maarten Baes, Peter Camps, Sebastien Viaene, Thomas M. Hughes","submitted_at":"2014-03-28T20:00:16Z","abstract_excerpt":"We investigate the amount and spatial distribution of interstellar dust in edge-on spiral galaxies, using detailed radiative transfer modeling of a homogeneous sample of 12 galaxies selected from the CALIFA survey. Our automated fitting routine, FitSKIRT, was first validated against artificial data. This is done by simultaneously reproducing the SDSS $g$-, $r$-, $i$- and $z$-band observations of a toy model in order to combine the information present in the different bands. We show that this combined, oligochromatic fitting, has clear advantages over standard monochromatic fitting especially r"},"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":"1403.7527","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-28T20:00:16Z","cross_cats_sorted":[],"title_canon_sha256":"cef1e1f0890965c9d1f7cf876e3de030590827f703ff997428052c36e19c3ac3","abstract_canon_sha256":"2ee7f3223319f2c48365b855d3d0f104dbae4e890ffabfeb93ba755a9c5f1716"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:44.197207Z","signature_b64":"rb7yGwnN4onOpgf+bBV7iP+b9tKy+lH7k6xuSVqURHijs2vZYEk3Z5XTTu2OKV2DTOkDc1VJ51awTRZEqXugDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"21a497d5d4808b6a3c90113b6adca1f9c6dbfa4a2ace77a5e62669c801e21a9c","last_reissued_at":"2026-05-18T01:43:44.196552Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:44.196552Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The distribution of interstellar dust in CALIFA edge-on galaxies via oligochromatic radiative transfer fitting","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Gert De Geyter, Gianfranco Gentile, Ilse De Looze, Jacopo Fritz, Maarten Baes, Peter Camps, Sebastien Viaene, Thomas M. Hughes","submitted_at":"2014-03-28T20:00:16Z","abstract_excerpt":"We investigate the amount and spatial distribution of interstellar dust in edge-on spiral galaxies, using detailed radiative transfer modeling of a homogeneous sample of 12 galaxies selected from the CALIFA survey. Our automated fitting routine, FitSKIRT, was first validated against artificial data. This is done by simultaneously reproducing the SDSS $g$-, $r$-, $i$- and $z$-band observations of a toy model in order to combine the information present in the different bands. We show that this combined, oligochromatic fitting, has clear advantages over standard monochromatic fitting especially r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.7527","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":"1403.7527","created_at":"2026-05-18T01:43:44.196663+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.7527v1","created_at":"2026-05-18T01:43:44.196663+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.7527","created_at":"2026-05-18T01:43:44.196663+00:00"},{"alias_kind":"pith_short_12","alias_value":"EGSJPVOUQCFW","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_16","alias_value":"EGSJPVOUQCFWUPEQ","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_8","alias_value":"EGSJPVOU","created_at":"2026-05-18T12:28:25.294606+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/EGSJPVOUQCFWUPEQCE5WVXFB7H","json":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H.json","graph_json":"https://pith.science/api/pith-number/EGSJPVOUQCFWUPEQCE5WVXFB7H/graph.json","events_json":"https://pith.science/api/pith-number/EGSJPVOUQCFWUPEQCE5WVXFB7H/events.json","paper":"https://pith.science/paper/EGSJPVOU"},"agent_actions":{"view_html":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H","download_json":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H.json","view_paper":"https://pith.science/paper/EGSJPVOU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.7527&json=true","fetch_graph":"https://pith.science/api/pith-number/EGSJPVOUQCFWUPEQCE5WVXFB7H/graph.json","fetch_events":"https://pith.science/api/pith-number/EGSJPVOUQCFWUPEQCE5WVXFB7H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H/action/storage_attestation","attest_author":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H/action/author_attestation","sign_citation":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H/action/citation_signature","submit_replication":"https://pith.science/pith/EGSJPVOUQCFWUPEQCE5WVXFB7H/action/replication_record"}},"created_at":"2026-05-18T01:43:44.196663+00:00","updated_at":"2026-05-18T01:43:44.196663+00:00"}