{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:SSFWAX4HCOI6FHAHYZJ45XPTAR","short_pith_number":"pith:SSFWAX4H","schema_version":"1.0","canonical_sha256":"948b605f871391e29c07c653ceddf3047d9053d867c60ef92e954497a32422a0","source":{"kind":"arxiv","id":"1603.07764","version":3},"attestation_state":"computed","paper":{"title":"Analysis of the Intrinsic Mid-Infrared L-band to Visible--Near-Infrared Flux Ratios in Spectral Synthesis Models of Composite Stellar Populations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Duho Kim, Rogier A. Windhorst, Rolf A. Jansen","submitted_at":"2016-03-24T21:56:31Z","abstract_excerpt":"We analyze the intrinsic flux ratios of various visible--near-infrared filters with respect to 3.5micron for simple and composite stellar populations, and their dependence on age, metallicity and star formation history. UV/optical light from stars is reddened and attenuated by dust, where different sightlines across a galaxy suffer varying amounts of extinction. Tamura et al. (2009) developed an approximate method to correct for dust extinction on a pixel-by-pixel basis, dubbed the \"beta_V\" method, by comparing the observed flux ratio to an empirical estimate of the intrinsic ratio of visible "},"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":"1603.07764","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-03-24T21:56:31Z","cross_cats_sorted":[],"title_canon_sha256":"0461f06615d50dae19565dc9fcccd19c974b7b502808b41232497969d6e7acd0","abstract_canon_sha256":"f1df7d1608f19ce986031488256f60e7a4ec46f816b5c3fe14c0fc3aa2a87b28"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:44:38.968007Z","signature_b64":"2HTPHV+l/uW01RABjiD1S3F00xhavVIfxraZBkce4/FrjyhnlSTCDtpj8hugeePaEFQovgBDQ8OyZFDOrdd+Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"948b605f871391e29c07c653ceddf3047d9053d867c60ef92e954497a32422a0","last_reissued_at":"2026-05-18T00:44:38.967565Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:44:38.967565Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Analysis of the Intrinsic Mid-Infrared L-band to Visible--Near-Infrared Flux Ratios in Spectral Synthesis Models of Composite Stellar Populations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Duho Kim, Rogier A. Windhorst, Rolf A. Jansen","submitted_at":"2016-03-24T21:56:31Z","abstract_excerpt":"We analyze the intrinsic flux ratios of various visible--near-infrared filters with respect to 3.5micron for simple and composite stellar populations, and their dependence on age, metallicity and star formation history. UV/optical light from stars is reddened and attenuated by dust, where different sightlines across a galaxy suffer varying amounts of extinction. Tamura et al. (2009) developed an approximate method to correct for dust extinction on a pixel-by-pixel basis, dubbed the \"beta_V\" method, by comparing the observed flux ratio to an empirical estimate of the intrinsic ratio of visible "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.07764","kind":"arxiv","version":3},"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":"1603.07764","created_at":"2026-05-18T00:44:38.967639+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.07764v3","created_at":"2026-05-18T00:44:38.967639+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.07764","created_at":"2026-05-18T00:44:38.967639+00:00"},{"alias_kind":"pith_short_12","alias_value":"SSFWAX4HCOI6","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"SSFWAX4HCOI6FHAH","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"SSFWAX4H","created_at":"2026-05-18T12:30:44.179134+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/SSFWAX4HCOI6FHAHYZJ45XPTAR","json":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR.json","graph_json":"https://pith.science/api/pith-number/SSFWAX4HCOI6FHAHYZJ45XPTAR/graph.json","events_json":"https://pith.science/api/pith-number/SSFWAX4HCOI6FHAHYZJ45XPTAR/events.json","paper":"https://pith.science/paper/SSFWAX4H"},"agent_actions":{"view_html":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR","download_json":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR.json","view_paper":"https://pith.science/paper/SSFWAX4H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.07764&json=true","fetch_graph":"https://pith.science/api/pith-number/SSFWAX4HCOI6FHAHYZJ45XPTAR/graph.json","fetch_events":"https://pith.science/api/pith-number/SSFWAX4HCOI6FHAHYZJ45XPTAR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR/action/storage_attestation","attest_author":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR/action/author_attestation","sign_citation":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR/action/citation_signature","submit_replication":"https://pith.science/pith/SSFWAX4HCOI6FHAHYZJ45XPTAR/action/replication_record"}},"created_at":"2026-05-18T00:44:38.967639+00:00","updated_at":"2026-05-18T00:44:38.967639+00:00"}