{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:TY6VS7EPYGEGLV7XDV3736WKFN","short_pith_number":"pith:TY6VS7EP","schema_version":"1.0","canonical_sha256":"9e3d597c8fc18865d7f71d77fdfaca2b696ece65fd67a43a42af20e0a08a2319","source":{"kind":"arxiv","id":"1311.2941","version":1},"attestation_state":"computed","paper":{"title":"Ultraviolet Extinction at High Galactic Latitudes II: The Ultraviolet Extinction Function","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J.E.G. Peek","submitted_at":"2013-11-12T21:00:07Z","abstract_excerpt":"We present a dust-column--dependent extinction curve parameters for ultraviolet wavelengths at high Galactic latitudes. This extinction function diverges from previous work in that it takes into account the results of Peek & Schiminovich 2013 (Paper I), which demonstrated that there is more reddening in the GALEX bands than would be otherwise expected for E(B-V) < 0.2. We also test the biases in the Planck and SFD extinction maps, and find that the SFD extinction maps are significantly biased at E(B-V) < 0.2. We find that while an extinction function that that takes into account a varying R_FU"},"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":"1311.2941","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-11-12T21:00:07Z","cross_cats_sorted":[],"title_canon_sha256":"0c043a02a053855feb2a26ca4499ac6a4991faf669ae63c219256be86fa41f8b","abstract_canon_sha256":"ba0bc316b2d1fde74f07d8ece3df7c17adcc41504d0f1f2ede9c151693ce6937"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:07:13.608270Z","signature_b64":"2vyk9apdV+J5fjtfxQvtSOc1q284rLy3Zv02tSNu4jbWlCdbsS0ivNQVsV998z2eYwCj5lRJBfwWzwj/kMNEDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e3d597c8fc18865d7f71d77fdfaca2b696ece65fd67a43a42af20e0a08a2319","last_reissued_at":"2026-05-18T03:07:13.607517Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:07:13.607517Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ultraviolet Extinction at High Galactic Latitudes II: The Ultraviolet Extinction Function","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J.E.G. Peek","submitted_at":"2013-11-12T21:00:07Z","abstract_excerpt":"We present a dust-column--dependent extinction curve parameters for ultraviolet wavelengths at high Galactic latitudes. This extinction function diverges from previous work in that it takes into account the results of Peek & Schiminovich 2013 (Paper I), which demonstrated that there is more reddening in the GALEX bands than would be otherwise expected for E(B-V) < 0.2. We also test the biases in the Planck and SFD extinction maps, and find that the SFD extinction maps are significantly biased at E(B-V) < 0.2. We find that while an extinction function that that takes into account a varying R_FU"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.2941","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":"1311.2941","created_at":"2026-05-18T03:07:13.607646+00:00"},{"alias_kind":"arxiv_version","alias_value":"1311.2941v1","created_at":"2026-05-18T03:07:13.607646+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1311.2941","created_at":"2026-05-18T03:07:13.607646+00:00"},{"alias_kind":"pith_short_12","alias_value":"TY6VS7EPYGEG","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_16","alias_value":"TY6VS7EPYGEGLV7X","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_8","alias_value":"TY6VS7EP","created_at":"2026-05-18T12:28:02.375192+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/TY6VS7EPYGEGLV7XDV3736WKFN","json":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN.json","graph_json":"https://pith.science/api/pith-number/TY6VS7EPYGEGLV7XDV3736WKFN/graph.json","events_json":"https://pith.science/api/pith-number/TY6VS7EPYGEGLV7XDV3736WKFN/events.json","paper":"https://pith.science/paper/TY6VS7EP"},"agent_actions":{"view_html":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN","download_json":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN.json","view_paper":"https://pith.science/paper/TY6VS7EP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1311.2941&json=true","fetch_graph":"https://pith.science/api/pith-number/TY6VS7EPYGEGLV7XDV3736WKFN/graph.json","fetch_events":"https://pith.science/api/pith-number/TY6VS7EPYGEGLV7XDV3736WKFN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN/action/storage_attestation","attest_author":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN/action/author_attestation","sign_citation":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN/action/citation_signature","submit_replication":"https://pith.science/pith/TY6VS7EPYGEGLV7XDV3736WKFN/action/replication_record"}},"created_at":"2026-05-18T03:07:13.607646+00:00","updated_at":"2026-05-18T03:07:13.607646+00:00"}