{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:AV4W4RBBQS4A6PMLGSZFJBKKZE","short_pith_number":"pith:AV4W4RBB","schema_version":"1.0","canonical_sha256":"05796e442184b80f3d8b34b254854ac92ce5924fdba712455dcdf105a797b677","source":{"kind":"arxiv","id":"1403.1368","version":2},"attestation_state":"computed","paper":{"title":"On calibration of some distance scales in astrophysics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"B. Arbutina, B. Vukotic, D. Urosevic, M. Jurkovic","submitted_at":"2014-03-06T07:54:23Z","abstract_excerpt":"We present a method for distance calibration without using standard fitting procedures. Instead we use random resampling to reconstruct the probability density function (PDF) of calibration data points in the fitting plane. The resulting PDF is then used to estimate distance-related properties. The method is applied to samples of radio surface brightness to diameter (\\Sigma-D) data for the Galactic supernova remnants (SNRs) and planetary nebulae (PNe), and period-luminosity (PL) data for the Large Magellanic Cloud (LMC) fundamental mode classical Cepheids. We argue that resulting density maps "},"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":"1403.1368","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2014-03-06T07:54:23Z","cross_cats_sorted":[],"title_canon_sha256":"d07e2f02b7e35469cb54e1804b9bda050f2105688202feef4233f9619983622a","abstract_canon_sha256":"46fabe5c4a837c0633169870eed8936a20b4f33d62532f4b43ed4ab0d854f0be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:54:30.231176Z","signature_b64":"ctLk0yA/7zADyaXnj74jAl6mX/0cCD5lo7Oeu6W6WkgwanRfvAfIZnAIlYiDwRgTeFftLzDXwrnaukWrL9zBBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"05796e442184b80f3d8b34b254854ac92ce5924fdba712455dcdf105a797b677","last_reissued_at":"2026-05-18T02:54:30.230652Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:54:30.230652Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On calibration of some distance scales in astrophysics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"B. Arbutina, B. Vukotic, D. Urosevic, M. Jurkovic","submitted_at":"2014-03-06T07:54:23Z","abstract_excerpt":"We present a method for distance calibration without using standard fitting procedures. Instead we use random resampling to reconstruct the probability density function (PDF) of calibration data points in the fitting plane. The resulting PDF is then used to estimate distance-related properties. The method is applied to samples of radio surface brightness to diameter (\\Sigma-D) data for the Galactic supernova remnants (SNRs) and planetary nebulae (PNe), and period-luminosity (PL) data for the Large Magellanic Cloud (LMC) fundamental mode classical Cepheids. We argue that resulting density maps "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.1368","kind":"arxiv","version":2},"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":"1403.1368","created_at":"2026-05-18T02:54:30.230719+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.1368v2","created_at":"2026-05-18T02:54:30.230719+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.1368","created_at":"2026-05-18T02:54:30.230719+00:00"},{"alias_kind":"pith_short_12","alias_value":"AV4W4RBBQS4A","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_16","alias_value":"AV4W4RBBQS4A6PML","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_8","alias_value":"AV4W4RBB","created_at":"2026-05-18T12:28:19.803747+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/AV4W4RBBQS4A6PMLGSZFJBKKZE","json":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE.json","graph_json":"https://pith.science/api/pith-number/AV4W4RBBQS4A6PMLGSZFJBKKZE/graph.json","events_json":"https://pith.science/api/pith-number/AV4W4RBBQS4A6PMLGSZFJBKKZE/events.json","paper":"https://pith.science/paper/AV4W4RBB"},"agent_actions":{"view_html":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE","download_json":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE.json","view_paper":"https://pith.science/paper/AV4W4RBB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.1368&json=true","fetch_graph":"https://pith.science/api/pith-number/AV4W4RBBQS4A6PMLGSZFJBKKZE/graph.json","fetch_events":"https://pith.science/api/pith-number/AV4W4RBBQS4A6PMLGSZFJBKKZE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE/action/storage_attestation","attest_author":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE/action/author_attestation","sign_citation":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE/action/citation_signature","submit_replication":"https://pith.science/pith/AV4W4RBBQS4A6PMLGSZFJBKKZE/action/replication_record"}},"created_at":"2026-05-18T02:54:30.230719+00:00","updated_at":"2026-05-18T02:54:30.230719+00:00"}