{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:QIYPMVMWU5TCAUYKRDX5CYY7FC","short_pith_number":"pith:QIYPMVMW","schema_version":"1.0","canonical_sha256":"8230f65596a76620530a88efd1631f288ffa8f150d6608cfd6744d1feb04144f","source":{"kind":"arxiv","id":"1409.5468","version":1},"attestation_state":"computed","paper":{"title":"The Star Formation Relation for Regions in the Galactic Plane: The Effect of Spatial Resolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Cara Battersby, Nalin Vutisalchavakul, Neal J. Evans II","submitted_at":"2014-09-18T21:27:58Z","abstract_excerpt":"We examined the relations between molecular gas surface density and star formation rate surface density in a 11 square degree region of the Galactic Plane. Dust continuum at 1.1 mm from the Bolocam Galactic Plane Survey and 22 micron emission from the WISE All-sky survey were used as tracers of molecular gas and star formation rate, respectively, across Galactic longitude of 31.5 > l > 20.5 and Galactic latitude of 0.5 > b > -0.5. The relation was studied over a range of resolutions from 33 arcsecond to 20 arcminute by convolving images to larger scales. The pixel-by-pixel correlation between "},"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":"1409.5468","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-09-18T21:27:58Z","cross_cats_sorted":[],"title_canon_sha256":"1704c9c77e2c9d410563c3ef3abcc24faaef63b9ed9820fb2f1521c75134ea6d","abstract_canon_sha256":"8a25a518b920169ec6ebba06a7686aa60c8d1732ad405fa726fdbf7c4e1ee656"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:01.265596Z","signature_b64":"/dBCtuNO7N3kb2wO/NyWMSK0s2GKkL4b8Lm6267gsI0iH50+ZQ9Bw7sPS1OVlXEtrmb1gdg3Ehzatd0qRVUIBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8230f65596a76620530a88efd1631f288ffa8f150d6608cfd6744d1feb04144f","last_reissued_at":"2026-05-18T01:42:01.265079Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:01.265079Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Star Formation Relation for Regions in the Galactic Plane: The Effect of Spatial Resolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Cara Battersby, Nalin Vutisalchavakul, Neal J. Evans II","submitted_at":"2014-09-18T21:27:58Z","abstract_excerpt":"We examined the relations between molecular gas surface density and star formation rate surface density in a 11 square degree region of the Galactic Plane. Dust continuum at 1.1 mm from the Bolocam Galactic Plane Survey and 22 micron emission from the WISE All-sky survey were used as tracers of molecular gas and star formation rate, respectively, across Galactic longitude of 31.5 > l > 20.5 and Galactic latitude of 0.5 > b > -0.5. The relation was studied over a range of resolutions from 33 arcsecond to 20 arcminute by convolving images to larger scales. The pixel-by-pixel correlation between "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.5468","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":"1409.5468","created_at":"2026-05-18T01:42:01.265148+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.5468v1","created_at":"2026-05-18T01:42:01.265148+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.5468","created_at":"2026-05-18T01:42:01.265148+00:00"},{"alias_kind":"pith_short_12","alias_value":"QIYPMVMWU5TC","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"QIYPMVMWU5TCAUYK","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"QIYPMVMW","created_at":"2026-05-18T12:28:46.137349+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/QIYPMVMWU5TCAUYKRDX5CYY7FC","json":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC.json","graph_json":"https://pith.science/api/pith-number/QIYPMVMWU5TCAUYKRDX5CYY7FC/graph.json","events_json":"https://pith.science/api/pith-number/QIYPMVMWU5TCAUYKRDX5CYY7FC/events.json","paper":"https://pith.science/paper/QIYPMVMW"},"agent_actions":{"view_html":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC","download_json":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC.json","view_paper":"https://pith.science/paper/QIYPMVMW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.5468&json=true","fetch_graph":"https://pith.science/api/pith-number/QIYPMVMWU5TCAUYKRDX5CYY7FC/graph.json","fetch_events":"https://pith.science/api/pith-number/QIYPMVMWU5TCAUYKRDX5CYY7FC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC/action/storage_attestation","attest_author":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC/action/author_attestation","sign_citation":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC/action/citation_signature","submit_replication":"https://pith.science/pith/QIYPMVMWU5TCAUYKRDX5CYY7FC/action/replication_record"}},"created_at":"2026-05-18T01:42:01.265148+00:00","updated_at":"2026-05-18T01:42:01.265148+00:00"}