{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:NSUAT3QZLMBMBLJTHGDGUGMNJH","short_pith_number":"pith:NSUAT3QZ","schema_version":"1.0","canonical_sha256":"6ca809ee195b02c0ad3339866a198d49f3295b23a57a970070835fc659825e7f","source":{"kind":"arxiv","id":"1909.04714","version":2},"attestation_state":"computed","paper":{"title":"CHIMPS: Physical properties of molecular clumps across the inner Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. J. Rigby, D. J. Eden, G. Park, J. S. Urquhart, M. A. Thompson, M. J. Currie, N. Peretto, R. Plume, S. E. Ragan, T. J. T. Moore","submitted_at":"2019-09-10T19:27:45Z","abstract_excerpt":"The latest generation of high-angular-resolution unbiased Galactic plane surveys in molecular-gas tracers are enabling the interiors of molecular clouds to be studied across a range of environments. The CHIMPS survey simultaneously mapped a sector of the inner Galactic plane, within 27.8 < l < 46.2 deg and |b| < 0.5 deg, in 13CO and C18O (3-2) at 15 arcsec resolution. The combination of CHIMPS data with 12CO (3-2) data from the COHRS survey has enabled us to perform a voxel-by-voxel local-thermodynamic-equilibrium analysis, determining the excitation temperature, optical depth, and column dens"},"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":"1909.04714","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-09-10T19:27:45Z","cross_cats_sorted":[],"title_canon_sha256":"571e4c3d7012fa740442a405027909a74cf40ac4e23493ee10b564082c31ab3b","abstract_canon_sha256":"a792104aa7d7bb647ba1b93670f058e96e9f0c6a8deea0af6d3d68a347e4c7e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:22:19.497828Z","signature_b64":"w5faBjUn5KKX/d6kmkISyOOJJsxvz3y6CeITY2WR+TtaHiIDHesdo2cBl1RwiohQWk0x7TmNBruhXiSJFb5aBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ca809ee195b02c0ad3339866a198d49f3295b23a57a970070835fc659825e7f","last_reissued_at":"2026-07-05T00:22:19.497329Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:22:19.497329Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CHIMPS: Physical properties of molecular clumps across the inner Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. J. Rigby, D. J. Eden, G. Park, J. S. Urquhart, M. A. Thompson, M. J. Currie, N. Peretto, R. Plume, S. E. Ragan, T. J. T. Moore","submitted_at":"2019-09-10T19:27:45Z","abstract_excerpt":"The latest generation of high-angular-resolution unbiased Galactic plane surveys in molecular-gas tracers are enabling the interiors of molecular clouds to be studied across a range of environments. The CHIMPS survey simultaneously mapped a sector of the inner Galactic plane, within 27.8 < l < 46.2 deg and |b| < 0.5 deg, in 13CO and C18O (3-2) at 15 arcsec resolution. The combination of CHIMPS data with 12CO (3-2) data from the COHRS survey has enabled us to perform a voxel-by-voxel local-thermodynamic-equilibrium analysis, determining the excitation temperature, optical depth, and column dens"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.04714","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1909.04714/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"1909.04714","created_at":"2026-07-05T00:22:19.497392+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.04714v2","created_at":"2026-07-05T00:22:19.497392+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.04714","created_at":"2026-07-05T00:22:19.497392+00:00"},{"alias_kind":"pith_short_12","alias_value":"NSUAT3QZLMBM","created_at":"2026-07-05T00:22:19.497392+00:00"},{"alias_kind":"pith_short_16","alias_value":"NSUAT3QZLMBMBLJT","created_at":"2026-07-05T00:22:19.497392+00:00"},{"alias_kind":"pith_short_8","alias_value":"NSUAT3QZ","created_at":"2026-07-05T00:22:19.497392+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/NSUAT3QZLMBMBLJTHGDGUGMNJH","json":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH.json","graph_json":"https://pith.science/api/pith-number/NSUAT3QZLMBMBLJTHGDGUGMNJH/graph.json","events_json":"https://pith.science/api/pith-number/NSUAT3QZLMBMBLJTHGDGUGMNJH/events.json","paper":"https://pith.science/paper/NSUAT3QZ"},"agent_actions":{"view_html":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH","download_json":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH.json","view_paper":"https://pith.science/paper/NSUAT3QZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.04714&json=true","fetch_graph":"https://pith.science/api/pith-number/NSUAT3QZLMBMBLJTHGDGUGMNJH/graph.json","fetch_events":"https://pith.science/api/pith-number/NSUAT3QZLMBMBLJTHGDGUGMNJH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH/action/storage_attestation","attest_author":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH/action/author_attestation","sign_citation":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH/action/citation_signature","submit_replication":"https://pith.science/pith/NSUAT3QZLMBMBLJTHGDGUGMNJH/action/replication_record"}},"created_at":"2026-07-05T00:22:19.497392+00:00","updated_at":"2026-07-05T00:22:19.497392+00:00"}