{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:RS3YNQAEKQ3TAPXAR34PSJFPCR","short_pith_number":"pith:RS3YNQAE","schema_version":"1.0","canonical_sha256":"8cb786c0045437303ee08ef8f924af1478be754f8b9792722ab5851b30eb08a9","source":{"kind":"arxiv","id":"1412.2911","version":1},"attestation_state":"computed","paper":{"title":"The Interstellar Medium and star formation on kpc size scales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Clare L. Dobbs","submitted_at":"2014-12-09T11:01:19Z","abstract_excerpt":"By resimulating a region of a global disc simulation at higher resolution, we resolve and study the properties of molecular clouds with a range of masses from a few 100's M$_{\\odot}$ to $10^6$ M$_{\\odot}$. The purpose of our paper is twofold, i) to compare the ISM and GMCs at much higher resolution compared to previous global simulations, and ii) to investigate smaller clouds and characteristics such as the internal properties of GMCs which cannot be resolved in galactic simulations. We confirm the robustness of cloud properties seen in previous galactic simulations, and that these properties "},"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":"1412.2911","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-12-09T11:01:19Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"466d3bfd6d69cd2e6fd0019b54292831a450e3c990f436a2784ca9633455f6af","abstract_canon_sha256":"a52372fa0b048663b13dd579746d8b4c3347495e98d918c97ac4021274b9061a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:20.522132Z","signature_b64":"+SOt+dYD3H05wQESl3GG+Rv+5WUFOVTkGMtQb8wBcu/2GnFmvAevTg4mUjxgXR5gPv1GKOBGOy3Kft0teddECw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8cb786c0045437303ee08ef8f924af1478be754f8b9792722ab5851b30eb08a9","last_reissued_at":"2026-05-18T01:41:20.521489Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:20.521489Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Interstellar Medium and star formation on kpc size scales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Clare L. Dobbs","submitted_at":"2014-12-09T11:01:19Z","abstract_excerpt":"By resimulating a region of a global disc simulation at higher resolution, we resolve and study the properties of molecular clouds with a range of masses from a few 100's M$_{\\odot}$ to $10^6$ M$_{\\odot}$. The purpose of our paper is twofold, i) to compare the ISM and GMCs at much higher resolution compared to previous global simulations, and ii) to investigate smaller clouds and characteristics such as the internal properties of GMCs which cannot be resolved in galactic simulations. We confirm the robustness of cloud properties seen in previous galactic simulations, and that these properties "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.2911","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":"1412.2911","created_at":"2026-05-18T01:41:20.521584+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.2911v1","created_at":"2026-05-18T01:41:20.521584+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.2911","created_at":"2026-05-18T01:41:20.521584+00:00"},{"alias_kind":"pith_short_12","alias_value":"RS3YNQAEKQ3T","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"RS3YNQAEKQ3TAPXA","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"RS3YNQAE","created_at":"2026-05-18T12:28:46.137349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.17024","citing_title":"The ${}^{13}\\mathrm{CO}(2{-}1)/^{12}\\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud","ref_index":199,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR","json":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR.json","graph_json":"https://pith.science/api/pith-number/RS3YNQAEKQ3TAPXAR34PSJFPCR/graph.json","events_json":"https://pith.science/api/pith-number/RS3YNQAEKQ3TAPXAR34PSJFPCR/events.json","paper":"https://pith.science/paper/RS3YNQAE"},"agent_actions":{"view_html":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR","download_json":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR.json","view_paper":"https://pith.science/paper/RS3YNQAE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.2911&json=true","fetch_graph":"https://pith.science/api/pith-number/RS3YNQAEKQ3TAPXAR34PSJFPCR/graph.json","fetch_events":"https://pith.science/api/pith-number/RS3YNQAEKQ3TAPXAR34PSJFPCR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR/action/storage_attestation","attest_author":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR/action/author_attestation","sign_citation":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR/action/citation_signature","submit_replication":"https://pith.science/pith/RS3YNQAEKQ3TAPXAR34PSJFPCR/action/replication_record"}},"created_at":"2026-05-18T01:41:20.521584+00:00","updated_at":"2026-05-18T01:41:20.521584+00:00"}