{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:66MM45BGMF3TGSB4IOKVTVVX5W","short_pith_number":"pith:66MM45BG","schema_version":"1.0","canonical_sha256":"f798ce7426617733483c439559d6b7ed8a87d5497ab051e34268ddea0dd406d2","source":{"kind":"arxiv","id":"1805.09775","version":1},"attestation_state":"computed","paper":{"title":"Assessing the Impact of Astrochemistry on Molecular Cloud Turbulence Statistics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Eric W. Koch, Erik W. Rosolowsky, Ryan D. Boyden, Stella S. R. Offner","submitted_at":"2018-05-24T16:53:42Z","abstract_excerpt":"We analyze hydrodynamic simulations of turbulent, star-forming molecular clouds that are post-processed with the photo-dissociation region astrochemistry code 3D-PDR. We investigate the sensitivity of 15 commonly applied turbulence statistics to post-processing assumptions, namely variations in gas temperature, abundance and external radiation field. We produce synthetic $^{12}$CO(1-0) and CI($^{3}$P$_{1}$-$^{3}$P$_{0}$) observations and examine how the variations influence the resulting emission distributions. To characterize differences between the datasets, we perform statistical measuremen"},"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":"1805.09775","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-05-24T16:53:42Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"5a4e2521a2d3848196b3eda053aaf3a18d9cd666d138d7bd3c0f4bbc53c3b327","abstract_canon_sha256":"71163f1ffae8cb4754f76a5eab599f77e8334855e98fa77b67d26823230c3fa9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:04.746153Z","signature_b64":"GC7tYVyRs+wQVQsbiX6HB+UqhxhQFNrSdOsuylFwaeYqNnhfHg2r2mp8YZQpyLVWn9m3ubjG1c4rHyIIm1ZOCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f798ce7426617733483c439559d6b7ed8a87d5497ab051e34268ddea0dd406d2","last_reissued_at":"2026-05-18T00:11:04.745389Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:04.745389Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Assessing the Impact of Astrochemistry on Molecular Cloud Turbulence Statistics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Eric W. Koch, Erik W. Rosolowsky, Ryan D. Boyden, Stella S. R. Offner","submitted_at":"2018-05-24T16:53:42Z","abstract_excerpt":"We analyze hydrodynamic simulations of turbulent, star-forming molecular clouds that are post-processed with the photo-dissociation region astrochemistry code 3D-PDR. We investigate the sensitivity of 15 commonly applied turbulence statistics to post-processing assumptions, namely variations in gas temperature, abundance and external radiation field. We produce synthetic $^{12}$CO(1-0) and CI($^{3}$P$_{1}$-$^{3}$P$_{0}$) observations and examine how the variations influence the resulting emission distributions. To characterize differences between the datasets, we perform statistical measuremen"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.09775","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":"1805.09775","created_at":"2026-05-18T00:11:04.745496+00:00"},{"alias_kind":"arxiv_version","alias_value":"1805.09775v1","created_at":"2026-05-18T00:11:04.745496+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1805.09775","created_at":"2026-05-18T00:11:04.745496+00:00"},{"alias_kind":"pith_short_12","alias_value":"66MM45BGMF3T","created_at":"2026-05-18T12:32:08.215937+00:00"},{"alias_kind":"pith_short_16","alias_value":"66MM45BGMF3TGSB4","created_at":"2026-05-18T12:32:08.215937+00:00"},{"alias_kind":"pith_short_8","alias_value":"66MM45BG","created_at":"2026-05-18T12:32:08.215937+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/66MM45BGMF3TGSB4IOKVTVVX5W","json":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W.json","graph_json":"https://pith.science/api/pith-number/66MM45BGMF3TGSB4IOKVTVVX5W/graph.json","events_json":"https://pith.science/api/pith-number/66MM45BGMF3TGSB4IOKVTVVX5W/events.json","paper":"https://pith.science/paper/66MM45BG"},"agent_actions":{"view_html":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W","download_json":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W.json","view_paper":"https://pith.science/paper/66MM45BG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1805.09775&json=true","fetch_graph":"https://pith.science/api/pith-number/66MM45BGMF3TGSB4IOKVTVVX5W/graph.json","fetch_events":"https://pith.science/api/pith-number/66MM45BGMF3TGSB4IOKVTVVX5W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W/action/storage_attestation","attest_author":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W/action/author_attestation","sign_citation":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W/action/citation_signature","submit_replication":"https://pith.science/pith/66MM45BGMF3TGSB4IOKVTVVX5W/action/replication_record"}},"created_at":"2026-05-18T00:11:04.745496+00:00","updated_at":"2026-05-18T00:11:04.745496+00:00"}