{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:2OLM6PLJLP7YSRDSYET77M6FI5","short_pith_number":"pith:2OLM6PLJ","schema_version":"1.0","canonical_sha256":"d396cf3d695bff894472c127ffb3c547485253e4a48a689b90dee86d6c14458a","source":{"kind":"arxiv","id":"2501.07717","version":1},"attestation_state":"computed","paper":{"title":"3D MC I: X-ray Tomography Begins to Unravel the 3-D Structure of a Molecular Cloud in our Galaxy's Center","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Cara Battersby, Daniel L. Walker, Dani Lipman, Danya Alboslani, H Perry Hatchfield, Ma\\\"ica Clavel, R\\'egis Terrier, Samantha W. Brunker","submitted_at":"2025-01-13T22:07:20Z","abstract_excerpt":"Astronomers have used observations of the Galactic gas and dust via infrared, microwave, and radio to study molecular clouds in extreme environments such as the Galactic center. More recently, X- ray telescopes have opened up a new wavelength range in which to study these molecular clouds. Previous flaring events from SgrA* propagate X-rays outwards in all directions, and these X-rays interact with the surrounding molecular gas, illuminating different parts of the clouds over time. We use a combination of X-ray observations from Chandra and molecular gas tracers (line data from Herschel and th"},"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":"2501.07717","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-01-13T22:07:20Z","cross_cats_sorted":[],"title_canon_sha256":"cd5370484d06e9ede8ffc1f3ca366164174764ac438f6edc1a514161d3647bc3","abstract_canon_sha256":"7aeb6ada46d81a63b2f74741507450d3438108db43c4df3497a735f5c5728557"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:00:49.010941Z","signature_b64":"1yaSlDgPPNlkyvwetYECQ+Bl2mjRblyUOeNo/uAxu7zkC49Qz9f/AK9ccljW1YyxtcswxCRu3h9zjGeXRcTkAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d396cf3d695bff894472c127ffb3c547485253e4a48a689b90dee86d6c14458a","last_reissued_at":"2026-07-05T10:00:49.010489Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:00:49.010489Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"3D MC I: X-ray Tomography Begins to Unravel the 3-D Structure of a Molecular Cloud in our Galaxy's Center","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Cara Battersby, Daniel L. Walker, Dani Lipman, Danya Alboslani, H Perry Hatchfield, Ma\\\"ica Clavel, R\\'egis Terrier, Samantha W. Brunker","submitted_at":"2025-01-13T22:07:20Z","abstract_excerpt":"Astronomers have used observations of the Galactic gas and dust via infrared, microwave, and radio to study molecular clouds in extreme environments such as the Galactic center. More recently, X- ray telescopes have opened up a new wavelength range in which to study these molecular clouds. Previous flaring events from SgrA* propagate X-rays outwards in all directions, and these X-rays interact with the surrounding molecular gas, illuminating different parts of the clouds over time. We use a combination of X-ray observations from Chandra and molecular gas tracers (line data from Herschel and th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.07717","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2501.07717/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":"2501.07717","created_at":"2026-07-05T10:00:49.010549+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.07717v1","created_at":"2026-07-05T10:00:49.010549+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.07717","created_at":"2026-07-05T10:00:49.010549+00:00"},{"alias_kind":"pith_short_12","alias_value":"2OLM6PLJLP7Y","created_at":"2026-07-05T10:00:49.010549+00:00"},{"alias_kind":"pith_short_16","alias_value":"2OLM6PLJLP7YSRDS","created_at":"2026-07-05T10:00:49.010549+00:00"},{"alias_kind":"pith_short_8","alias_value":"2OLM6PLJ","created_at":"2026-07-05T10:00:49.010549+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.07669","citing_title":"3D MC II: X ray echoes reveal a clumpy molecular cloud in the CMZ","ref_index":5,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5","json":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5.json","graph_json":"https://pith.science/api/pith-number/2OLM6PLJLP7YSRDSYET77M6FI5/graph.json","events_json":"https://pith.science/api/pith-number/2OLM6PLJLP7YSRDSYET77M6FI5/events.json","paper":"https://pith.science/paper/2OLM6PLJ"},"agent_actions":{"view_html":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5","download_json":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5.json","view_paper":"https://pith.science/paper/2OLM6PLJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.07717&json=true","fetch_graph":"https://pith.science/api/pith-number/2OLM6PLJLP7YSRDSYET77M6FI5/graph.json","fetch_events":"https://pith.science/api/pith-number/2OLM6PLJLP7YSRDSYET77M6FI5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5/action/storage_attestation","attest_author":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5/action/author_attestation","sign_citation":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5/action/citation_signature","submit_replication":"https://pith.science/pith/2OLM6PLJLP7YSRDSYET77M6FI5/action/replication_record"}},"created_at":"2026-07-05T10:00:49.010549+00:00","updated_at":"2026-07-05T10:00:49.010549+00:00"}