{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:UMU7ILF3JSDYUC6TWD5AMLKPVD","short_pith_number":"pith:UMU7ILF3","schema_version":"1.0","canonical_sha256":"a329f42cbb4c878a0bd3b0fa062d4fa8c6008b82528c7d5b26d92e740856b44e","source":{"kind":"arxiv","id":"1301.5240","version":1},"attestation_state":"computed","paper":{"title":"On the potential of the Cherenkov Telescope Array for the study of cosmic-ray diffusion in molecular clouds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. F. Torres, D. Mazin, E. de O\\~na Wilhelmi, G. Pedaletti, S. Gabici, V. Stamatescu","submitted_at":"2013-01-22T17:00:11Z","abstract_excerpt":"Molecular clouds act as primary targets for cosmic-ray interactions and are expected to shine in gamma-rays as a by-product of these interactions. Indeed several detected gamma-ray sources both in HE and VHE gamma-rays (HE: 100 MeV < E < 100 GeV; VHE: E > 100 GeV) have been directly or indirectly associated with molecular clouds. Information on the local diffusion coefficient and the cosmic-ray population can be inferred from the observed gamma-ray signals. In this work we explore the capability of the forthcoming Cherenkov Telescope Array Observatory (CTA) to provide such measurements. We inv"},"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":"1301.5240","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-22T17:00:11Z","cross_cats_sorted":[],"title_canon_sha256":"074133ed8a84ca0990521173513c5db3e7fd03a26cc43945d9ca9a278062f8f8","abstract_canon_sha256":"f3e62d54108938bc8b91093231e4c6fb21f2c3446c62fefaa056702855f370b6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:52:04.631842Z","signature_b64":"5Mq4yARxUeFJ+qVpfzGC1N89p6+ZhQubby8k0MtPbdEsbw2q8oedzrVAe6IQ+t9nIRe32dXzHIZ/H7LNT4EWBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a329f42cbb4c878a0bd3b0fa062d4fa8c6008b82528c7d5b26d92e740856b44e","last_reissued_at":"2026-05-18T01:52:04.631440Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:52:04.631440Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the potential of the Cherenkov Telescope Array for the study of cosmic-ray diffusion in molecular clouds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. F. Torres, D. Mazin, E. de O\\~na Wilhelmi, G. Pedaletti, S. Gabici, V. Stamatescu","submitted_at":"2013-01-22T17:00:11Z","abstract_excerpt":"Molecular clouds act as primary targets for cosmic-ray interactions and are expected to shine in gamma-rays as a by-product of these interactions. Indeed several detected gamma-ray sources both in HE and VHE gamma-rays (HE: 100 MeV < E < 100 GeV; VHE: E > 100 GeV) have been directly or indirectly associated with molecular clouds. Information on the local diffusion coefficient and the cosmic-ray population can be inferred from the observed gamma-ray signals. In this work we explore the capability of the forthcoming Cherenkov Telescope Array Observatory (CTA) to provide such measurements. We inv"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.5240","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":"1301.5240","created_at":"2026-05-18T01:52:04.631499+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.5240v1","created_at":"2026-05-18T01:52:04.631499+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.5240","created_at":"2026-05-18T01:52:04.631499+00:00"},{"alias_kind":"pith_short_12","alias_value":"UMU7ILF3JSDY","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_16","alias_value":"UMU7ILF3JSDYUC6T","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_8","alias_value":"UMU7ILF3","created_at":"2026-05-18T12:28:02.375192+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21672","citing_title":"Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas","ref_index":46,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD","json":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD.json","graph_json":"https://pith.science/api/pith-number/UMU7ILF3JSDYUC6TWD5AMLKPVD/graph.json","events_json":"https://pith.science/api/pith-number/UMU7ILF3JSDYUC6TWD5AMLKPVD/events.json","paper":"https://pith.science/paper/UMU7ILF3"},"agent_actions":{"view_html":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD","download_json":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD.json","view_paper":"https://pith.science/paper/UMU7ILF3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.5240&json=true","fetch_graph":"https://pith.science/api/pith-number/UMU7ILF3JSDYUC6TWD5AMLKPVD/graph.json","fetch_events":"https://pith.science/api/pith-number/UMU7ILF3JSDYUC6TWD5AMLKPVD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD/action/storage_attestation","attest_author":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD/action/author_attestation","sign_citation":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD/action/citation_signature","submit_replication":"https://pith.science/pith/UMU7ILF3JSDYUC6TWD5AMLKPVD/action/replication_record"}},"created_at":"2026-05-18T01:52:04.631499+00:00","updated_at":"2026-05-18T01:52:04.631499+00:00"}