{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:MAPJFQZVZW3AGOB2SYYGU7YGWC","short_pith_number":"pith:MAPJFQZV","schema_version":"1.0","canonical_sha256":"601e92c335cdb603383a96306a7f06b0a5da702d02693165ba87d38cbe22a078","source":{"kind":"arxiv","id":"1402.2858","version":2},"attestation_state":"computed","paper":{"title":"HI observations of three compact high-velocity clouds around the Milky Way","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"J\\\"urgen Kerp, Lars Fl\\\"oer, Shahram Faridani, Tobias Westmeier","submitted_at":"2014-02-12T15:43:46Z","abstract_excerpt":"We present deep HI observations of three compact high-velocity clouds (CHVCs). The main goal is to study their diffuse warm gas and compact cold cores. We use both low- and high-resolution data obtained with the 100 m Effelsberg telescope and the Westerbork Synthesis Radio Telescope (WSRT). The combination is essential in order to study the morphological properties of the clouds since the single-dish telescope lacks a sufficient angular resolution while the interferometer misses a large portion of the diffuse gas. Here single-dish and interferometer data are combined in the image domain with a"},"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":"1402.2858","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-12T15:43:46Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"63e755c538f7ea9eb193aa7c4f4a39d42d839089375417b6a1e0ceaeed9b73ce","abstract_canon_sha256":"b6cb497d1d0ab2647346b76c96497d6d819f0bbd57cd7b5f57e6cf2133dbd59b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:38.970267Z","signature_b64":"ZP+TZLBfqIZIlc9zUiG7uNdf5briVydsCx2fqqJVexFYNYPW8qDYOzIK+4kvSWO3nheYkr1LAYL1EXyvGptbCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"601e92c335cdb603383a96306a7f06b0a5da702d02693165ba87d38cbe22a078","last_reissued_at":"2026-05-18T01:44:38.969786Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:38.969786Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HI observations of three compact high-velocity clouds around the Milky Way","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"J\\\"urgen Kerp, Lars Fl\\\"oer, Shahram Faridani, Tobias Westmeier","submitted_at":"2014-02-12T15:43:46Z","abstract_excerpt":"We present deep HI observations of three compact high-velocity clouds (CHVCs). The main goal is to study their diffuse warm gas and compact cold cores. We use both low- and high-resolution data obtained with the 100 m Effelsberg telescope and the Westerbork Synthesis Radio Telescope (WSRT). The combination is essential in order to study the morphological properties of the clouds since the single-dish telescope lacks a sufficient angular resolution while the interferometer misses a large portion of the diffuse gas. Here single-dish and interferometer data are combined in the image domain with a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.2858","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":""},"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":"1402.2858","created_at":"2026-05-18T01:44:38.969862+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.2858v2","created_at":"2026-05-18T01:44:38.969862+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.2858","created_at":"2026-05-18T01:44:38.969862+00:00"},{"alias_kind":"pith_short_12","alias_value":"MAPJFQZVZW3A","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_16","alias_value":"MAPJFQZVZW3AGOB2","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_8","alias_value":"MAPJFQZV","created_at":"2026-05-18T12:28:38.356838+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/MAPJFQZVZW3AGOB2SYYGU7YGWC","json":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC.json","graph_json":"https://pith.science/api/pith-number/MAPJFQZVZW3AGOB2SYYGU7YGWC/graph.json","events_json":"https://pith.science/api/pith-number/MAPJFQZVZW3AGOB2SYYGU7YGWC/events.json","paper":"https://pith.science/paper/MAPJFQZV"},"agent_actions":{"view_html":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC","download_json":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC.json","view_paper":"https://pith.science/paper/MAPJFQZV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.2858&json=true","fetch_graph":"https://pith.science/api/pith-number/MAPJFQZVZW3AGOB2SYYGU7YGWC/graph.json","fetch_events":"https://pith.science/api/pith-number/MAPJFQZVZW3AGOB2SYYGU7YGWC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC/action/storage_attestation","attest_author":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC/action/author_attestation","sign_citation":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC/action/citation_signature","submit_replication":"https://pith.science/pith/MAPJFQZVZW3AGOB2SYYGU7YGWC/action/replication_record"}},"created_at":"2026-05-18T01:44:38.969862+00:00","updated_at":"2026-05-18T01:44:38.969862+00:00"}