{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:L7NCRSZ6JWPNBCSW6VXL3H7BEN","short_pith_number":"pith:L7NCRSZ6","schema_version":"1.0","canonical_sha256":"5fda28cb3e4d9ed08a56f56ebd9fe1234d0c127f7328b292197fc96a4aa18d8c","source":{"kind":"arxiv","id":"1404.3842","version":1},"attestation_state":"computed","paper":{"title":"AGB stars and the plate archives heritage","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Camilla Pezzotti, Corinne Rossi, Kamo Gigoyan, Nicolas Mauron, Roberto Nesci, Silvia Gaudenzi","submitted_at":"2014-04-15T08:01:15Z","abstract_excerpt":"We report on the characterization of a number of AGB candidate stars identified with objective-prism plates of the Byurakan Observatory. Digitized photographic sky survey plates and recent CCD photometry have been used to improve the selection and distinguish variable and non-variable stars. Some comparisons among published catalog magnitudes are also made. Slit spectroscopy from the Asiago and Loiano Observatories allowed a firm spectral classification, separating C-Type, N-Type and normal M giants. Color-color plots using WISE, AKARI and 2MASS J-band data allow an efficient discrimination of"},"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":"1404.3842","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-04-15T08:01:15Z","cross_cats_sorted":[],"title_canon_sha256":"a321195b3997e2888a4dca2ae16f6f4ea34de2cbe35be14dbeb3adf7e65e4834","abstract_canon_sha256":"36044d5100d42d0202600665a77923aad6a5995978293689cddb4815c33cc399"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:54:13.504399Z","signature_b64":"j5J6clZb5EArrSV+IMVozcbhTKjljvusqIvEzKQBEDmP997ULR9dWQlnv9eqkubrX1LzpidcLNP5GCpLi1lFCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5fda28cb3e4d9ed08a56f56ebd9fe1234d0c127f7328b292197fc96a4aa18d8c","last_reissued_at":"2026-05-18T02:54:13.503902Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:54:13.503902Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"AGB stars and the plate archives heritage","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Camilla Pezzotti, Corinne Rossi, Kamo Gigoyan, Nicolas Mauron, Roberto Nesci, Silvia Gaudenzi","submitted_at":"2014-04-15T08:01:15Z","abstract_excerpt":"We report on the characterization of a number of AGB candidate stars identified with objective-prism plates of the Byurakan Observatory. Digitized photographic sky survey plates and recent CCD photometry have been used to improve the selection and distinguish variable and non-variable stars. Some comparisons among published catalog magnitudes are also made. Slit spectroscopy from the Asiago and Loiano Observatories allowed a firm spectral classification, separating C-Type, N-Type and normal M giants. Color-color plots using WISE, AKARI and 2MASS J-band data allow an efficient discrimination of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.3842","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":"1404.3842","created_at":"2026-05-18T02:54:13.503985+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.3842v1","created_at":"2026-05-18T02:54:13.503985+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.3842","created_at":"2026-05-18T02:54:13.503985+00:00"},{"alias_kind":"pith_short_12","alias_value":"L7NCRSZ6JWPN","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_16","alias_value":"L7NCRSZ6JWPNBCSW","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_8","alias_value":"L7NCRSZ6","created_at":"2026-05-18T12:28:35.611951+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/L7NCRSZ6JWPNBCSW6VXL3H7BEN","json":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN.json","graph_json":"https://pith.science/api/pith-number/L7NCRSZ6JWPNBCSW6VXL3H7BEN/graph.json","events_json":"https://pith.science/api/pith-number/L7NCRSZ6JWPNBCSW6VXL3H7BEN/events.json","paper":"https://pith.science/paper/L7NCRSZ6"},"agent_actions":{"view_html":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN","download_json":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN.json","view_paper":"https://pith.science/paper/L7NCRSZ6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.3842&json=true","fetch_graph":"https://pith.science/api/pith-number/L7NCRSZ6JWPNBCSW6VXL3H7BEN/graph.json","fetch_events":"https://pith.science/api/pith-number/L7NCRSZ6JWPNBCSW6VXL3H7BEN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN/action/storage_attestation","attest_author":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN/action/author_attestation","sign_citation":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN/action/citation_signature","submit_replication":"https://pith.science/pith/L7NCRSZ6JWPNBCSW6VXL3H7BEN/action/replication_record"}},"created_at":"2026-05-18T02:54:13.503985+00:00","updated_at":"2026-05-18T02:54:13.503985+00:00"}