{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:GDQY3UFOE7NBD3C7FD53B55R4Y","short_pith_number":"pith:GDQY3UFO","schema_version":"1.0","canonical_sha256":"30e18dd0ae27da11ec5f28fbb0f7b1e61000e18f8bd4e4255a84bb1603dbb5d4","source":{"kind":"arxiv","id":"2012.12269","version":1},"attestation_state":"computed","paper":{"title":"A Study of Open Clusters Frolov 1 and NGC 7510 using CCD UBV Photometry and Gaia DR2 Astrometry","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. Akbulut, E. Paunzen, R. Canbay, S. Ak, S. Bilir, T. Ak, T. Banks, T. Yontan, Z. F. Bostanci","submitted_at":"2020-12-22T19:00:01Z","abstract_excerpt":"We present reddening, photometric metallicity, age and distance estimates for the Frolov 1 and NGC 7510 open clusters based on CCD UBV photometric and Gaia data. Photometric observations were collected using the 1-m telescope of the T\\\"UB\\.ITAK National Observatory. Gaia DR2 proper motion data in the direction of two groupings were used to identify cluster membership. We determined mean proper motion values ($ \\mu_{\\alpha}\\cos\\delta, \\mu_{\\delta}$) = ($-3.02\\pm 0.10$, $-1.75 \\pm 0.08$) and ($-3.66 \\pm 0.07$, $-2.17 \\pm 0.06$) mas yr$^{-1}$ for Frolov 1 and NGC 7510, respectively. We used two-c"},"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":"2012.12269","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-12-22T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"1b06487a6c55c2849cd471ad7f1a9ad340b0f08be2e5d172dcaa63b981ab9279","abstract_canon_sha256":"525528cbaa29e93b7aafb27eaffbd026239cf6fb502134c1d1d10fd9f5a328aa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:35:31.047769Z","signature_b64":"Q5lX2NG5VQYwzcFGgsvEqLqfobyDKeqJxV0UG37vL4d4J13ayKbM6nEKqrA4lhdsHdnK8Zk+9V3IJdqPILX5DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"30e18dd0ae27da11ec5f28fbb0f7b1e61000e18f8bd4e4255a84bb1603dbb5d4","last_reissued_at":"2026-07-05T02:35:31.047218Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:35:31.047218Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Study of Open Clusters Frolov 1 and NGC 7510 using CCD UBV Photometry and Gaia DR2 Astrometry","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. Akbulut, E. Paunzen, R. Canbay, S. Ak, S. Bilir, T. Ak, T. Banks, T. Yontan, Z. F. Bostanci","submitted_at":"2020-12-22T19:00:01Z","abstract_excerpt":"We present reddening, photometric metallicity, age and distance estimates for the Frolov 1 and NGC 7510 open clusters based on CCD UBV photometric and Gaia data. Photometric observations were collected using the 1-m telescope of the T\\\"UB\\.ITAK National Observatory. Gaia DR2 proper motion data in the direction of two groupings were used to identify cluster membership. We determined mean proper motion values ($ \\mu_{\\alpha}\\cos\\delta, \\mu_{\\delta}$) = ($-3.02\\pm 0.10$, $-1.75 \\pm 0.08$) and ($-3.66 \\pm 0.07$, $-2.17 \\pm 0.06$) mas yr$^{-1}$ for Frolov 1 and NGC 7510, respectively. We used two-c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.12269","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/2012.12269/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":"2012.12269","created_at":"2026-07-05T02:35:31.047277+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.12269v1","created_at":"2026-07-05T02:35:31.047277+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.12269","created_at":"2026-07-05T02:35:31.047277+00:00"},{"alias_kind":"pith_short_12","alias_value":"GDQY3UFOE7NB","created_at":"2026-07-05T02:35:31.047277+00:00"},{"alias_kind":"pith_short_16","alias_value":"GDQY3UFOE7NBD3C7","created_at":"2026-07-05T02:35:31.047277+00:00"},{"alias_kind":"pith_short_8","alias_value":"GDQY3UFO","created_at":"2026-07-05T02:35:31.047277+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/GDQY3UFOE7NBD3C7FD53B55R4Y","json":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y.json","graph_json":"https://pith.science/api/pith-number/GDQY3UFOE7NBD3C7FD53B55R4Y/graph.json","events_json":"https://pith.science/api/pith-number/GDQY3UFOE7NBD3C7FD53B55R4Y/events.json","paper":"https://pith.science/paper/GDQY3UFO"},"agent_actions":{"view_html":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y","download_json":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y.json","view_paper":"https://pith.science/paper/GDQY3UFO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.12269&json=true","fetch_graph":"https://pith.science/api/pith-number/GDQY3UFOE7NBD3C7FD53B55R4Y/graph.json","fetch_events":"https://pith.science/api/pith-number/GDQY3UFOE7NBD3C7FD53B55R4Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y/action/storage_attestation","attest_author":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y/action/author_attestation","sign_citation":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y/action/citation_signature","submit_replication":"https://pith.science/pith/GDQY3UFOE7NBD3C7FD53B55R4Y/action/replication_record"}},"created_at":"2026-07-05T02:35:31.047277+00:00","updated_at":"2026-07-05T02:35:31.047277+00:00"}