{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:ODNFPO5RVJDWULNMRSRLWI6IS7","short_pith_number":"pith:ODNFPO5R","schema_version":"1.0","canonical_sha256":"70da57bbb1aa476a2dac8ca2bb23c897fbe7976074dab77cfcd76da53e3673ef","source":{"kind":"arxiv","id":"2201.04158","version":1},"attestation_state":"computed","paper":{"title":"Discovery of 74 new bright ZZ Ceti stars in the first three years of TESS","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. D. Romero, Andy Baran, B. C. Kaiser, Detlev Koester, Gabriela da Rosa Oliveira, Ingrid Pelisoli, J. J. Hermes, Joshua S. Reding, Keaton J. Bell, Larissa Antunes Amaral, Luciano Fraga, Madison VanWyngarden, Maja Vu\\v{c}kovi\\'c, Murat Uzundag, Paul A. Bradley, S. O. Kepler, St\\'ephane Charpinet, T. S. Klippel, Tyler M. Heintz, Zs\\'ofia Bogn\\'ar","submitted_at":"2022-01-11T19:10:53Z","abstract_excerpt":"We report the discovery of 74 new pulsating DA white dwarf stars, or ZZ Cetis, from the data obtained by the Transiting Exoplanet Survey Satellite (TESS) mission, from Sectors 1 to 39, corresponding to the first 3 cycles. This includes objects from the Southern Hemisphere (Sectors 1-13 and 27-39) and the Northern Hemisphere (Sectors 14-26), observed with 120 s- and 20 s-cadence. Our sample likely includes 13 low-mass and one extremely low-mass white dwarf candidate, considering the mass determinations from fitting Gaia magnitudes and parallax. In addition, we present follow-up time series phot"},"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":"2201.04158","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2022-01-11T19:10:53Z","cross_cats_sorted":[],"title_canon_sha256":"2c34cf525f60cc8d91b425df246d14b44260cd18df13c8b4e647d974400a4e62","abstract_canon_sha256":"96d69de47c81ef14a55278b8e4f55179209c24def34be6962109c077a9bb668f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:51:38.990277Z","signature_b64":"NgLYE02DshjThyI/plWH4bTO79s+Z+e2BgyjNBaMTF5P6Nsi01019zuo86bwHAYCLOyaI1hbSRKJnx2ET9OkCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"70da57bbb1aa476a2dac8ca2bb23c897fbe7976074dab77cfcd76da53e3673ef","last_reissued_at":"2026-07-05T03:51:38.989809Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:51:38.989809Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery of 74 new bright ZZ Ceti stars in the first three years of TESS","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. D. Romero, Andy Baran, B. C. Kaiser, Detlev Koester, Gabriela da Rosa Oliveira, Ingrid Pelisoli, J. J. Hermes, Joshua S. Reding, Keaton J. Bell, Larissa Antunes Amaral, Luciano Fraga, Madison VanWyngarden, Maja Vu\\v{c}kovi\\'c, Murat Uzundag, Paul A. Bradley, S. O. Kepler, St\\'ephane Charpinet, T. S. Klippel, Tyler M. Heintz, Zs\\'ofia Bogn\\'ar","submitted_at":"2022-01-11T19:10:53Z","abstract_excerpt":"We report the discovery of 74 new pulsating DA white dwarf stars, or ZZ Cetis, from the data obtained by the Transiting Exoplanet Survey Satellite (TESS) mission, from Sectors 1 to 39, corresponding to the first 3 cycles. This includes objects from the Southern Hemisphere (Sectors 1-13 and 27-39) and the Northern Hemisphere (Sectors 14-26), observed with 120 s- and 20 s-cadence. Our sample likely includes 13 low-mass and one extremely low-mass white dwarf candidate, considering the mass determinations from fitting Gaia magnitudes and parallax. In addition, we present follow-up time series phot"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.04158","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/2201.04158/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":"2201.04158","created_at":"2026-07-05T03:51:38.989865+00:00"},{"alias_kind":"arxiv_version","alias_value":"2201.04158v1","created_at":"2026-07-05T03:51:38.989865+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2201.04158","created_at":"2026-07-05T03:51:38.989865+00:00"},{"alias_kind":"pith_short_12","alias_value":"ODNFPO5RVJDW","created_at":"2026-07-05T03:51:38.989865+00:00"},{"alias_kind":"pith_short_16","alias_value":"ODNFPO5RVJDWULNM","created_at":"2026-07-05T03:51:38.989865+00:00"},{"alias_kind":"pith_short_8","alias_value":"ODNFPO5R","created_at":"2026-07-05T03:51:38.989865+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/ODNFPO5RVJDWULNMRSRLWI6IS7","json":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7.json","graph_json":"https://pith.science/api/pith-number/ODNFPO5RVJDWULNMRSRLWI6IS7/graph.json","events_json":"https://pith.science/api/pith-number/ODNFPO5RVJDWULNMRSRLWI6IS7/events.json","paper":"https://pith.science/paper/ODNFPO5R"},"agent_actions":{"view_html":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7","download_json":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7.json","view_paper":"https://pith.science/paper/ODNFPO5R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2201.04158&json=true","fetch_graph":"https://pith.science/api/pith-number/ODNFPO5RVJDWULNMRSRLWI6IS7/graph.json","fetch_events":"https://pith.science/api/pith-number/ODNFPO5RVJDWULNMRSRLWI6IS7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7/action/storage_attestation","attest_author":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7/action/author_attestation","sign_citation":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7/action/citation_signature","submit_replication":"https://pith.science/pith/ODNFPO5RVJDWULNMRSRLWI6IS7/action/replication_record"}},"created_at":"2026-07-05T03:51:38.989865+00:00","updated_at":"2026-07-05T03:51:38.989865+00:00"}