{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:XGSRFGJD6E2LYMPVSAQQH2ESDO","short_pith_number":"pith:XGSRFGJD","schema_version":"1.0","canonical_sha256":"b9a5129923f134bc31f5902103e8921b835c5b0c69eb3b1abd719382f5787089","source":{"kind":"arxiv","id":"2403.14214","version":2},"attestation_state":"computed","paper":{"title":"Asteroseismological analysis of the non-Blazhko RRab star EPIC~248846335 in LAMOST -- Kepler$/$ K2 project","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Antonio Frasca, Bo Zhang, Gang Meng, Gao-Chao Liu, Gianni Catanzaro, Haotian Wang, Jian-Ning Fu, Jiaxin Wang, Jie Su, Peng Zong, Weikai Zong, Xueying Hu","submitted_at":"2024-03-21T08:11:10Z","abstract_excerpt":"We conduct an asteroseismological analysis on the non-Blazhko ab-type RR Lyrae star EPIC 248846335 employing the Radial Stellar Pulsations (RSP) module of the Modules for Experiments in Stellar Astrophysics (MESA) based on the set of stellar parameters. The atmospheric parameters as $T_\\mathrm{eff}$ = 6933$\\pm$70 $K$, log $g$ = 3.35$\\pm$ 0.50 and [Fe/H] = -1.18 $\\pm$ 0.14 are estimated from the Low-Resolution Spectra of LAMOST DR9. The luminosity $L$ = 49.70$_{-1.80}^{+2.99}$ $L_\\odot$ and mass M = 0.56 $\\pm$ 0.07 $M_\\odot$ are calculated, respectively, using the distance provided by Gaia and "},"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":"2403.14214","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-03-21T08:11:10Z","cross_cats_sorted":[],"title_canon_sha256":"7323c66005b426569e54f1b03a0843b71eef99a0f9e21e19333f6f685bb8b801","abstract_canon_sha256":"74cafc10bd5aab468fd223cdc83fd8b7541e0f08d283957eac815bca2198ed50"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:00:04.240876Z","signature_b64":"ce9xvMHRv/9qO6rweuNVAbYto/mioL5Ea8h2d8cLdS6lXKE/myVuOQu1BTADM/zgPRZNUdVkl/H/4bSmu62MBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b9a5129923f134bc31f5902103e8921b835c5b0c69eb3b1abd719382f5787089","last_reissued_at":"2026-07-05T08:00:04.240460Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:00:04.240460Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Asteroseismological analysis of the non-Blazhko RRab star EPIC~248846335 in LAMOST -- Kepler$/$ K2 project","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Antonio Frasca, Bo Zhang, Gang Meng, Gao-Chao Liu, Gianni Catanzaro, Haotian Wang, Jian-Ning Fu, Jiaxin Wang, Jie Su, Peng Zong, Weikai Zong, Xueying Hu","submitted_at":"2024-03-21T08:11:10Z","abstract_excerpt":"We conduct an asteroseismological analysis on the non-Blazhko ab-type RR Lyrae star EPIC 248846335 employing the Radial Stellar Pulsations (RSP) module of the Modules for Experiments in Stellar Astrophysics (MESA) based on the set of stellar parameters. The atmospheric parameters as $T_\\mathrm{eff}$ = 6933$\\pm$70 $K$, log $g$ = 3.35$\\pm$ 0.50 and [Fe/H] = -1.18 $\\pm$ 0.14 are estimated from the Low-Resolution Spectra of LAMOST DR9. The luminosity $L$ = 49.70$_{-1.80}^{+2.99}$ $L_\\odot$ and mass M = 0.56 $\\pm$ 0.07 $M_\\odot$ are calculated, respectively, using the distance provided by Gaia and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.14214","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.14214/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":"2403.14214","created_at":"2026-07-05T08:00:04.240520+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.14214v2","created_at":"2026-07-05T08:00:04.240520+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.14214","created_at":"2026-07-05T08:00:04.240520+00:00"},{"alias_kind":"pith_short_12","alias_value":"XGSRFGJD6E2L","created_at":"2026-07-05T08:00:04.240520+00:00"},{"alias_kind":"pith_short_16","alias_value":"XGSRFGJD6E2LYMPV","created_at":"2026-07-05T08:00:04.240520+00:00"},{"alias_kind":"pith_short_8","alias_value":"XGSRFGJD","created_at":"2026-07-05T08:00:04.240520+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/XGSRFGJD6E2LYMPVSAQQH2ESDO","json":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO.json","graph_json":"https://pith.science/api/pith-number/XGSRFGJD6E2LYMPVSAQQH2ESDO/graph.json","events_json":"https://pith.science/api/pith-number/XGSRFGJD6E2LYMPVSAQQH2ESDO/events.json","paper":"https://pith.science/paper/XGSRFGJD"},"agent_actions":{"view_html":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO","download_json":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO.json","view_paper":"https://pith.science/paper/XGSRFGJD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.14214&json=true","fetch_graph":"https://pith.science/api/pith-number/XGSRFGJD6E2LYMPVSAQQH2ESDO/graph.json","fetch_events":"https://pith.science/api/pith-number/XGSRFGJD6E2LYMPVSAQQH2ESDO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO/action/storage_attestation","attest_author":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO/action/author_attestation","sign_citation":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO/action/citation_signature","submit_replication":"https://pith.science/pith/XGSRFGJD6E2LYMPVSAQQH2ESDO/action/replication_record"}},"created_at":"2026-07-05T08:00:04.240520+00:00","updated_at":"2026-07-05T08:00:04.240520+00:00"}