{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:NHT6WJLAGMGT27TADKAC52NJLU","short_pith_number":"pith:NHT6WJLA","schema_version":"1.0","canonical_sha256":"69e7eb2560330d3d7e601a802ee9a95d0477170a9d0ed33c007ade5f7a1b0abd","source":{"kind":"arxiv","id":"2011.06090","version":2},"attestation_state":"computed","paper":{"title":"An approximation to determine the source of the WOW! Signal","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"physics.pop-ph","authors_text":"Alberto Caballero","submitted_at":"2020-11-08T07:31:45Z","abstract_excerpt":"In this paper it is analysed which of the thousands of stars in the WOW! Signal region could have the highest chance of being the real source of the signal, providing that it came from a star system similar to ours. A total of 66 G and K-type stars are sampled, but only one of them is identified as a potential Sun-like star considering the available information in the Gaia Archive. This candidate source, which is named 2MASS 19281982-2640123, therefore becomes an ideal target to conduct observations in the search for potentially habitable exoplanets. Another two candidate stars have a luminosi"},"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":"2011.06090","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.pop-ph","submitted_at":"2020-11-08T07:31:45Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"7e2eb99fcda195992d631377d0c04d2d579098b28bacdb70e8a995670657d71d","abstract_canon_sha256":"e1aba4529a552badd82cd9de48ceb98a69dfdce0021b40061f407244b4ac2964"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:55:31.121064Z","signature_b64":"CvjE2ayIRikIsmHBqf8SjtcpmEvrMvKL7Wv9KEey059VF/+IAT/519YQUnNaec+k3vxlFuAMB/iPsDU6wCcAAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"69e7eb2560330d3d7e601a802ee9a95d0477170a9d0ed33c007ade5f7a1b0abd","last_reissued_at":"2026-07-05T01:55:31.120643Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:55:31.120643Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An approximation to determine the source of the WOW! Signal","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"physics.pop-ph","authors_text":"Alberto Caballero","submitted_at":"2020-11-08T07:31:45Z","abstract_excerpt":"In this paper it is analysed which of the thousands of stars in the WOW! Signal region could have the highest chance of being the real source of the signal, providing that it came from a star system similar to ours. A total of 66 G and K-type stars are sampled, but only one of them is identified as a potential Sun-like star considering the available information in the Gaia Archive. This candidate source, which is named 2MASS 19281982-2640123, therefore becomes an ideal target to conduct observations in the search for potentially habitable exoplanets. Another two candidate stars have a luminosi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2011.06090","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/2011.06090/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":"2011.06090","created_at":"2026-07-05T01:55:31.120696+00:00"},{"alias_kind":"arxiv_version","alias_value":"2011.06090v2","created_at":"2026-07-05T01:55:31.120696+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2011.06090","created_at":"2026-07-05T01:55:31.120696+00:00"},{"alias_kind":"pith_short_12","alias_value":"NHT6WJLAGMGT","created_at":"2026-07-05T01:55:31.120696+00:00"},{"alias_kind":"pith_short_16","alias_value":"NHT6WJLAGMGT27TA","created_at":"2026-07-05T01:55:31.120696+00:00"},{"alias_kind":"pith_short_8","alias_value":"NHT6WJLA","created_at":"2026-07-05T01:55:31.120696+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/NHT6WJLAGMGT27TADKAC52NJLU","json":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU.json","graph_json":"https://pith.science/api/pith-number/NHT6WJLAGMGT27TADKAC52NJLU/graph.json","events_json":"https://pith.science/api/pith-number/NHT6WJLAGMGT27TADKAC52NJLU/events.json","paper":"https://pith.science/paper/NHT6WJLA"},"agent_actions":{"view_html":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU","download_json":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU.json","view_paper":"https://pith.science/paper/NHT6WJLA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2011.06090&json=true","fetch_graph":"https://pith.science/api/pith-number/NHT6WJLAGMGT27TADKAC52NJLU/graph.json","fetch_events":"https://pith.science/api/pith-number/NHT6WJLAGMGT27TADKAC52NJLU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU/action/storage_attestation","attest_author":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU/action/author_attestation","sign_citation":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU/action/citation_signature","submit_replication":"https://pith.science/pith/NHT6WJLAGMGT27TADKAC52NJLU/action/replication_record"}},"created_at":"2026-07-05T01:55:31.120696+00:00","updated_at":"2026-07-05T01:55:31.120696+00:00"}