{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:HCCB5QY272ORDZPKALB27PGHUH","short_pith_number":"pith:HCCB5QY2","schema_version":"1.0","canonical_sha256":"38841ec31afe9d11e5ea02c3afbcc7a1d9646c49e9ba1a5ab6c3c30118848a82","source":{"kind":"arxiv","id":"1908.03593","version":2},"attestation_state":"computed","paper":{"title":"Design Considerations for a Ground-Based Search for Transiting Planets around L and T Dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Patrick Tamburo, Philip S. Muirhead","submitted_at":"2019-08-09T18:47:45Z","abstract_excerpt":"We present design considerations for a ground-based survey for transiting exoplanets around L and T dwarfs, spectral classes that have yet to be thoroughly probed for planets. We simulate photometry for L and T targets with a variety of red-optical and near-infrared detectors, and compare the scatter in the photometry to anticipated transit depths. Based on these results, we recommend the use of a low-dark-current detector with H-band NIR photometric capabilities. We then investigate the potential for performing a survey for Earth-sized planets for a variety of telescope sizes. We simulate pla"},"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":"1908.03593","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2019-08-09T18:47:45Z","cross_cats_sorted":[],"title_canon_sha256":"d0e2dd27f836fd2c66c1b608d421121cf2c80bb68b16678dac2d720d7ccc5179","abstract_canon_sha256":"3bd06b930aadb2bfded2937d0b9f6e4bfd0252a088445a74ce49d89bf44e0b81"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:10:41.471107Z","signature_b64":"foeFYTsyhCOwfRFyPIwLrEvmmz9jrZjiI2VxVid4oy/8Zk3EG7Pfp94hGi3NCsi+Rw2OYXthu2me19uW1NV5CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"38841ec31afe9d11e5ea02c3afbcc7a1d9646c49e9ba1a5ab6c3c30118848a82","last_reissued_at":"2026-07-05T00:10:41.470698Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:10:41.470698Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Design Considerations for a Ground-Based Search for Transiting Planets around L and T Dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Patrick Tamburo, Philip S. Muirhead","submitted_at":"2019-08-09T18:47:45Z","abstract_excerpt":"We present design considerations for a ground-based survey for transiting exoplanets around L and T dwarfs, spectral classes that have yet to be thoroughly probed for planets. We simulate photometry for L and T targets with a variety of red-optical and near-infrared detectors, and compare the scatter in the photometry to anticipated transit depths. Based on these results, we recommend the use of a low-dark-current detector with H-band NIR photometric capabilities. We then investigate the potential for performing a survey for Earth-sized planets for a variety of telescope sizes. We simulate pla"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1908.03593","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/1908.03593/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":"1908.03593","created_at":"2026-07-05T00:10:41.470746+00:00"},{"alias_kind":"arxiv_version","alias_value":"1908.03593v2","created_at":"2026-07-05T00:10:41.470746+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1908.03593","created_at":"2026-07-05T00:10:41.470746+00:00"},{"alias_kind":"pith_short_12","alias_value":"HCCB5QY272OR","created_at":"2026-07-05T00:10:41.470746+00:00"},{"alias_kind":"pith_short_16","alias_value":"HCCB5QY272ORDZPK","created_at":"2026-07-05T00:10:41.470746+00:00"},{"alias_kind":"pith_short_8","alias_value":"HCCB5QY2","created_at":"2026-07-05T00:10:41.470746+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/HCCB5QY272ORDZPKALB27PGHUH","json":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH.json","graph_json":"https://pith.science/api/pith-number/HCCB5QY272ORDZPKALB27PGHUH/graph.json","events_json":"https://pith.science/api/pith-number/HCCB5QY272ORDZPKALB27PGHUH/events.json","paper":"https://pith.science/paper/HCCB5QY2"},"agent_actions":{"view_html":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH","download_json":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH.json","view_paper":"https://pith.science/paper/HCCB5QY2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1908.03593&json=true","fetch_graph":"https://pith.science/api/pith-number/HCCB5QY272ORDZPKALB27PGHUH/graph.json","fetch_events":"https://pith.science/api/pith-number/HCCB5QY272ORDZPKALB27PGHUH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH/action/storage_attestation","attest_author":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH/action/author_attestation","sign_citation":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH/action/citation_signature","submit_replication":"https://pith.science/pith/HCCB5QY272ORDZPKALB27PGHUH/action/replication_record"}},"created_at":"2026-07-05T00:10:41.470746+00:00","updated_at":"2026-07-05T00:10:41.470746+00:00"}