{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:4Z5CEQ6DSRUTUYFENBLDTLDTWS","short_pith_number":"pith:4Z5CEQ6D","schema_version":"1.0","canonical_sha256":"e67a2243c394693a60a4685639ac73b48158e526ad859525d0332d748f3dcf77","source":{"kind":"arxiv","id":"1310.7952","version":2},"attestation_state":"computed","paper":{"title":"A Spitzer Search for Transits of Radial Velocity Detected Super-Earths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Burrows, A. P. Showman, A. W. Howard, D. Deming, E. Agol, G. P. Laughlin, H. A. Knutson, J. A. Kammer, J. J. Fortney, J.-M. Desert, K. O. Todorov, N. K. Lewis","submitted_at":"2013-10-29T20:17:52Z","abstract_excerpt":"Unlike hot Jupiters or other gas giants, super-Earths are expected to have a wide variety of compositions, ranging from terrestrial bodies like our own to more gaseous planets like Neptune. Observations of transiting systems, which allow us to directly measure planet masses and radii and constrain atmospheric properties, are key to understanding the compositional diversity of the planets in this mass range. Although Kepler has discovered hundreds of transiting super-Earth candidates over the past four years, the majority of these planets orbit stars that are too far away and too faint to allow"},"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":"1310.7952","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-10-29T20:17:52Z","cross_cats_sorted":[],"title_canon_sha256":"a23eab0058690f3849524571de92a355bec688087d238f5c01caff5eeba20368","abstract_canon_sha256":"a17ef30b88ff673f4e26a3d4b5a8c2155ac301422d734b33f6bf3c87f482710a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:47.626126Z","signature_b64":"Tzdj60AzQotuhbGXXD7wQhROZ36XHWY4zKPul+PH6hYRvw9VmlZp8xXAt7EmzTezDDXaP1cchRycSWMYlZtjBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e67a2243c394693a60a4685639ac73b48158e526ad859525d0332d748f3dcf77","last_reissued_at":"2026-05-18T01:46:47.625440Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:47.625440Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Spitzer Search for Transits of Radial Velocity Detected Super-Earths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Burrows, A. P. Showman, A. W. Howard, D. Deming, E. Agol, G. P. Laughlin, H. A. Knutson, J. A. Kammer, J. J. Fortney, J.-M. Desert, K. O. Todorov, N. K. Lewis","submitted_at":"2013-10-29T20:17:52Z","abstract_excerpt":"Unlike hot Jupiters or other gas giants, super-Earths are expected to have a wide variety of compositions, ranging from terrestrial bodies like our own to more gaseous planets like Neptune. Observations of transiting systems, which allow us to directly measure planet masses and radii and constrain atmospheric properties, are key to understanding the compositional diversity of the planets in this mass range. Although Kepler has discovered hundreds of transiting super-Earth candidates over the past four years, the majority of these planets orbit stars that are too far away and too faint to allow"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.7952","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":""},"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":"1310.7952","created_at":"2026-05-18T01:46:47.625549+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.7952v2","created_at":"2026-05-18T01:46:47.625549+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.7952","created_at":"2026-05-18T01:46:47.625549+00:00"},{"alias_kind":"pith_short_12","alias_value":"4Z5CEQ6DSRUT","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"4Z5CEQ6DSRUTUYFE","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"4Z5CEQ6D","created_at":"2026-05-18T12:27:34.582898+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/4Z5CEQ6DSRUTUYFENBLDTLDTWS","json":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS.json","graph_json":"https://pith.science/api/pith-number/4Z5CEQ6DSRUTUYFENBLDTLDTWS/graph.json","events_json":"https://pith.science/api/pith-number/4Z5CEQ6DSRUTUYFENBLDTLDTWS/events.json","paper":"https://pith.science/paper/4Z5CEQ6D"},"agent_actions":{"view_html":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS","download_json":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS.json","view_paper":"https://pith.science/paper/4Z5CEQ6D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.7952&json=true","fetch_graph":"https://pith.science/api/pith-number/4Z5CEQ6DSRUTUYFENBLDTLDTWS/graph.json","fetch_events":"https://pith.science/api/pith-number/4Z5CEQ6DSRUTUYFENBLDTLDTWS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS/action/storage_attestation","attest_author":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS/action/author_attestation","sign_citation":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS/action/citation_signature","submit_replication":"https://pith.science/pith/4Z5CEQ6DSRUTUYFENBLDTLDTWS/action/replication_record"}},"created_at":"2026-05-18T01:46:47.625549+00:00","updated_at":"2026-05-18T01:46:47.625549+00:00"}