{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:M3JMPAA7JRO2UVTYZRAM5BSGBJ","short_pith_number":"pith:M3JMPAA7","schema_version":"1.0","canonical_sha256":"66d2c7801f4c5daa5678cc40ce86460a4922dd25ebed5aefffa36e54569af406","source":{"kind":"arxiv","id":"1303.5487","version":1},"attestation_state":"computed","paper":{"title":"Physical properties of B-type asteroids from WISE data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Humberto Campins, Javier Licandro, Julia de Le\\'on, Marco Delb\\'o, Michael S. Kelley, Noem\\'i Pinilla-Alonso, V\\'ictor Al\\'i-Lagoa","submitted_at":"2013-03-22T00:17:55Z","abstract_excerpt":"Aims: Our aim is to obtain more information about the physical nature of B-type asteroids and extend on the previous work by studying their physical properties derived from fitting an asteroid thermal model to their NASA's Wide-field Infrared Survey Explorer (WISE) data. We also examine the Pallas collisional family, a B-type family with a moderately high albedo in contrast to the large majority of B-types. Methods: We apply a combination of the NEATM and a model of the reflected sunlight to WISE asteroid data in order to derive effective diameter (D), the so-called infrared beaming parameter "},"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":"1303.5487","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-03-22T00:17:55Z","cross_cats_sorted":[],"title_canon_sha256":"f6a54a7c805dffc003c8d6782704ff49400e02405c799cc8f6e17c05803b6096","abstract_canon_sha256":"4ef6111c7a6349d43c5af9fa3b86d01e7e61308ff409c65ffb70a737ba7fcb0d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:59.717002Z","signature_b64":"I8FjpjwG8rD4EWu+lfVwMf7Q0fdp23eq2kyFxEoYBe1v9qiCJ+dqK6GV9TFwkeepxjNCyy0ATqFJXdI/DTTyDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"66d2c7801f4c5daa5678cc40ce86460a4922dd25ebed5aefffa36e54569af406","last_reissued_at":"2026-05-18T01:50:59.716563Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:59.716563Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Physical properties of B-type asteroids from WISE data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Humberto Campins, Javier Licandro, Julia de Le\\'on, Marco Delb\\'o, Michael S. Kelley, Noem\\'i Pinilla-Alonso, V\\'ictor Al\\'i-Lagoa","submitted_at":"2013-03-22T00:17:55Z","abstract_excerpt":"Aims: Our aim is to obtain more information about the physical nature of B-type asteroids and extend on the previous work by studying their physical properties derived from fitting an asteroid thermal model to their NASA's Wide-field Infrared Survey Explorer (WISE) data. We also examine the Pallas collisional family, a B-type family with a moderately high albedo in contrast to the large majority of B-types. Methods: We apply a combination of the NEATM and a model of the reflected sunlight to WISE asteroid data in order to derive effective diameter (D), the so-called infrared beaming parameter "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.5487","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":""},"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":"1303.5487","created_at":"2026-05-18T01:50:59.716622+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.5487v1","created_at":"2026-05-18T01:50:59.716622+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.5487","created_at":"2026-05-18T01:50:59.716622+00:00"},{"alias_kind":"pith_short_12","alias_value":"M3JMPAA7JRO2","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"M3JMPAA7JRO2UVTY","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"M3JMPAA7","created_at":"2026-05-18T12:27:51.066281+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/M3JMPAA7JRO2UVTYZRAM5BSGBJ","json":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ.json","graph_json":"https://pith.science/api/pith-number/M3JMPAA7JRO2UVTYZRAM5BSGBJ/graph.json","events_json":"https://pith.science/api/pith-number/M3JMPAA7JRO2UVTYZRAM5BSGBJ/events.json","paper":"https://pith.science/paper/M3JMPAA7"},"agent_actions":{"view_html":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ","download_json":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ.json","view_paper":"https://pith.science/paper/M3JMPAA7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.5487&json=true","fetch_graph":"https://pith.science/api/pith-number/M3JMPAA7JRO2UVTYZRAM5BSGBJ/graph.json","fetch_events":"https://pith.science/api/pith-number/M3JMPAA7JRO2UVTYZRAM5BSGBJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ/action/storage_attestation","attest_author":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ/action/author_attestation","sign_citation":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ/action/citation_signature","submit_replication":"https://pith.science/pith/M3JMPAA7JRO2UVTYZRAM5BSGBJ/action/replication_record"}},"created_at":"2026-05-18T01:50:59.716622+00:00","updated_at":"2026-05-18T01:50:59.716622+00:00"}