{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:66QHB67MENEKT7TVLPQOOA2YQX","short_pith_number":"pith:66QHB67M","canonical_record":{"source":{"id":"1705.10263","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-05-29T15:45:16Z","cross_cats_sorted":[],"title_canon_sha256":"42641ee578a0ae0ea104f39e85752323969efb20719d62205717cc2a1914f1a1","abstract_canon_sha256":"d151a6bb86a8297178cf1c78bb3fd3cf395ce26dd4562500ba24fa86d5eb3831"},"schema_version":"1.0"},"canonical_sha256":"f7a070fbec2348a9fe755be0e7035885d141f9ad617ab9689164f70c71e19887","source":{"kind":"arxiv","id":"1705.10263","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.10263","created_at":"2026-05-18T00:40:29Z"},{"alias_kind":"arxiv_version","alias_value":"1705.10263v1","created_at":"2026-05-18T00:40:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.10263","created_at":"2026-05-18T00:40:29Z"},{"alias_kind":"pith_short_12","alias_value":"66QHB67MENEK","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_16","alias_value":"66QHB67MENEKT7TV","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_8","alias_value":"66QHB67M","created_at":"2026-05-18T12:31:03Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:66QHB67MENEKT7TVLPQOOA2YQX","target":"record","payload":{"canonical_record":{"source":{"id":"1705.10263","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-05-29T15:45:16Z","cross_cats_sorted":[],"title_canon_sha256":"42641ee578a0ae0ea104f39e85752323969efb20719d62205717cc2a1914f1a1","abstract_canon_sha256":"d151a6bb86a8297178cf1c78bb3fd3cf395ce26dd4562500ba24fa86d5eb3831"},"schema_version":"1.0"},"canonical_sha256":"f7a070fbec2348a9fe755be0e7035885d141f9ad617ab9689164f70c71e19887","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:29.887403Z","signature_b64":"pjRakim3SC7CdgVAByiIwedlAjhNLeU7JPpodlimWdCWsl5Zyd+DyvzSCUtMt5Ukpcyxv6DlvqSG1Ye4lqNgAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f7a070fbec2348a9fe755be0e7035885d141f9ad617ab9689164f70c71e19887","last_reissued_at":"2026-05-18T00:40:29.886980Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:29.886980Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1705.10263","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:40:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"wX6aWzGNfrceJHJLt/CKVZYSne8y4tmh4QZx95HnjouzICH80Vntjs8F8WsFLcdkGMhtDvoSumk7BoPPl2x1DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-10T18:44:31.848715Z"},"content_sha256":"4dea04ae264800631b28ef3d2a9e4cacca8954e75c6e53a955f42ff31cafbfab","schema_version":"1.0","event_id":"sha256:4dea04ae264800631b28ef3d2a9e4cacca8954e75c6e53a955f42ff31cafbfab"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:66QHB67MENEKT7TVLPQOOA2YQX","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Marco Delbo', V\\'ictor Al\\'i-Lagoa","submitted_at":"2017-05-29T15:45:16Z","abstract_excerpt":"Context. Mars-crossing asteroids (MCs) are a dynamically unstable group between the main belt and the near-Earth populations. Characterising the physical properties of a large sample of MCs can help to understand the original sources of many near-Earth asteroids, some of which may produce meteorites on Earth. Aims. Our aim is to provide diameters and albedos of MCs with available WISE/NEOWISE data. Methods. We used the near-Earth asteroid thermal model to find the best-fitting values of equivalent diameter and, whenever possible, the infrared beaming parameter. With the diameter and tabulated "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.10263","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:40:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"sU5LxoS8rQCMiIHW8UaJkcUnJnayDH2X7puBc69UaQOIvQeGJosVN135bNLEfogLi9eOI10spSWZp/k3nQowCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-10T18:44:31.849161Z"},"content_sha256":"f259ddecf6166dd909c5d46030e16e2df0cd631b910bc1a6dd68f434f5bc83dd","schema_version":"1.0","event_id":"sha256:f259ddecf6166dd909c5d46030e16e2df0cd631b910bc1a6dd68f434f5bc83dd"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/66QHB67MENEKT7TVLPQOOA2YQX/bundle.json","state_url":"https://pith.science/pith/66QHB67MENEKT7TVLPQOOA2YQX/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/66QHB67MENEKT7TVLPQOOA2YQX/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-10T18:44:31Z","links":{"resolver":"https://pith.science/pith/66QHB67MENEKT7TVLPQOOA2YQX","bundle":"https://pith.science/pith/66QHB67MENEKT7TVLPQOOA2YQX/bundle.json","state":"https://pith.science/pith/66QHB67MENEKT7TVLPQOOA2YQX/state.json","well_known_bundle":"https://pith.science/.well-known/pith/66QHB67MENEKT7TVLPQOOA2YQX/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:66QHB67MENEKT7TVLPQOOA2YQX","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"d151a6bb86a8297178cf1c78bb3fd3cf395ce26dd4562500ba24fa86d5eb3831","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-05-29T15:45:16Z","title_canon_sha256":"42641ee578a0ae0ea104f39e85752323969efb20719d62205717cc2a1914f1a1"},"schema_version":"1.0","source":{"id":"1705.10263","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.10263","created_at":"2026-05-18T00:40:29Z"},{"alias_kind":"arxiv_version","alias_value":"1705.10263v1","created_at":"2026-05-18T00:40:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.10263","created_at":"2026-05-18T00:40:29Z"},{"alias_kind":"pith_short_12","alias_value":"66QHB67MENEK","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_16","alias_value":"66QHB67MENEKT7TV","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_8","alias_value":"66QHB67M","created_at":"2026-05-18T12:31:03Z"}],"graph_snapshots":[{"event_id":"sha256:f259ddecf6166dd909c5d46030e16e2df0cd631b910bc1a6dd68f434f5bc83dd","target":"graph","created_at":"2026-05-18T00:40:29Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Context. Mars-crossing asteroids (MCs) are a dynamically unstable group between the main belt and the near-Earth populations. Characterising the physical properties of a large sample of MCs can help to understand the original sources of many near-Earth asteroids, some of which may produce meteorites on Earth. Aims. Our aim is to provide diameters and albedos of MCs with available WISE/NEOWISE data. Methods. We used the near-Earth asteroid thermal model to find the best-fitting values of equivalent diameter and, whenever possible, the infrared beaming parameter. With the diameter and tabulated ","authors_text":"Marco Delbo', V\\'ictor Al\\'i-Lagoa","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-05-29T15:45:16Z","title":"Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.10263","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:4dea04ae264800631b28ef3d2a9e4cacca8954e75c6e53a955f42ff31cafbfab","target":"record","created_at":"2026-05-18T00:40:29Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"d151a6bb86a8297178cf1c78bb3fd3cf395ce26dd4562500ba24fa86d5eb3831","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-05-29T15:45:16Z","title_canon_sha256":"42641ee578a0ae0ea104f39e85752323969efb20719d62205717cc2a1914f1a1"},"schema_version":"1.0","source":{"id":"1705.10263","kind":"arxiv","version":1}},"canonical_sha256":"f7a070fbec2348a9fe755be0e7035885d141f9ad617ab9689164f70c71e19887","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"f7a070fbec2348a9fe755be0e7035885d141f9ad617ab9689164f70c71e19887","first_computed_at":"2026-05-18T00:40:29.886980Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:40:29.886980Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"pjRakim3SC7CdgVAByiIwedlAjhNLeU7JPpodlimWdCWsl5Zyd+DyvzSCUtMt5Ukpcyxv6DlvqSG1Ye4lqNgAg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:40:29.887403Z","signed_message":"canonical_sha256_bytes"},"source_id":"1705.10263","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:4dea04ae264800631b28ef3d2a9e4cacca8954e75c6e53a955f42ff31cafbfab","sha256:f259ddecf6166dd909c5d46030e16e2df0cd631b910bc1a6dd68f434f5bc83dd"],"state_sha256":"dbcbacffc285df69632e962c5411f92f849a53601204a0385db29fdb66b9300b"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"4Mon3Nd/LBOYPdDJQuvXAKDpI1k0P+1ZRczIiIQRw8OscqgCbld32dbgsOQVWa3cmpI7gK+AoEpJw2CDc6uSBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-10T18:44:31.852962Z","bundle_sha256":"386f7bfa2da7fbe34f388d2b2dbbecfa432fdaa78e1000d3f5473483401732ea"}}