{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2006:ZAVNXFCSQKSHV5BIKFNUEB7M3D","short_pith_number":"pith:ZAVNXFCS","canonical_record":{"source":{"id":"astro-ph/0601690","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-01-30T17:41:38Z","cross_cats_sorted":[],"title_canon_sha256":"b837794f2a58602cbbd7a10adbf564353606b4a0e525e65fe795bc7c5e62b602","abstract_canon_sha256":"f2792471ca9578864aaba34178851201d57d15ac64fd433b1d39b8fd9588490a"},"schema_version":"1.0"},"canonical_sha256":"c82adb945282a47af428515b4207ecd8ee7df692bedb6aba90af0c2f8f97ce5d","source":{"kind":"arxiv","id":"astro-ph/0601690","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0601690","created_at":"2026-05-18T00:20:32Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0601690v1","created_at":"2026-05-18T00:20:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0601690","created_at":"2026-05-18T00:20:32Z"},{"alias_kind":"pith_short_12","alias_value":"ZAVNXFCSQKSH","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_16","alias_value":"ZAVNXFCSQKSHV5BI","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_8","alias_value":"ZAVNXFCS","created_at":"2026-05-18T12:25:54Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2006:ZAVNXFCSQKSHV5BIKFNUEB7M3D","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0601690","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-01-30T17:41:38Z","cross_cats_sorted":[],"title_canon_sha256":"b837794f2a58602cbbd7a10adbf564353606b4a0e525e65fe795bc7c5e62b602","abstract_canon_sha256":"f2792471ca9578864aaba34178851201d57d15ac64fd433b1d39b8fd9588490a"},"schema_version":"1.0"},"canonical_sha256":"c82adb945282a47af428515b4207ecd8ee7df692bedb6aba90af0c2f8f97ce5d","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:20:32.852891Z","signature_b64":"JfDu2T6AOyBL1KmfMD9IbNqdTY4G1hJLslJFQB5lGMxlsyik4vVrqLvnmF7oUgyAMc/8cAE/CEWx4GRlRJiCBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c82adb945282a47af428515b4207ecd8ee7df692bedb6aba90af0c2f8f97ce5d","last_reissued_at":"2026-05-18T00:20:32.852259Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:20:32.852259Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0601690","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":"2026-05-18T00:20:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"KfsAOoNEueoyDjfPYQiDvZMLo/9CM8pVYNgw4Em1RNyT7qL+PgxmLgUYUUV+SC0xuN1tU8OqbzHCwcN5SZACBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-10T01:12:11.448813Z"},"content_sha256":"255f84e8662e0add2db04c0b44dd60081f5e3920ccb26cdf07e1497a08d4540e","schema_version":"1.0","event_id":"sha256:255f84e8662e0add2db04c0b44dd60081f5e3920ccb26cdf07e1497a08d4540e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2006:ZAVNXFCSQKSHV5BIKFNUEB7M3D","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A radio and infrared exploration of the Cygnus X-3 environments","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) Dpto. de Ing. Mecanica y Minera, (3) Departament d'Astronomia i Meteorologia, 4), (4) Grupo de Investigacion FQM-322, A. J. Munoz-Arjonilla (4), D. Perez-Ramirez (1, EPS, J. L. Garrido (1, J. Marti (1, J. M. Paredes (3), J. R. Sanchez-Sutil (4) ((1) Departamento de Fisica, P. Luque-Escamilla (2, Spain, Spain), Universidad de Jaen, Universitat de Barcelona","submitted_at":"2006-01-30T17:41:38Z","abstract_excerpt":"To confirm, or rule out, the possible hot spot nature of two previously detected radio sources in the vicinity of the Cygnus X-3 microquasar.\n  We present the results of a radio and near infrared exploration of the several arc-minute field around the well known galactic relativistic jet source Cygnus X-3 using the Very Large Array and the Calar Alto 3.5~m telescope.\n  The data this paper is based on do not presently support the hot spot hypothesis. Instead, our new observations suggest that these sources are most likely background or foreground objects. Actually, none of them appears to be eve"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0601690","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":"2026-05-18T00:20:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3eqEr1/fxCG+i4q5vjf3MSVp/316VZCbLeAxH04HASgF2fb7rtjMd4rdpDCnYXPX+417XfCbNCuFHq9W+vvBAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-10T01:12:11.449561Z"},"content_sha256":"3cb3df9e507dae2224d958c5ca7cd7b2c7be2d74b13986f30c326662deb00c75","schema_version":"1.0","event_id":"sha256:3cb3df9e507dae2224d958c5ca7cd7b2c7be2d74b13986f30c326662deb00c75"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ZAVNXFCSQKSHV5BIKFNUEB7M3D/bundle.json","state_url":"https://pith.science/pith/ZAVNXFCSQKSHV5BIKFNUEB7M3D/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ZAVNXFCSQKSHV5BIKFNUEB7M3D/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":"2026-06-10T01:12:11Z","links":{"resolver":"https://pith.science/pith/ZAVNXFCSQKSHV5BIKFNUEB7M3D","bundle":"https://pith.science/pith/ZAVNXFCSQKSHV5BIKFNUEB7M3D/bundle.json","state":"https://pith.science/pith/ZAVNXFCSQKSHV5BIKFNUEB7M3D/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ZAVNXFCSQKSHV5BIKFNUEB7M3D/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2006:ZAVNXFCSQKSHV5BIKFNUEB7M3D","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":"f2792471ca9578864aaba34178851201d57d15ac64fd433b1d39b8fd9588490a","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-01-30T17:41:38Z","title_canon_sha256":"b837794f2a58602cbbd7a10adbf564353606b4a0e525e65fe795bc7c5e62b602"},"schema_version":"1.0","source":{"id":"astro-ph/0601690","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0601690","created_at":"2026-05-18T00:20:32Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0601690v1","created_at":"2026-05-18T00:20:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0601690","created_at":"2026-05-18T00:20:32Z"},{"alias_kind":"pith_short_12","alias_value":"ZAVNXFCSQKSH","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_16","alias_value":"ZAVNXFCSQKSHV5BI","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_8","alias_value":"ZAVNXFCS","created_at":"2026-05-18T12:25:54Z"}],"graph_snapshots":[{"event_id":"sha256:3cb3df9e507dae2224d958c5ca7cd7b2c7be2d74b13986f30c326662deb00c75","target":"graph","created_at":"2026-05-18T00:20:32Z","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":"To confirm, or rule out, the possible hot spot nature of two previously detected radio sources in the vicinity of the Cygnus X-3 microquasar.\n  We present the results of a radio and near infrared exploration of the several arc-minute field around the well known galactic relativistic jet source Cygnus X-3 using the Very Large Array and the Calar Alto 3.5~m telescope.\n  The data this paper is based on do not presently support the hot spot hypothesis. Instead, our new observations suggest that these sources are most likely background or foreground objects. Actually, none of them appears to be eve","authors_text":"(2) Dpto. de Ing. Mecanica y Minera, (3) Departament d'Astronomia i Meteorologia, 4), (4) Grupo de Investigacion FQM-322, A. J. Munoz-Arjonilla (4), D. Perez-Ramirez (1, EPS, J. L. Garrido (1, J. Marti (1, J. M. Paredes (3), J. R. Sanchez-Sutil (4) ((1) Departamento de Fisica, P. Luque-Escamilla (2, Spain, Spain), Universidad de Jaen, Universitat de Barcelona","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2006-01-30T17:41:38Z","title":"A radio and infrared exploration of the Cygnus X-3 environments"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0601690","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":"sha256:255f84e8662e0add2db04c0b44dd60081f5e3920ccb26cdf07e1497a08d4540e","target":"record","created_at":"2026-05-18T00:20:32Z","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":"f2792471ca9578864aaba34178851201d57d15ac64fd433b1d39b8fd9588490a","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-01-30T17:41:38Z","title_canon_sha256":"b837794f2a58602cbbd7a10adbf564353606b4a0e525e65fe795bc7c5e62b602"},"schema_version":"1.0","source":{"id":"astro-ph/0601690","kind":"arxiv","version":1}},"canonical_sha256":"c82adb945282a47af428515b4207ecd8ee7df692bedb6aba90af0c2f8f97ce5d","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"c82adb945282a47af428515b4207ecd8ee7df692bedb6aba90af0c2f8f97ce5d","first_computed_at":"2026-05-18T00:20:32.852259Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:20:32.852259Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"JfDu2T6AOyBL1KmfMD9IbNqdTY4G1hJLslJFQB5lGMxlsyik4vVrqLvnmF7oUgyAMc/8cAE/CEWx4GRlRJiCBA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:20:32.852891Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0601690","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:255f84e8662e0add2db04c0b44dd60081f5e3920ccb26cdf07e1497a08d4540e","sha256:3cb3df9e507dae2224d958c5ca7cd7b2c7be2d74b13986f30c326662deb00c75"],"state_sha256":"76b83cedcaeaff07f823507ada72dfe922dd022a01aab1127d84b9ef729cdebf"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2NKm51nKzSye6KRfYYMUyDyvaGKVrR8Ci0mhadLDlfO68SExVMvjGUlq7cVD/j3RWNV06UjOoN4gFZBi4O8JDg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-10T01:12:11.453470Z","bundle_sha256":"1554c7e99339e69e43a175040826b078d91428f830db1cdd8f4dbcedbb45084b"}}