{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2004:CB6VDJSZOXLJFQIDPR562UXAW6","short_pith_number":"pith:CB6VDJSZ","canonical_record":{"source":{"id":"astro-ph/0410257","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-11T08:29:46Z","cross_cats_sorted":[],"title_canon_sha256":"336956ddddaa4b09e52629b64b270e80cdd00402715b170e6170858cb46e89b5","abstract_canon_sha256":"413d11a7beeb059cb0eeb38d61021be9398c1f03b03cdcdb3d7394b52d65a4cd"},"schema_version":"1.0"},"canonical_sha256":"107d51a65975d692c1037c7bed52e0b7b122525cafc7138a6c57926882cc8ab1","source":{"kind":"arxiv","id":"astro-ph/0410257","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0410257","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0410257v1","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0410257","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"pith_short_12","alias_value":"CB6VDJSZOXLJ","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"pith_short_16","alias_value":"CB6VDJSZOXLJFQID","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"pith_short_8","alias_value":"CB6VDJSZ","created_at":"2026-07-04T16:44:56Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2004:CB6VDJSZOXLJFQIDPR562UXAW6","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0410257","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-11T08:29:46Z","cross_cats_sorted":[],"title_canon_sha256":"336956ddddaa4b09e52629b64b270e80cdd00402715b170e6170858cb46e89b5","abstract_canon_sha256":"413d11a7beeb059cb0eeb38d61021be9398c1f03b03cdcdb3d7394b52d65a4cd"},"schema_version":"1.0"},"canonical_sha256":"107d51a65975d692c1037c7bed52e0b7b122525cafc7138a6c57926882cc8ab1","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:44:56.914616Z","signature_b64":"pxF5wbAkcxllN2y2LoWs3kHVzY3sn+28jOArf7D1sd+mrCGcUb9LXyHvk8MkBISC3po6vVdKsYSZn/3NH1VUAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"107d51a65975d692c1037c7bed52e0b7b122525cafc7138a6c57926882cc8ab1","last_reissued_at":"2026-07-04T16:44:56.914155Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:44:56.914155Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0410257","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":"2026-07-04T16:44:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"J7UgcOKgYdnV/xWimDoMZx0pWOEC8g6FOZBUkJvftqXMwkJ0tUQybaPgkQhYLAcGhB78fSQMrLofTVHLFdzFAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-09T23:38:12.003184Z"},"content_sha256":"8e33337acfe61eb39903b88edd287831ddd2ca015c616c3e3fa669a199842213","schema_version":"1.0","event_id":"sha256:8e33337acfe61eb39903b88edd287831ddd2ca015c616c3e3fa669a199842213"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2004:CB6VDJSZOXLJFQIDPR562UXAW6","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Looking for outflows from brown dwarfs","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A.C. Raga, E. Masciadri","submitted_at":"2004-10-11T08:29:46Z","abstract_excerpt":"First evidences of IR excess and disk mass accretion (strong H$\\alpha$ emission) around brown dwarfs seem to indicate the existence of circumstellar disks around these sub-stellar objects. Nothing is known at the present time about outflows which potentially might be launched from brown dwarfs, although jets are typically associated with the accretion in standard T Tauri star disks. In this paper we calculate the H$\\alpha$ emission of internal working surfaces produced by a radiative jet in a neutral and in a photoionized environment as a function of the jet parameters (the ejection velocity $"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0410257","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0410257/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:44:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"fhgo3kqghC41vP71T2c2fZ2f2/6MDTw1atwXnaCFEhVa6/Ee+y0qgyvg0rqT6RG9k1+rztwmEq1zToI+ZiZuBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-09T23:38:12.003568Z"},"content_sha256":"f725b8e0ec3166ce6def09bceb25fcca32a3e2e60b0ae675d3f251fe9efa5340","schema_version":"1.0","event_id":"sha256:f725b8e0ec3166ce6def09bceb25fcca32a3e2e60b0ae675d3f251fe9efa5340"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/CB6VDJSZOXLJFQIDPR562UXAW6/bundle.json","state_url":"https://pith.science/pith/CB6VDJSZOXLJFQIDPR562UXAW6/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/CB6VDJSZOXLJFQIDPR562UXAW6/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":"2026-07-09T23:38:12Z","links":{"resolver":"https://pith.science/pith/CB6VDJSZOXLJFQIDPR562UXAW6","bundle":"https://pith.science/pith/CB6VDJSZOXLJFQIDPR562UXAW6/bundle.json","state":"https://pith.science/pith/CB6VDJSZOXLJFQIDPR562UXAW6/state.json","well_known_bundle":"https://pith.science/.well-known/pith/CB6VDJSZOXLJFQIDPR562UXAW6/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2004:CB6VDJSZOXLJFQIDPR562UXAW6","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":"413d11a7beeb059cb0eeb38d61021be9398c1f03b03cdcdb3d7394b52d65a4cd","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-11T08:29:46Z","title_canon_sha256":"336956ddddaa4b09e52629b64b270e80cdd00402715b170e6170858cb46e89b5"},"schema_version":"1.0","source":{"id":"astro-ph/0410257","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0410257","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0410257v1","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0410257","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"pith_short_12","alias_value":"CB6VDJSZOXLJ","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"pith_short_16","alias_value":"CB6VDJSZOXLJFQID","created_at":"2026-07-04T16:44:56Z"},{"alias_kind":"pith_short_8","alias_value":"CB6VDJSZ","created_at":"2026-07-04T16:44:56Z"}],"graph_snapshots":[{"event_id":"sha256:f725b8e0ec3166ce6def09bceb25fcca32a3e2e60b0ae675d3f251fe9efa5340","target":"graph","created_at":"2026-07-04T16:44:56Z","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"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/astro-ph/0410257/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"First evidences of IR excess and disk mass accretion (strong H$\\alpha$ emission) around brown dwarfs seem to indicate the existence of circumstellar disks around these sub-stellar objects. Nothing is known at the present time about outflows which potentially might be launched from brown dwarfs, although jets are typically associated with the accretion in standard T Tauri star disks. In this paper we calculate the H$\\alpha$ emission of internal working surfaces produced by a radiative jet in a neutral and in a photoionized environment as a function of the jet parameters (the ejection velocity $","authors_text":"A.C. Raga, E. Masciadri","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2004-10-11T08:29:46Z","title":"Looking for outflows from brown dwarfs"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0410257","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":"sha256:8e33337acfe61eb39903b88edd287831ddd2ca015c616c3e3fa669a199842213","target":"record","created_at":"2026-07-04T16:44:56Z","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":"413d11a7beeb059cb0eeb38d61021be9398c1f03b03cdcdb3d7394b52d65a4cd","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-11T08:29:46Z","title_canon_sha256":"336956ddddaa4b09e52629b64b270e80cdd00402715b170e6170858cb46e89b5"},"schema_version":"1.0","source":{"id":"astro-ph/0410257","kind":"arxiv","version":1}},"canonical_sha256":"107d51a65975d692c1037c7bed52e0b7b122525cafc7138a6c57926882cc8ab1","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"107d51a65975d692c1037c7bed52e0b7b122525cafc7138a6c57926882cc8ab1","first_computed_at":"2026-07-04T16:44:56.914155Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T16:44:56.914155Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"pxF5wbAkcxllN2y2LoWs3kHVzY3sn+28jOArf7D1sd+mrCGcUb9LXyHvk8MkBISC3po6vVdKsYSZn/3NH1VUAw==","signature_status":"signed_v1","signed_at":"2026-07-04T16:44:56.914616Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0410257","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8e33337acfe61eb39903b88edd287831ddd2ca015c616c3e3fa669a199842213","sha256:f725b8e0ec3166ce6def09bceb25fcca32a3e2e60b0ae675d3f251fe9efa5340"],"state_sha256":"cf080201b7026052a646af2a4c5f76c3e48b07687963c3376c82c529798a925f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"XchXCJgWqLqLQWzdRTekc3DA3mjHc8XlB5Wi+c0jqwQUZOBoUxoAWJQC0DskWq2SOhPk5GIFauTqa93+H93tBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-09T23:38:12.005511Z","bundle_sha256":"542dd0f0b2048a59d9315eebf996b87874b40461aee3d0c5aa9458867cacdd71"}}