{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:GFE623BBOCSVQWOCMOP6P356HA","short_pith_number":"pith:GFE623BB","canonical_record":{"source":{"id":"1609.09832","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-30T17:43:31Z","cross_cats_sorted":[],"title_canon_sha256":"3b320497a443a306c61177a302218c6ec42292738d62eca5425863f300c7ba64","abstract_canon_sha256":"163309a3208bd7be8181867af4f5b3410a160ff41ba3425cbed147f628f7bd42"},"schema_version":"1.0"},"canonical_sha256":"3149ed6c2170a55859c2639fe7efbe383de35f79b690e7fd9feed0db811701f3","source":{"kind":"arxiv","id":"1609.09832","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1609.09832","created_at":"2026-05-18T01:03:33Z"},{"alias_kind":"arxiv_version","alias_value":"1609.09832v1","created_at":"2026-05-18T01:03:33Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.09832","created_at":"2026-05-18T01:03:33Z"},{"alias_kind":"pith_short_12","alias_value":"GFE623BBOCSV","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_16","alias_value":"GFE623BBOCSVQWOC","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_8","alias_value":"GFE623BB","created_at":"2026-05-18T12:30:19Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:GFE623BBOCSVQWOCMOP6P356HA","target":"record","payload":{"canonical_record":{"source":{"id":"1609.09832","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-30T17:43:31Z","cross_cats_sorted":[],"title_canon_sha256":"3b320497a443a306c61177a302218c6ec42292738d62eca5425863f300c7ba64","abstract_canon_sha256":"163309a3208bd7be8181867af4f5b3410a160ff41ba3425cbed147f628f7bd42"},"schema_version":"1.0"},"canonical_sha256":"3149ed6c2170a55859c2639fe7efbe383de35f79b690e7fd9feed0db811701f3","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:33.238956Z","signature_b64":"NR50f7IeF1IzMVlvpLaqZIGAvWv4AjK14fD1GlQSda+aQah+cdJ+tni5FbdD6ymRJbsF3DqLokcvybDrHAt5Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3149ed6c2170a55859c2639fe7efbe383de35f79b690e7fd9feed0db811701f3","last_reissued_at":"2026-05-18T01:03:33.238451Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:33.238451Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1609.09832","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":"2026-05-18T01:03:33Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IuW58BL5QV6R0b95J9wSQmICONcgBJCPhchaRKLlb4033YD4iQ9q3nUjccXj3e3HP3h/oQU7jnqo+864SvrhBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T07:48:39.533000Z"},"content_sha256":"ff9c6844f22638ac73c3328bd8f0551c1ecb065e7e0e3b2001446713f05b44fe","schema_version":"1.0","event_id":"sha256:ff9c6844f22638ac73c3328bd8f0551c1ecb065e7e0e3b2001446713f05b44fe"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:GFE623BBOCSVQWOCMOP6P356HA","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"How beaming of gravitational waves compares to the beaming of electromagnetic waves: impacts to gravitational wave detection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrew L. Miller, Thulsi Wickramasinghe","submitted_at":"2016-09-30T17:43:31Z","abstract_excerpt":"We focus on understanding the beaming of gravitational radiation from gamma ray bursts (GRBs) by approximating GRBs as linearly accelerated point masses. For accelerated point masses, it is known that gravitational radiation is beamed isotropicly at high speeds, and beamed along the polar axis at low speeds. Aside from this knowledge, there has been very little work done on beaming of gravitational radiation from GRBs, and the impact beaming could have on gravitational wave (GW) detection. We determine the following: (1) the observation angle at which the most power is emitted as a function of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.09832","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":"2026-05-18T01:03:33Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"yFkhHfcR6RHLF0MUkBPSyItr3S39B1CqArjLhnpIy1nc4JZ7hzx1i9sb6sEO8bln3glTF7HxFMWvfETUZ3+5Cg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T07:48:39.533361Z"},"content_sha256":"e9649bc46d8feb292c936e2c3e6cce7b6a20b3dfc7bb2441ece3521efa795adb","schema_version":"1.0","event_id":"sha256:e9649bc46d8feb292c936e2c3e6cce7b6a20b3dfc7bb2441ece3521efa795adb"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GFE623BBOCSVQWOCMOP6P356HA/bundle.json","state_url":"https://pith.science/pith/GFE623BBOCSVQWOCMOP6P356HA/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GFE623BBOCSVQWOCMOP6P356HA/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":"2026-06-02T07:48:39Z","links":{"resolver":"https://pith.science/pith/GFE623BBOCSVQWOCMOP6P356HA","bundle":"https://pith.science/pith/GFE623BBOCSVQWOCMOP6P356HA/bundle.json","state":"https://pith.science/pith/GFE623BBOCSVQWOCMOP6P356HA/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GFE623BBOCSVQWOCMOP6P356HA/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:GFE623BBOCSVQWOCMOP6P356HA","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":"163309a3208bd7be8181867af4f5b3410a160ff41ba3425cbed147f628f7bd42","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-30T17:43:31Z","title_canon_sha256":"3b320497a443a306c61177a302218c6ec42292738d62eca5425863f300c7ba64"},"schema_version":"1.0","source":{"id":"1609.09832","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1609.09832","created_at":"2026-05-18T01:03:33Z"},{"alias_kind":"arxiv_version","alias_value":"1609.09832v1","created_at":"2026-05-18T01:03:33Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.09832","created_at":"2026-05-18T01:03:33Z"},{"alias_kind":"pith_short_12","alias_value":"GFE623BBOCSV","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_16","alias_value":"GFE623BBOCSVQWOC","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_8","alias_value":"GFE623BB","created_at":"2026-05-18T12:30:19Z"}],"graph_snapshots":[{"event_id":"sha256:e9649bc46d8feb292c936e2c3e6cce7b6a20b3dfc7bb2441ece3521efa795adb","target":"graph","created_at":"2026-05-18T01:03:33Z","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":"We focus on understanding the beaming of gravitational radiation from gamma ray bursts (GRBs) by approximating GRBs as linearly accelerated point masses. For accelerated point masses, it is known that gravitational radiation is beamed isotropicly at high speeds, and beamed along the polar axis at low speeds. Aside from this knowledge, there has been very little work done on beaming of gravitational radiation from GRBs, and the impact beaming could have on gravitational wave (GW) detection. We determine the following: (1) the observation angle at which the most power is emitted as a function of","authors_text":"Andrew L. Miller, Thulsi Wickramasinghe","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-30T17:43:31Z","title":"How beaming of gravitational waves compares to the beaming of electromagnetic waves: impacts to gravitational wave detection"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.09832","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:ff9c6844f22638ac73c3328bd8f0551c1ecb065e7e0e3b2001446713f05b44fe","target":"record","created_at":"2026-05-18T01:03:33Z","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":"163309a3208bd7be8181867af4f5b3410a160ff41ba3425cbed147f628f7bd42","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-30T17:43:31Z","title_canon_sha256":"3b320497a443a306c61177a302218c6ec42292738d62eca5425863f300c7ba64"},"schema_version":"1.0","source":{"id":"1609.09832","kind":"arxiv","version":1}},"canonical_sha256":"3149ed6c2170a55859c2639fe7efbe383de35f79b690e7fd9feed0db811701f3","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3149ed6c2170a55859c2639fe7efbe383de35f79b690e7fd9feed0db811701f3","first_computed_at":"2026-05-18T01:03:33.238451Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:03:33.238451Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"NR50f7IeF1IzMVlvpLaqZIGAvWv4AjK14fD1GlQSda+aQah+cdJ+tni5FbdD6ymRJbsF3DqLokcvybDrHAt5Cg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:03:33.238956Z","signed_message":"canonical_sha256_bytes"},"source_id":"1609.09832","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ff9c6844f22638ac73c3328bd8f0551c1ecb065e7e0e3b2001446713f05b44fe","sha256:e9649bc46d8feb292c936e2c3e6cce7b6a20b3dfc7bb2441ece3521efa795adb"],"state_sha256":"cd4f05e2b92bba1510c8ae549f85629ad40a8f2358ba13cd41cc2cd420356f0b"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"tlwNrulcgtcYSHXg2CLKBpYKjqkP7ibsRRpz6VJxaxRTzpehhnslWrls9N/gi6V/C4Ck1biOAgN/8YMwDnIWCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T07:48:39.535336Z","bundle_sha256":"39512208874277fb4ad5df79f1c6fc3d66593601229607c17080f8db473b6dde"}}