{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:3OCT6XCXPUA37GBPHAC4IL3FGW","short_pith_number":"pith:3OCT6XCX","canonical_record":{"source":{"id":"1611.03510","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-10T21:02:00Z","cross_cats_sorted":[],"title_canon_sha256":"184aee2a7b52373ae6cabcb4d8bbc05b151809eebaafd9f3c70d9cbb208cae82","abstract_canon_sha256":"b69de35c6b937bed617a2d065c8e743a5d9c544b0f2218f801f0ba043d6bdcfc"},"schema_version":"1.0"},"canonical_sha256":"db853f5c577d01bf982f3805c42f653587a9802ad9f2942e12ca15286135ab53","source":{"kind":"arxiv","id":"1611.03510","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1611.03510","created_at":"2026-05-18T00:48:16Z"},{"alias_kind":"arxiv_version","alias_value":"1611.03510v3","created_at":"2026-05-18T00:48:16Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.03510","created_at":"2026-05-18T00:48:16Z"},{"alias_kind":"pith_short_12","alias_value":"3OCT6XCXPUA3","created_at":"2026-05-18T12:29:55Z"},{"alias_kind":"pith_short_16","alias_value":"3OCT6XCXPUA37GBP","created_at":"2026-05-18T12:29:55Z"},{"alias_kind":"pith_short_8","alias_value":"3OCT6XCX","created_at":"2026-05-18T12:29:55Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:3OCT6XCXPUA37GBPHAC4IL3FGW","target":"record","payload":{"canonical_record":{"source":{"id":"1611.03510","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-10T21:02:00Z","cross_cats_sorted":[],"title_canon_sha256":"184aee2a7b52373ae6cabcb4d8bbc05b151809eebaafd9f3c70d9cbb208cae82","abstract_canon_sha256":"b69de35c6b937bed617a2d065c8e743a5d9c544b0f2218f801f0ba043d6bdcfc"},"schema_version":"1.0"},"canonical_sha256":"db853f5c577d01bf982f3805c42f653587a9802ad9f2942e12ca15286135ab53","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:16.328435Z","signature_b64":"mJjzpqd1Odb75tOzq4vFwvJpJeAqnsQEUhBPQvPxmxZjoflW1oKnzPcHMCGSe82fk/gSN/K04SH8FpEdkietBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"db853f5c577d01bf982f3805c42f653587a9802ad9f2942e12ca15286135ab53","last_reissued_at":"2026-05-18T00:48:16.327715Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:16.327715Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1611.03510","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:48:16Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ZfwoLCtaR8GFVP2WXr+Y7xTAWS18Q7qsWb+G3asDpfKG7h6mefNS/sJHJCg6BEiRsm5NgxeeejwUJa6FNtGACA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T16:09:10.793922Z"},"content_sha256":"0b326e4d9f16c308da2af9e7bd503685e70b5d9daefb197b41b3e988f93343be","schema_version":"1.0","event_id":"sha256:0b326e4d9f16c308da2af9e7bd503685e70b5d9daefb197b41b3e988f93343be"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:3OCT6XCXPUA37GBPHAC4IL3FGW","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The Diversity of Diffuse Ly$\\alpha$ Nebulae around Star-Forming Galaxies at High Redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anthony H. Gonzalez, Arjun Dey, Buell T. Jannuzi, Hanae Inami, Kyoung-Soo Lee, Moire K. M. Prescott, Naveen Reddy, Rui Xue, Sungryong Hong","submitted_at":"2016-11-10T21:02:00Z","abstract_excerpt":"We report the detection of diffuse Ly$\\alpha$ emission, or Ly$\\alpha$ halos (LAHs), around star-forming galaxies at $z\\approx3.78$ and $2.66$ in the NOAO Deep Wide-Field Survey Bo\\\"otes field. Our samples consist of a total of $\\sim$1400 galaxies, within two separate regions containing spectroscopically confirmed galaxy overdensities. They provide a unique opportunity to investigate how the LAH characteristics vary with host galaxy large-scale environment and physical properties. We stack Ly$\\alpha$ images of different samples defined by these properties and measure their median LAH sizes by d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.03510","kind":"arxiv","version":3},"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":"2026-05-18T00:48:16Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Ts/cM6ePxSl9zouKqr3/ZTUnfdvxDPgRDnerztf0170uy9rK4uSF1IvTD0PR6rLebaK6ra/2jaeRoxhfgNAAAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T16:09:10.794275Z"},"content_sha256":"22fb4f0953e947453654cd92c9598617d728f786951d47b214ff7f96079b9c5c","schema_version":"1.0","event_id":"sha256:22fb4f0953e947453654cd92c9598617d728f786951d47b214ff7f96079b9c5c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/3OCT6XCXPUA37GBPHAC4IL3FGW/bundle.json","state_url":"https://pith.science/pith/3OCT6XCXPUA37GBPHAC4IL3FGW/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/3OCT6XCXPUA37GBPHAC4IL3FGW/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":"2026-05-26T16:09:10Z","links":{"resolver":"https://pith.science/pith/3OCT6XCXPUA37GBPHAC4IL3FGW","bundle":"https://pith.science/pith/3OCT6XCXPUA37GBPHAC4IL3FGW/bundle.json","state":"https://pith.science/pith/3OCT6XCXPUA37GBPHAC4IL3FGW/state.json","well_known_bundle":"https://pith.science/.well-known/pith/3OCT6XCXPUA37GBPHAC4IL3FGW/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:3OCT6XCXPUA37GBPHAC4IL3FGW","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":"b69de35c6b937bed617a2d065c8e743a5d9c544b0f2218f801f0ba043d6bdcfc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-10T21:02:00Z","title_canon_sha256":"184aee2a7b52373ae6cabcb4d8bbc05b151809eebaafd9f3c70d9cbb208cae82"},"schema_version":"1.0","source":{"id":"1611.03510","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1611.03510","created_at":"2026-05-18T00:48:16Z"},{"alias_kind":"arxiv_version","alias_value":"1611.03510v3","created_at":"2026-05-18T00:48:16Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.03510","created_at":"2026-05-18T00:48:16Z"},{"alias_kind":"pith_short_12","alias_value":"3OCT6XCXPUA3","created_at":"2026-05-18T12:29:55Z"},{"alias_kind":"pith_short_16","alias_value":"3OCT6XCXPUA37GBP","created_at":"2026-05-18T12:29:55Z"},{"alias_kind":"pith_short_8","alias_value":"3OCT6XCX","created_at":"2026-05-18T12:29:55Z"}],"graph_snapshots":[{"event_id":"sha256:22fb4f0953e947453654cd92c9598617d728f786951d47b214ff7f96079b9c5c","target":"graph","created_at":"2026-05-18T00:48:16Z","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 report the detection of diffuse Ly$\\alpha$ emission, or Ly$\\alpha$ halos (LAHs), around star-forming galaxies at $z\\approx3.78$ and $2.66$ in the NOAO Deep Wide-Field Survey Bo\\\"otes field. Our samples consist of a total of $\\sim$1400 galaxies, within two separate regions containing spectroscopically confirmed galaxy overdensities. They provide a unique opportunity to investigate how the LAH characteristics vary with host galaxy large-scale environment and physical properties. We stack Ly$\\alpha$ images of different samples defined by these properties and measure their median LAH sizes by d","authors_text":"Anthony H. Gonzalez, Arjun Dey, Buell T. Jannuzi, Hanae Inami, Kyoung-Soo Lee, Moire K. M. Prescott, Naveen Reddy, Rui Xue, Sungryong Hong","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-10T21:02:00Z","title":"The Diversity of Diffuse Ly$\\alpha$ Nebulae around Star-Forming Galaxies at High Redshift"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.03510","kind":"arxiv","version":3},"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":"sha256:0b326e4d9f16c308da2af9e7bd503685e70b5d9daefb197b41b3e988f93343be","target":"record","created_at":"2026-05-18T00:48:16Z","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":"b69de35c6b937bed617a2d065c8e743a5d9c544b0f2218f801f0ba043d6bdcfc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-10T21:02:00Z","title_canon_sha256":"184aee2a7b52373ae6cabcb4d8bbc05b151809eebaafd9f3c70d9cbb208cae82"},"schema_version":"1.0","source":{"id":"1611.03510","kind":"arxiv","version":3}},"canonical_sha256":"db853f5c577d01bf982f3805c42f653587a9802ad9f2942e12ca15286135ab53","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"db853f5c577d01bf982f3805c42f653587a9802ad9f2942e12ca15286135ab53","first_computed_at":"2026-05-18T00:48:16.327715Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:48:16.327715Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"mJjzpqd1Odb75tOzq4vFwvJpJeAqnsQEUhBPQvPxmxZjoflW1oKnzPcHMCGSe82fk/gSN/K04SH8FpEdkietBw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:48:16.328435Z","signed_message":"canonical_sha256_bytes"},"source_id":"1611.03510","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0b326e4d9f16c308da2af9e7bd503685e70b5d9daefb197b41b3e988f93343be","sha256:22fb4f0953e947453654cd92c9598617d728f786951d47b214ff7f96079b9c5c"],"state_sha256":"28471d53d64acc787a1af7ef62613b94c8f5d7c8cd7eeda327fd42048b9fbc9f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"iCBeTgUB+THd414HnK+SJ8vzUIk68yT/hI6LLdxPp+nvJsFTYiqWPHbVQZTo+8wpQFi1gPpBd2TuPaRGgkupCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T16:09:10.796620Z","bundle_sha256":"1a784c5c4f43781ffe7d912508a67f93c50301de5a360403b47edc6c9ba4fff6"}}