{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:SYG2NY3N44AIZSCJDXDRC4RI6W","short_pith_number":"pith:SYG2NY3N","canonical_record":{"source":{"id":"1606.00184","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-01T09:22:49Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"b7ce6e56844e7d02f3ff10da3e1a9f9e17a8e9285f3266ab0bda913fac5a8ba3","abstract_canon_sha256":"1b0917fd9ef107be10af58e3e4440d4b2e411616dd6341772156cf032b9313a6"},"schema_version":"1.0"},"canonical_sha256":"960da6e36de7008cc8491dc7117228f5bd33acefcd95c73ce7acdb927faae99f","source":{"kind":"arxiv","id":"1606.00184","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1606.00184","created_at":"2026-05-18T01:09:30Z"},{"alias_kind":"arxiv_version","alias_value":"1606.00184v1","created_at":"2026-05-18T01:09:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.00184","created_at":"2026-05-18T01:09:30Z"},{"alias_kind":"pith_short_12","alias_value":"SYG2NY3N44AI","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_16","alias_value":"SYG2NY3N44AIZSCJ","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_8","alias_value":"SYG2NY3N","created_at":"2026-05-18T12:30:44Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:SYG2NY3N44AIZSCJDXDRC4RI6W","target":"record","payload":{"canonical_record":{"source":{"id":"1606.00184","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-01T09:22:49Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"b7ce6e56844e7d02f3ff10da3e1a9f9e17a8e9285f3266ab0bda913fac5a8ba3","abstract_canon_sha256":"1b0917fd9ef107be10af58e3e4440d4b2e411616dd6341772156cf032b9313a6"},"schema_version":"1.0"},"canonical_sha256":"960da6e36de7008cc8491dc7117228f5bd33acefcd95c73ce7acdb927faae99f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:30.766489Z","signature_b64":"lRVCeUGy3yc70H90BJWG0C0p+AjFvlAXtBM2s4Up517F3NdJmN8QGiGgOwUWsR1n82JD0zv0Ddgv7McKVpIWAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"960da6e36de7008cc8491dc7117228f5bd33acefcd95c73ce7acdb927faae99f","last_reissued_at":"2026-05-18T01:09:30.765843Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:30.765843Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1606.00184","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":"2026-05-18T01:09:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"UoXLl/w4l83Od7YAhvJf0DAhOxIhmOoDMHbFu2P7NdLM6NlG+ny9LuNQild9ma8iPvjJyrRMDvHmlQ/V8IE2Cg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T05:40:41.027997Z"},"content_sha256":"abd3801828d9b222bff7ea00bea3ab16deff05384244f5ed6f20b6bfddc35c2d","schema_version":"1.0","event_id":"sha256:abd3801828d9b222bff7ea00bea3ab16deff05384244f5ed6f20b6bfddc35c2d"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:SYG2NY3N44AIZSCJDXDRC4RI6W","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Changbom Park, Juhan Kim, Sungwook E. Hong","submitted_at":"2016-06-01T09:22:49Z","abstract_excerpt":"We develop a galaxy assignment scheme that populates dark matter halos with galaxies by tracing the most bound member particles (MBPs) of simulated halos. Several merger-timescale models based on analytic calculations and numerical simulations are adopted as the survival time of mock satellite galaxies. We build mock galaxy samples from halo merger data of the Horizon Run 4 $N$-body simulation from $z = 12-0$. We compare group properties and two-point correlation functions (2pCFs) of mock galaxies with those of volume-limited SDSS galaxies, with $r$-band absolute magnitudes of $\\mathcal{M}_r -"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.00184","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":"2026-05-18T01:09:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"h9TpV2wjmB43npDv31FFju5n+0QaNjpYTck3z3mX5NWpKwV3pD0inQPp+0sYe9AoolH9IB9GX2SJPGoq7RUWAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T05:40:41.028358Z"},"content_sha256":"46e0c8b4ee773f8aa2c621b2d408839421ce496942ec92441e4eb86e70fa72e2","schema_version":"1.0","event_id":"sha256:46e0c8b4ee773f8aa2c621b2d408839421ce496942ec92441e4eb86e70fa72e2"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/SYG2NY3N44AIZSCJDXDRC4RI6W/bundle.json","state_url":"https://pith.science/pith/SYG2NY3N44AIZSCJDXDRC4RI6W/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/SYG2NY3N44AIZSCJDXDRC4RI6W/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":"2026-05-28T05:40:41Z","links":{"resolver":"https://pith.science/pith/SYG2NY3N44AIZSCJDXDRC4RI6W","bundle":"https://pith.science/pith/SYG2NY3N44AIZSCJDXDRC4RI6W/bundle.json","state":"https://pith.science/pith/SYG2NY3N44AIZSCJDXDRC4RI6W/state.json","well_known_bundle":"https://pith.science/.well-known/pith/SYG2NY3N44AIZSCJDXDRC4RI6W/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:SYG2NY3N44AIZSCJDXDRC4RI6W","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":"1b0917fd9ef107be10af58e3e4440d4b2e411616dd6341772156cf032b9313a6","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-01T09:22:49Z","title_canon_sha256":"b7ce6e56844e7d02f3ff10da3e1a9f9e17a8e9285f3266ab0bda913fac5a8ba3"},"schema_version":"1.0","source":{"id":"1606.00184","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1606.00184","created_at":"2026-05-18T01:09:30Z"},{"alias_kind":"arxiv_version","alias_value":"1606.00184v1","created_at":"2026-05-18T01:09:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.00184","created_at":"2026-05-18T01:09:30Z"},{"alias_kind":"pith_short_12","alias_value":"SYG2NY3N44AI","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_16","alias_value":"SYG2NY3N44AIZSCJ","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_8","alias_value":"SYG2NY3N","created_at":"2026-05-18T12:30:44Z"}],"graph_snapshots":[{"event_id":"sha256:46e0c8b4ee773f8aa2c621b2d408839421ce496942ec92441e4eb86e70fa72e2","target":"graph","created_at":"2026-05-18T01:09:30Z","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 develop a galaxy assignment scheme that populates dark matter halos with galaxies by tracing the most bound member particles (MBPs) of simulated halos. Several merger-timescale models based on analytic calculations and numerical simulations are adopted as the survival time of mock satellite galaxies. We build mock galaxy samples from halo merger data of the Horizon Run 4 $N$-body simulation from $z = 12-0$. We compare group properties and two-point correlation functions (2pCFs) of mock galaxies with those of volume-limited SDSS galaxies, with $r$-band absolute magnitudes of $\\mathcal{M}_r -","authors_text":"Changbom Park, Juhan Kim, Sungwook E. Hong","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-01T09:22:49Z","title":"The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.00184","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:abd3801828d9b222bff7ea00bea3ab16deff05384244f5ed6f20b6bfddc35c2d","target":"record","created_at":"2026-05-18T01:09:30Z","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":"1b0917fd9ef107be10af58e3e4440d4b2e411616dd6341772156cf032b9313a6","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-01T09:22:49Z","title_canon_sha256":"b7ce6e56844e7d02f3ff10da3e1a9f9e17a8e9285f3266ab0bda913fac5a8ba3"},"schema_version":"1.0","source":{"id":"1606.00184","kind":"arxiv","version":1}},"canonical_sha256":"960da6e36de7008cc8491dc7117228f5bd33acefcd95c73ce7acdb927faae99f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"960da6e36de7008cc8491dc7117228f5bd33acefcd95c73ce7acdb927faae99f","first_computed_at":"2026-05-18T01:09:30.765843Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:09:30.765843Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"lRVCeUGy3yc70H90BJWG0C0p+AjFvlAXtBM2s4Up517F3NdJmN8QGiGgOwUWsR1n82JD0zv0Ddgv7McKVpIWAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:09:30.766489Z","signed_message":"canonical_sha256_bytes"},"source_id":"1606.00184","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:abd3801828d9b222bff7ea00bea3ab16deff05384244f5ed6f20b6bfddc35c2d","sha256:46e0c8b4ee773f8aa2c621b2d408839421ce496942ec92441e4eb86e70fa72e2"],"state_sha256":"e74839f8edb83b4a87849a4da7edeae85753f3f0820dbe76a893b3aef17ba493"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"OrfgsZ/2ngFVT1RrZBC1bDtnohkVAmxlAoKCq8Ajgo6YP1lhikyV0S0O6mwGAALQU8X+PW3RSFhMtQKbrMaeCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T05:40:41.030414Z","bundle_sha256":"c558da4400039c95a3fe4233158cdd0ba81a6e85ee291aec728bb067057fa2cc"}}