{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:H5AH4ARMUWE3JB6SKDKMBTPJD5","short_pith_number":"pith:H5AH4ARM","canonical_record":{"source":{"id":"1605.05323","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-17T20:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"fbef14c7c1cc4e992a3cf293ca308793912332a9678e18be2692385aa3df4e92","abstract_canon_sha256":"43def40382973e2e5cc3fc6e1141d3b6c7817715404d01270a482e0debe2468d"},"schema_version":"1.0"},"canonical_sha256":"3f407e022ca589b487d250d4c0cde91f4952c67a68d3b8f136b6ad3600eb0734","source":{"kind":"arxiv","id":"1605.05323","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1605.05323","created_at":"2026-05-18T01:10:29Z"},{"alias_kind":"arxiv_version","alias_value":"1605.05323v3","created_at":"2026-05-18T01:10:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.05323","created_at":"2026-05-18T01:10:29Z"},{"alias_kind":"pith_short_12","alias_value":"H5AH4ARMUWE3","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_16","alias_value":"H5AH4ARMUWE3JB6S","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_8","alias_value":"H5AH4ARM","created_at":"2026-05-18T12:30:19Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:H5AH4ARMUWE3JB6SKDKMBTPJD5","target":"record","payload":{"canonical_record":{"source":{"id":"1605.05323","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-17T20:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"fbef14c7c1cc4e992a3cf293ca308793912332a9678e18be2692385aa3df4e92","abstract_canon_sha256":"43def40382973e2e5cc3fc6e1141d3b6c7817715404d01270a482e0debe2468d"},"schema_version":"1.0"},"canonical_sha256":"3f407e022ca589b487d250d4c0cde91f4952c67a68d3b8f136b6ad3600eb0734","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:29.643702Z","signature_b64":"3ygNqsyiPXvQDDQCif6WeSGEDz/MBK5k4K4enoDmCxHsQaxJGMq8OKTt+LbZwZH3S8EG5BBGYieJwrwfqk+JBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3f407e022ca589b487d250d4c0cde91f4952c67a68d3b8f136b6ad3600eb0734","last_reissued_at":"2026-05-18T01:10:29.643000Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:29.643000Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1605.05323","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":"2026-05-18T01:10:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"etX6p28Kydg8hKYIqK8qA6MfeONGqfdvF7KQ9WYUQqukGyvLtwx/c8dI/6lkIpYviFMnTn24CablWUB6zge8Bw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T04:25:57.094684Z"},"content_sha256":"b6c8d587794d93dab922e823d271a7a635dd0ac327951a94fd2ba378192498f9","schema_version":"1.0","event_id":"sha256:b6c8d587794d93dab922e823d271a7a635dd0ac327951a94fd2ba378192498f9"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:H5AH4ARMUWE3JB6SKDKMBTPJD5","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron A. Dutton (NYUAD), Andrea V. Macci\\`o (NYUAD, Arianna Di Cintio (DARK), Aura Obreja (NYUAD), Avishai Dekel (HUJI), Chris B. Brook (UAM), Gregory S. Stinson (MPIA), Liang Wang (PMO), MPIA), Tobias Buck (MPIA), Xi Kang (PMO)","submitted_at":"2016-05-17T20:00:01Z","abstract_excerpt":"We use ~100 cosmological galaxy formation zoom-in simulations using the smoothed particle hydrodynamics code {\\sc gasoline} to study the effect of baryonic processes on the mass profiles of cold dark matter haloes. The haloes in our study range from dwarf (M_{200}~10^{10}Msun) to Milky Way (M_{200}~10^{12}Msun) masses. Our simulations exhibit a wide range of halo responses, primarily varying with mass, from expansion to contraction, with up to factor ~10 changes in the enclosed dark matter mass at one per cent of the virial radius. Confirming previous studies, the halo response is correlated w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.05323","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":"2026-05-18T01:10:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"yzpRwXKjsBrjHKOb8vxw6D0/nAHYJzap3aDithCoEagDYyTNBQgzuHLlOaIUk9okz5zrJWnVLxnSZ/2yvPKACA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T04:25:57.095337Z"},"content_sha256":"3f2a16ecd9d10c58e8e4c668d48a717458915dec795bac153e9e9dc9b9862c27","schema_version":"1.0","event_id":"sha256:3f2a16ecd9d10c58e8e4c668d48a717458915dec795bac153e9e9dc9b9862c27"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/H5AH4ARMUWE3JB6SKDKMBTPJD5/bundle.json","state_url":"https://pith.science/pith/H5AH4ARMUWE3JB6SKDKMBTPJD5/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/H5AH4ARMUWE3JB6SKDKMBTPJD5/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":"2026-06-01T04:25:57Z","links":{"resolver":"https://pith.science/pith/H5AH4ARMUWE3JB6SKDKMBTPJD5","bundle":"https://pith.science/pith/H5AH4ARMUWE3JB6SKDKMBTPJD5/bundle.json","state":"https://pith.science/pith/H5AH4ARMUWE3JB6SKDKMBTPJD5/state.json","well_known_bundle":"https://pith.science/.well-known/pith/H5AH4ARMUWE3JB6SKDKMBTPJD5/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:H5AH4ARMUWE3JB6SKDKMBTPJD5","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":"43def40382973e2e5cc3fc6e1141d3b6c7817715404d01270a482e0debe2468d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-17T20:00:01Z","title_canon_sha256":"fbef14c7c1cc4e992a3cf293ca308793912332a9678e18be2692385aa3df4e92"},"schema_version":"1.0","source":{"id":"1605.05323","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1605.05323","created_at":"2026-05-18T01:10:29Z"},{"alias_kind":"arxiv_version","alias_value":"1605.05323v3","created_at":"2026-05-18T01:10:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.05323","created_at":"2026-05-18T01:10:29Z"},{"alias_kind":"pith_short_12","alias_value":"H5AH4ARMUWE3","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_16","alias_value":"H5AH4ARMUWE3JB6S","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_8","alias_value":"H5AH4ARM","created_at":"2026-05-18T12:30:19Z"}],"graph_snapshots":[{"event_id":"sha256:3f2a16ecd9d10c58e8e4c668d48a717458915dec795bac153e9e9dc9b9862c27","target":"graph","created_at":"2026-05-18T01:10:29Z","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 use ~100 cosmological galaxy formation zoom-in simulations using the smoothed particle hydrodynamics code {\\sc gasoline} to study the effect of baryonic processes on the mass profiles of cold dark matter haloes. The haloes in our study range from dwarf (M_{200}~10^{10}Msun) to Milky Way (M_{200}~10^{12}Msun) masses. Our simulations exhibit a wide range of halo responses, primarily varying with mass, from expansion to contraction, with up to factor ~10 changes in the enclosed dark matter mass at one per cent of the virial radius. Confirming previous studies, the halo response is correlated w","authors_text":"Aaron A. Dutton (NYUAD), Andrea V. Macci\\`o (NYUAD, Arianna Di Cintio (DARK), Aura Obreja (NYUAD), Avishai Dekel (HUJI), Chris B. Brook (UAM), Gregory S. Stinson (MPIA), Liang Wang (PMO), MPIA), Tobias Buck (MPIA), Xi Kang (PMO)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-17T20:00:01Z","title":"NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.05323","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:b6c8d587794d93dab922e823d271a7a635dd0ac327951a94fd2ba378192498f9","target":"record","created_at":"2026-05-18T01:10:29Z","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":"43def40382973e2e5cc3fc6e1141d3b6c7817715404d01270a482e0debe2468d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-17T20:00:01Z","title_canon_sha256":"fbef14c7c1cc4e992a3cf293ca308793912332a9678e18be2692385aa3df4e92"},"schema_version":"1.0","source":{"id":"1605.05323","kind":"arxiv","version":3}},"canonical_sha256":"3f407e022ca589b487d250d4c0cde91f4952c67a68d3b8f136b6ad3600eb0734","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3f407e022ca589b487d250d4c0cde91f4952c67a68d3b8f136b6ad3600eb0734","first_computed_at":"2026-05-18T01:10:29.643000Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:10:29.643000Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"3ygNqsyiPXvQDDQCif6WeSGEDz/MBK5k4K4enoDmCxHsQaxJGMq8OKTt+LbZwZH3S8EG5BBGYieJwrwfqk+JBA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:10:29.643702Z","signed_message":"canonical_sha256_bytes"},"source_id":"1605.05323","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:b6c8d587794d93dab922e823d271a7a635dd0ac327951a94fd2ba378192498f9","sha256:3f2a16ecd9d10c58e8e4c668d48a717458915dec795bac153e9e9dc9b9862c27"],"state_sha256":"0b7da705b52c03aab2e9e8939a93a159a35032b337fdd3a5104abae9f4301c88"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dn9eggUtsRPg+uOxuZkaEOHl15IgcUS0fz3CNVklSgF4wu8wrBfK0Z841cgGWCvyYa8G+S3sHAov+kx1LxvOAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T04:25:57.098512Z","bundle_sha256":"cdde846d2eeccf8270e921a44ffe82980127962fefa31d23586182f6a3bc70e1"}}