{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:QN5TDK4RUVFMMFG5WXEDNOHMVH","short_pith_number":"pith:QN5TDK4R","canonical_record":{"source":{"id":"1312.1729","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-12-05T23:06:14Z","cross_cats_sorted":[],"title_canon_sha256":"2c588d93c75c8a65bf2d2da255f1a78f410b9070a189d104284698d0bfb4636a","abstract_canon_sha256":"2d09cc334a740d9e1169cef54064fa1d2c28cae99e13d6d052cb726fc4ad7ff6"},"schema_version":"1.0"},"canonical_sha256":"837b31ab91a54ac614ddb5c836b8eca9ee51f620a3a5ba4d5527461b9e3de5c3","source":{"kind":"arxiv","id":"1312.1729","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1312.1729","created_at":"2026-05-18T01:45:58Z"},{"alias_kind":"arxiv_version","alias_value":"1312.1729v3","created_at":"2026-05-18T01:45:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.1729","created_at":"2026-05-18T01:45:58Z"},{"alias_kind":"pith_short_12","alias_value":"QN5TDK4RUVFM","created_at":"2026-05-18T12:27:57Z"},{"alias_kind":"pith_short_16","alias_value":"QN5TDK4RUVFMMFG5","created_at":"2026-05-18T12:27:57Z"},{"alias_kind":"pith_short_8","alias_value":"QN5TDK4R","created_at":"2026-05-18T12:27:57Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:QN5TDK4RUVFMMFG5WXEDNOHMVH","target":"record","payload":{"canonical_record":{"source":{"id":"1312.1729","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-12-05T23:06:14Z","cross_cats_sorted":[],"title_canon_sha256":"2c588d93c75c8a65bf2d2da255f1a78f410b9070a189d104284698d0bfb4636a","abstract_canon_sha256":"2d09cc334a740d9e1169cef54064fa1d2c28cae99e13d6d052cb726fc4ad7ff6"},"schema_version":"1.0"},"canonical_sha256":"837b31ab91a54ac614ddb5c836b8eca9ee51f620a3a5ba4d5527461b9e3de5c3","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:58.031215Z","signature_b64":"5L2HvEO363qK7zqemWK/ecHxAIubXKmFjF4hafkaXPGZu5/bDv8RqeOX+EMXA9yQn0umZAs8uQ8ui/H+fmZTBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"837b31ab91a54ac614ddb5c836b8eca9ee51f620a3a5ba4d5527461b9e3de5c3","last_reissued_at":"2026-05-18T01:45:58.030793Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:58.030793Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1312.1729","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":"2026-05-18T01:45:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"MjAUcKNgIvaZFB8GEIs4VHAxVyQQrtlIFqVBppqSDYDIzGUFo5NHXmKq+x8TUpYHE8wyF+lGKuo+zyExWC+wDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T03:34:24.671305Z"},"content_sha256":"fbb1544377b57069952e5fa9064aee11dcab2cbc556bdff8f6543692e4889a50","schema_version":"1.0","event_id":"sha256:fbb1544377b57069952e5fa9064aee11dcab2cbc556bdff8f6543692e4889a50"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:QN5TDK4RUVFMMFG5WXEDNOHMVH","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The flattening of the concentration-mass relation towards low halo masses and its implications for the annihilation signal boost","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Campus of International Excellence UAM+CSIC, 3) ((1) KIPAC/SLAC, Francisco Prada (2, Madrid, Miguel A. Sanchez-Conde (1), Spain (3) Instituto de Fisica Teorica (UAM/CSIC), Stanford, Universidad Autonoma de Madrid)","submitted_at":"2013-12-05T23:06:14Z","abstract_excerpt":"In the standard Cold Dark Matter (CDM) theory for understanding the formation of structure in the universe, there exists a tight connection between the properties of dark matter (DM) haloes, and their formation epochs. Such relation can be expressed in terms of a single key parameter, namely the halo concentration. In this work, we examine the median concentration-mass relation, c(M), at present time, over more than 20 orders of magnitude in halo mass, i.e., from tiny Earth-mass microhalos up to galaxy clusters. The c(M) model proposed by Prada et al. (2012), which links the halo concentration"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.1729","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":"2026-05-18T01:45:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"P/MOnN4L2I21OLjH9FqDeOT9yia+9qyXRHM3cUTALWY/b/zXiYSvTInR39vlROGMO1Qhf/u/G8B0NTOlBFCzCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T03:34:24.671685Z"},"content_sha256":"bf8e774ac1eb78862b64bca207cabdb674d213b76a2e64569e750b61354577d4","schema_version":"1.0","event_id":"sha256:bf8e774ac1eb78862b64bca207cabdb674d213b76a2e64569e750b61354577d4"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/QN5TDK4RUVFMMFG5WXEDNOHMVH/bundle.json","state_url":"https://pith.science/pith/QN5TDK4RUVFMMFG5WXEDNOHMVH/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/QN5TDK4RUVFMMFG5WXEDNOHMVH/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":"2026-06-01T03:34:24Z","links":{"resolver":"https://pith.science/pith/QN5TDK4RUVFMMFG5WXEDNOHMVH","bundle":"https://pith.science/pith/QN5TDK4RUVFMMFG5WXEDNOHMVH/bundle.json","state":"https://pith.science/pith/QN5TDK4RUVFMMFG5WXEDNOHMVH/state.json","well_known_bundle":"https://pith.science/.well-known/pith/QN5TDK4RUVFMMFG5WXEDNOHMVH/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:QN5TDK4RUVFMMFG5WXEDNOHMVH","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":"2d09cc334a740d9e1169cef54064fa1d2c28cae99e13d6d052cb726fc4ad7ff6","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-12-05T23:06:14Z","title_canon_sha256":"2c588d93c75c8a65bf2d2da255f1a78f410b9070a189d104284698d0bfb4636a"},"schema_version":"1.0","source":{"id":"1312.1729","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1312.1729","created_at":"2026-05-18T01:45:58Z"},{"alias_kind":"arxiv_version","alias_value":"1312.1729v3","created_at":"2026-05-18T01:45:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.1729","created_at":"2026-05-18T01:45:58Z"},{"alias_kind":"pith_short_12","alias_value":"QN5TDK4RUVFM","created_at":"2026-05-18T12:27:57Z"},{"alias_kind":"pith_short_16","alias_value":"QN5TDK4RUVFMMFG5","created_at":"2026-05-18T12:27:57Z"},{"alias_kind":"pith_short_8","alias_value":"QN5TDK4R","created_at":"2026-05-18T12:27:57Z"}],"graph_snapshots":[{"event_id":"sha256:bf8e774ac1eb78862b64bca207cabdb674d213b76a2e64569e750b61354577d4","target":"graph","created_at":"2026-05-18T01:45:58Z","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":"In the standard Cold Dark Matter (CDM) theory for understanding the formation of structure in the universe, there exists a tight connection between the properties of dark matter (DM) haloes, and their formation epochs. Such relation can be expressed in terms of a single key parameter, namely the halo concentration. In this work, we examine the median concentration-mass relation, c(M), at present time, over more than 20 orders of magnitude in halo mass, i.e., from tiny Earth-mass microhalos up to galaxy clusters. The c(M) model proposed by Prada et al. (2012), which links the halo concentration","authors_text":"(2) Campus of International Excellence UAM+CSIC, 3) ((1) KIPAC/SLAC, Francisco Prada (2, Madrid, Miguel A. Sanchez-Conde (1), Spain (3) Instituto de Fisica Teorica (UAM/CSIC), Stanford, Universidad Autonoma de Madrid)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-12-05T23:06:14Z","title":"The flattening of the concentration-mass relation towards low halo masses and its implications for the annihilation signal boost"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.1729","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:fbb1544377b57069952e5fa9064aee11dcab2cbc556bdff8f6543692e4889a50","target":"record","created_at":"2026-05-18T01:45:58Z","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":"2d09cc334a740d9e1169cef54064fa1d2c28cae99e13d6d052cb726fc4ad7ff6","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-12-05T23:06:14Z","title_canon_sha256":"2c588d93c75c8a65bf2d2da255f1a78f410b9070a189d104284698d0bfb4636a"},"schema_version":"1.0","source":{"id":"1312.1729","kind":"arxiv","version":3}},"canonical_sha256":"837b31ab91a54ac614ddb5c836b8eca9ee51f620a3a5ba4d5527461b9e3de5c3","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"837b31ab91a54ac614ddb5c836b8eca9ee51f620a3a5ba4d5527461b9e3de5c3","first_computed_at":"2026-05-18T01:45:58.030793Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:45:58.030793Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"5L2HvEO363qK7zqemWK/ecHxAIubXKmFjF4hafkaXPGZu5/bDv8RqeOX+EMXA9yQn0umZAs8uQ8ui/H+fmZTBA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:45:58.031215Z","signed_message":"canonical_sha256_bytes"},"source_id":"1312.1729","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:fbb1544377b57069952e5fa9064aee11dcab2cbc556bdff8f6543692e4889a50","sha256:bf8e774ac1eb78862b64bca207cabdb674d213b76a2e64569e750b61354577d4"],"state_sha256":"764bb9e27a5412c2827da0a0e07950d979e3fc9613453c449b191b6167d8793f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1g69lBrqgKqwBpnvUdpwA/jFTgOrm15pLJ/3hqYZgCwhdhjKpL9nJH3n89I3OLfLPk8gx/PBON42KTycxFcPCw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T03:34:24.673660Z","bundle_sha256":"8c624755c463aec761a3237f22e7c106846acf35509aebef5bdc8e739ce3b0a9"}}