{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:ZQ6656NZWIK5O7LM75EX4FYUNH","short_pith_number":"pith:ZQ6656NZ","canonical_record":{"source":{"id":"1408.0002","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-31T20:00:00Z","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"title_canon_sha256":"403211aaab8df627ca7df98070b42c0e5cecdf5065fed378d47179da7bd898e4","abstract_canon_sha256":"47b260aa1dbfc37df6e4265abf5ebeb80648d6887ae57e443e6d77197d4d2f9b"},"schema_version":"1.0"},"canonical_sha256":"cc3deef9b9b215d77d6cff497e171469e9ec3d099815f8de3c2dc35bf538c70a","source":{"kind":"arxiv","id":"1408.0002","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1408.0002","created_at":"2026-05-18T02:25:04Z"},{"alias_kind":"arxiv_version","alias_value":"1408.0002v2","created_at":"2026-05-18T02:25:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.0002","created_at":"2026-05-18T02:25:04Z"},{"alias_kind":"pith_short_12","alias_value":"ZQ6656NZWIK5","created_at":"2026-05-18T12:28:59Z"},{"alias_kind":"pith_short_16","alias_value":"ZQ6656NZWIK5O7LM","created_at":"2026-05-18T12:28:59Z"},{"alias_kind":"pith_short_8","alias_value":"ZQ6656NZ","created_at":"2026-05-18T12:28:59Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:ZQ6656NZWIK5O7LM75EX4FYUNH","target":"record","payload":{"canonical_record":{"source":{"id":"1408.0002","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-31T20:00:00Z","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"title_canon_sha256":"403211aaab8df627ca7df98070b42c0e5cecdf5065fed378d47179da7bd898e4","abstract_canon_sha256":"47b260aa1dbfc37df6e4265abf5ebeb80648d6887ae57e443e6d77197d4d2f9b"},"schema_version":"1.0"},"canonical_sha256":"cc3deef9b9b215d77d6cff497e171469e9ec3d099815f8de3c2dc35bf538c70a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:25:04.733726Z","signature_b64":"dh0qxgLgAboc/LepQD3gpfNtUW0S5khQp/rDJFk1DtZlze1AHGuXA3poWRx+z7uWiLbyMsT2Y6/km2uYl3pBCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc3deef9b9b215d77d6cff497e171469e9ec3d099815f8de3c2dc35bf538c70a","last_reissued_at":"2026-05-18T02:25:04.733380Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:25:04.733380Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1408.0002","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:25:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"LpvbpDzLdo93zrQb9zY0vloXhvfztmmDPEgW0ikRpH8hsDLf2FPh1FoGsMI2XpT1pIY2yn2SqZtyD4FzP0qfAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T03:01:22.678055Z"},"content_sha256":"0bce5a4052a5d08623e98cc77f6022543108c348d20af0e4c915f331947711a4","schema_version":"1.0","event_id":"sha256:0bce5a4052a5d08623e98cc77f6022543108c348d20af0e4c915f331947711a4"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:ZQ6656NZWIK5O7LM75EX4FYUNH","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Dwarf galaxy annihilation and decay emission profiles for dark matter experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Alex Geringer-Sameth, Matthew Walker, Savvas M. Koushiappas","submitted_at":"2014-07-31T20:00:00Z","abstract_excerpt":"Gamma-ray searches for dark matter annihilation and decay in dwarf galaxies rely on an understanding of the dark matter density profiles of these systems. Conversely, uncertainties in these density profiles propagate into the derived particle physics limits as systematic errors. In this paper we quantify the expected dark matter signal from 20 Milky Way dwarfs using a uniform analysis of the most recent stellar-kinematic data available. Assuming that the observed stellar populations are equilibrium tracers of spherically-symmetric gravitational potentials that are dominated by dark matter, we "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.0002","kind":"arxiv","version":2},"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":"2026-05-18T02:25:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"p8Lo3kl6EMTBiJJdPtDGoPINcm9aMDlWmYbttOBFoOdbee1YiEei/Zi8DUn4q5hMXJWBav1JhsDPSWr3foEWBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T03:01:22.678681Z"},"content_sha256":"c735f977e1c741bce4b9cd5529914a68366ea23f877532d5cdf7bdbf6e7aa259","schema_version":"1.0","event_id":"sha256:c735f977e1c741bce4b9cd5529914a68366ea23f877532d5cdf7bdbf6e7aa259"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ZQ6656NZWIK5O7LM75EX4FYUNH/bundle.json","state_url":"https://pith.science/pith/ZQ6656NZWIK5O7LM75EX4FYUNH/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ZQ6656NZWIK5O7LM75EX4FYUNH/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":"2026-06-04T03:01:22Z","links":{"resolver":"https://pith.science/pith/ZQ6656NZWIK5O7LM75EX4FYUNH","bundle":"https://pith.science/pith/ZQ6656NZWIK5O7LM75EX4FYUNH/bundle.json","state":"https://pith.science/pith/ZQ6656NZWIK5O7LM75EX4FYUNH/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ZQ6656NZWIK5O7LM75EX4FYUNH/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:ZQ6656NZWIK5O7LM75EX4FYUNH","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":"47b260aa1dbfc37df6e4265abf5ebeb80648d6887ae57e443e6d77197d4d2f9b","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-31T20:00:00Z","title_canon_sha256":"403211aaab8df627ca7df98070b42c0e5cecdf5065fed378d47179da7bd898e4"},"schema_version":"1.0","source":{"id":"1408.0002","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1408.0002","created_at":"2026-05-18T02:25:04Z"},{"alias_kind":"arxiv_version","alias_value":"1408.0002v2","created_at":"2026-05-18T02:25:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.0002","created_at":"2026-05-18T02:25:04Z"},{"alias_kind":"pith_short_12","alias_value":"ZQ6656NZWIK5","created_at":"2026-05-18T12:28:59Z"},{"alias_kind":"pith_short_16","alias_value":"ZQ6656NZWIK5O7LM","created_at":"2026-05-18T12:28:59Z"},{"alias_kind":"pith_short_8","alias_value":"ZQ6656NZ","created_at":"2026-05-18T12:28:59Z"}],"graph_snapshots":[{"event_id":"sha256:c735f977e1c741bce4b9cd5529914a68366ea23f877532d5cdf7bdbf6e7aa259","target":"graph","created_at":"2026-05-18T02:25:04Z","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":"Gamma-ray searches for dark matter annihilation and decay in dwarf galaxies rely on an understanding of the dark matter density profiles of these systems. Conversely, uncertainties in these density profiles propagate into the derived particle physics limits as systematic errors. In this paper we quantify the expected dark matter signal from 20 Milky Way dwarfs using a uniform analysis of the most recent stellar-kinematic data available. Assuming that the observed stellar populations are equilibrium tracers of spherically-symmetric gravitational potentials that are dominated by dark matter, we ","authors_text":"Alex Geringer-Sameth, Matthew Walker, Savvas M. Koushiappas","cross_cats":["astro-ph.GA","astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-31T20:00:00Z","title":"Dwarf galaxy annihilation and decay emission profiles for dark matter experiments"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.0002","kind":"arxiv","version":2},"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":"sha256:0bce5a4052a5d08623e98cc77f6022543108c348d20af0e4c915f331947711a4","target":"record","created_at":"2026-05-18T02:25:04Z","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":"47b260aa1dbfc37df6e4265abf5ebeb80648d6887ae57e443e6d77197d4d2f9b","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-31T20:00:00Z","title_canon_sha256":"403211aaab8df627ca7df98070b42c0e5cecdf5065fed378d47179da7bd898e4"},"schema_version":"1.0","source":{"id":"1408.0002","kind":"arxiv","version":2}},"canonical_sha256":"cc3deef9b9b215d77d6cff497e171469e9ec3d099815f8de3c2dc35bf538c70a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"cc3deef9b9b215d77d6cff497e171469e9ec3d099815f8de3c2dc35bf538c70a","first_computed_at":"2026-05-18T02:25:04.733380Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:25:04.733380Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"dh0qxgLgAboc/LepQD3gpfNtUW0S5khQp/rDJFk1DtZlze1AHGuXA3poWRx+z7uWiLbyMsT2Y6/km2uYl3pBCw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:25:04.733726Z","signed_message":"canonical_sha256_bytes"},"source_id":"1408.0002","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0bce5a4052a5d08623e98cc77f6022543108c348d20af0e4c915f331947711a4","sha256:c735f977e1c741bce4b9cd5529914a68366ea23f877532d5cdf7bdbf6e7aa259"],"state_sha256":"45560abd44d5fd9ea51088f63ca308062eeba65c399991f85ddc211aeafcd0af"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"oJgH8q7mUSwArM2nsyFDtfrKDIeLm/ycjANRpPaZQYT/YnF4uqfyRVAEFa5FAucPT3pMGcifUhDI8sQgeDA0Bg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T03:01:22.681380Z","bundle_sha256":"69d8e60a1d8c2ac879fda22d8cdfb9c0d22a251b9bcc34ad68fc9e355f88c905"}}