{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:EM6SJ4LDAPFTICPQP6F6OIZGDF","short_pith_number":"pith:EM6SJ4LD","canonical_record":{"source":{"id":"1411.4557","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-11-17T17:21:58Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"14d488c4a5908d1d587714c1799a0e56c9813f31fbf3152f48b123520f526866","abstract_canon_sha256":"4b9447c9b8fcd6a23c9dbed6d477b52d6de4282ad3b3cea702607e356488dac8"},"schema_version":"1.0"},"canonical_sha256":"233d24f16303cb3409f07f8be723261977659f2be0b59a80419adfb92c14c95c","source":{"kind":"arxiv","id":"1411.4557","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.4557","created_at":"2026-05-18T02:35:45Z"},{"alias_kind":"arxiv_version","alias_value":"1411.4557v1","created_at":"2026-05-18T02:35:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.4557","created_at":"2026-05-18T02:35:45Z"},{"alias_kind":"pith_short_12","alias_value":"EM6SJ4LDAPFT","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_16","alias_value":"EM6SJ4LDAPFTICPQ","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_8","alias_value":"EM6SJ4LD","created_at":"2026-05-18T12:28:28Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:EM6SJ4LDAPFTICPQP6F6OIZGDF","target":"record","payload":{"canonical_record":{"source":{"id":"1411.4557","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-11-17T17:21:58Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"14d488c4a5908d1d587714c1799a0e56c9813f31fbf3152f48b123520f526866","abstract_canon_sha256":"4b9447c9b8fcd6a23c9dbed6d477b52d6de4282ad3b3cea702607e356488dac8"},"schema_version":"1.0"},"canonical_sha256":"233d24f16303cb3409f07f8be723261977659f2be0b59a80419adfb92c14c95c","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:35:45.490092Z","signature_b64":"CfyI/siVKHjktGYxb09HMGmyPXH47J3Vk25yLgPGllRcwsWRKF3vf3sXEzGoa8yWuLRJJDJ+K5YTbAoJ9B+gBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"233d24f16303cb3409f07f8be723261977659f2be0b59a80419adfb92c14c95c","last_reissued_at":"2026-05-18T02:35:45.489647Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:35:45.489647Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1411.4557","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":"2026-05-18T02:35:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"XLfM6Fzw4nWxexi3/BXgLsZrurK7BJ0QHCKnFTBpZGYjMyewSj5K8B4wteGXko6EY8YStXETV7IENXb5aXhzDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T16:51:03.800203Z"},"content_sha256":"c1ffac6b03ba057fbf4e563845113fec52037aea5d3d46c843be4f7f066ce562","schema_version":"1.0","event_id":"sha256:c1ffac6b03ba057fbf4e563845113fec52037aea5d3d46c843be4f7f066ce562"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:EM6SJ4LDAPFTICPQP6F6OIZGDF","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Unbinned halo-independent methods for emerging dark matter signals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Yonatan Kahn","submitted_at":"2014-11-17T17:21:58Z","abstract_excerpt":"Halo-independent methods for analyzing direct detection experiments can provide robust results while making no assumptions about the dark matter halo in our galaxy. We extend existing methods to the case of unbinned data, which is especially well suited to emerging dark matter signals with only a few events in a nearly background-free environment. We show that such methods can easily be generalized to the case of inelastic or exothermic scattering, and provide a useful handle on extracting results independent of the halo model while maximizing the available experimental information."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.4557","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":"2026-05-18T02:35:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PtNBig6Ntnk/hfsWx/3qjB+vmOPLI4AOfs18SEEmLJrScBNiT6vS8n4DNWzOARKQEN2BkN/F/k6bvlxKKJCOBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T16:51:03.800604Z"},"content_sha256":"ed66d1a36b5282180ddca2037f5f01cd704c4c4c209ee40f52d003951b41479d","schema_version":"1.0","event_id":"sha256:ed66d1a36b5282180ddca2037f5f01cd704c4c4c209ee40f52d003951b41479d"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/EM6SJ4LDAPFTICPQP6F6OIZGDF/bundle.json","state_url":"https://pith.science/pith/EM6SJ4LDAPFTICPQP6F6OIZGDF/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/EM6SJ4LDAPFTICPQP6F6OIZGDF/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":"2026-06-11T16:51:03Z","links":{"resolver":"https://pith.science/pith/EM6SJ4LDAPFTICPQP6F6OIZGDF","bundle":"https://pith.science/pith/EM6SJ4LDAPFTICPQP6F6OIZGDF/bundle.json","state":"https://pith.science/pith/EM6SJ4LDAPFTICPQP6F6OIZGDF/state.json","well_known_bundle":"https://pith.science/.well-known/pith/EM6SJ4LDAPFTICPQP6F6OIZGDF/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:EM6SJ4LDAPFTICPQP6F6OIZGDF","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":"4b9447c9b8fcd6a23c9dbed6d477b52d6de4282ad3b3cea702607e356488dac8","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-11-17T17:21:58Z","title_canon_sha256":"14d488c4a5908d1d587714c1799a0e56c9813f31fbf3152f48b123520f526866"},"schema_version":"1.0","source":{"id":"1411.4557","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.4557","created_at":"2026-05-18T02:35:45Z"},{"alias_kind":"arxiv_version","alias_value":"1411.4557v1","created_at":"2026-05-18T02:35:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.4557","created_at":"2026-05-18T02:35:45Z"},{"alias_kind":"pith_short_12","alias_value":"EM6SJ4LDAPFT","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_16","alias_value":"EM6SJ4LDAPFTICPQ","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_8","alias_value":"EM6SJ4LD","created_at":"2026-05-18T12:28:28Z"}],"graph_snapshots":[{"event_id":"sha256:ed66d1a36b5282180ddca2037f5f01cd704c4c4c209ee40f52d003951b41479d","target":"graph","created_at":"2026-05-18T02:35:45Z","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":"Halo-independent methods for analyzing direct detection experiments can provide robust results while making no assumptions about the dark matter halo in our galaxy. We extend existing methods to the case of unbinned data, which is especially well suited to emerging dark matter signals with only a few events in a nearly background-free environment. We show that such methods can easily be generalized to the case of inelastic or exothermic scattering, and provide a useful handle on extracting results independent of the halo model while maximizing the available experimental information.","authors_text":"Yonatan Kahn","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-11-17T17:21:58Z","title":"Unbinned halo-independent methods for emerging dark matter signals"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.4557","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:c1ffac6b03ba057fbf4e563845113fec52037aea5d3d46c843be4f7f066ce562","target":"record","created_at":"2026-05-18T02:35:45Z","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":"4b9447c9b8fcd6a23c9dbed6d477b52d6de4282ad3b3cea702607e356488dac8","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-11-17T17:21:58Z","title_canon_sha256":"14d488c4a5908d1d587714c1799a0e56c9813f31fbf3152f48b123520f526866"},"schema_version":"1.0","source":{"id":"1411.4557","kind":"arxiv","version":1}},"canonical_sha256":"233d24f16303cb3409f07f8be723261977659f2be0b59a80419adfb92c14c95c","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"233d24f16303cb3409f07f8be723261977659f2be0b59a80419adfb92c14c95c","first_computed_at":"2026-05-18T02:35:45.489647Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:35:45.489647Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"CfyI/siVKHjktGYxb09HMGmyPXH47J3Vk25yLgPGllRcwsWRKF3vf3sXEzGoa8yWuLRJJDJ+K5YTbAoJ9B+gBw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:35:45.490092Z","signed_message":"canonical_sha256_bytes"},"source_id":"1411.4557","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:c1ffac6b03ba057fbf4e563845113fec52037aea5d3d46c843be4f7f066ce562","sha256:ed66d1a36b5282180ddca2037f5f01cd704c4c4c209ee40f52d003951b41479d"],"state_sha256":"be4da32d4f469221ac6b997d3de7e0916f293e58d836a47c7aab7ba9f5a10e36"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"hNpIxvPXYd4jNmdRIftzAtuFgrXsTCAW7/gD3w/7hiXgdkzGi8FyLGKk2tccXo36ckRmEo+IcIOrx4RPFVZyCw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-11T16:51:03.803049Z","bundle_sha256":"21ab21ac3e896163c38ff7d639076c59a95ca106aab2fe0046de9bfd5f31fd73"}}