{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:MLM6CSRSSIQNIRXHUKSV5OOCZI","short_pith_number":"pith:MLM6CSRS","schema_version":"1.0","canonical_sha256":"62d9e14a329220d446e7a2a55eb9c2ca2045d576f5a9fb76daebe644c53dba76","source":{"kind":"arxiv","id":"1711.10489","version":3},"attestation_state":"computed","paper":{"title":"Revealing the Dark Matter Halo with Axion Direct Detection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Benjamin R. Safdi, Joshua W. Foster, Nicholas L. Rodd","submitted_at":"2017-11-28T19:00:00Z","abstract_excerpt":"The next generation of axion direct detection experiments may rule out or confirm axions as the dominant source of dark matter. We develop a general likelihood-based framework for studying the time-series data at such experiments, with a focus on the role of dark-matter astrophysics, to search for signatures of the QCD axion or axion like particles. We illustrate how in the event of a detection the likelihood framework may be used to extract measures of the local dark matter phase-space distribution, accounting for effects such as annual modulation and gravitational focusing, which is the pert"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1711.10489","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-28T19:00:00Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"35b4510e2d73f8299be82c376174758c9a331e38512872d0546a9b7124e407a2","abstract_canon_sha256":"ffe75eaa349f16e581f4831bacd61a872653f8e1a77b4d8afed9766598a1cdf5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:51:03.921631Z","signature_b64":"QgzwRyXDo520c9DHBiB7NQQ9C9oa2vpn+oM6BsRjt2t44IzYKJOT/5167sUXHlEmwIQldhtsxgLSPEdo5lRODQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"62d9e14a329220d446e7a2a55eb9c2ca2045d576f5a9fb76daebe644c53dba76","last_reissued_at":"2026-07-05T01:51:03.921258Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:51:03.921258Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revealing the Dark Matter Halo with Axion Direct Detection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Benjamin R. Safdi, Joshua W. Foster, Nicholas L. Rodd","submitted_at":"2017-11-28T19:00:00Z","abstract_excerpt":"The next generation of axion direct detection experiments may rule out or confirm axions as the dominant source of dark matter. We develop a general likelihood-based framework for studying the time-series data at such experiments, with a focus on the role of dark-matter astrophysics, to search for signatures of the QCD axion or axion like particles. We illustrate how in the event of a detection the likelihood framework may be used to extract measures of the local dark matter phase-space distribution, accounting for effects such as annual modulation and gravitational focusing, which is the pert"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.10489","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1711.10489/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1711.10489","created_at":"2026-07-05T01:51:03.921321+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.10489v3","created_at":"2026-07-05T01:51:03.921321+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.10489","created_at":"2026-07-05T01:51:03.921321+00:00"},{"alias_kind":"pith_short_12","alias_value":"MLM6CSRSSIQN","created_at":"2026-07-05T01:51:03.921321+00:00"},{"alias_kind":"pith_short_16","alias_value":"MLM6CSRSSIQNIRXH","created_at":"2026-07-05T01:51:03.921321+00:00"},{"alias_kind":"pith_short_8","alias_value":"MLM6CSRS","created_at":"2026-07-05T01:51:03.921321+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":13,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08248","citing_title":"Probing Quadratically Coupled Ultralight Dark Matter with the Laser Interferometer Space Antenna","ref_index":54,"is_internal_anchor":true},{"citing_arxiv_id":"2607.00072","citing_title":"Precision Solar System Dynamics for Ultralight Dark Matter Search","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28481","citing_title":"Background-Induced Forces from Quadratically Coupled Ultralight Dark Matter","ref_index":116,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28005","citing_title":"Transient axion streams from disrupted miniclusters","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"1907.04324","citing_title":"Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos","ref_index":94,"is_internal_anchor":false},{"citing_arxiv_id":"2508.13847","citing_title":"Discriminating scalar ultralight dark matter from quasi-monochromatic gravitational waves in LISA","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2507.17825","citing_title":"Ultralight dark matter detection with trapped-ion interferometry","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2601.00955","citing_title":"Is the Conventional Picture of Coherence Time Complete? Dark Matter Recoherence","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11071","citing_title":"Time-dependent signals of new physics at the LHC","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06777","citing_title":"Neutrino-Antineutrino Conversion from Ultralight Vector Dark Matter","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06843","citing_title":"Fast and accurate noise removal by curve fitting using orthogonal polynomials","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15241","citing_title":"Echoes of Global Cosmic Strings","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02172","citing_title":"Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2","ref_index":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI","json":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI.json","graph_json":"https://pith.science/api/pith-number/MLM6CSRSSIQNIRXHUKSV5OOCZI/graph.json","events_json":"https://pith.science/api/pith-number/MLM6CSRSSIQNIRXHUKSV5OOCZI/events.json","paper":"https://pith.science/paper/MLM6CSRS"},"agent_actions":{"view_html":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI","download_json":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI.json","view_paper":"https://pith.science/paper/MLM6CSRS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.10489&json=true","fetch_graph":"https://pith.science/api/pith-number/MLM6CSRSSIQNIRXHUKSV5OOCZI/graph.json","fetch_events":"https://pith.science/api/pith-number/MLM6CSRSSIQNIRXHUKSV5OOCZI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI/action/storage_attestation","attest_author":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI/action/author_attestation","sign_citation":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI/action/citation_signature","submit_replication":"https://pith.science/pith/MLM6CSRSSIQNIRXHUKSV5OOCZI/action/replication_record"}},"created_at":"2026-07-05T01:51:03.921321+00:00","updated_at":"2026-07-05T01:51:03.921321+00:00"}