{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:KDLX2SDQGRH23QCHDXWMTM5IUY","short_pith_number":"pith:KDLX2SDQ","schema_version":"1.0","canonical_sha256":"50d77d4870344fadc0471decc9b3a8a63d0a11c0317b3e7b6a46bc8d6dfafc88","source":{"kind":"arxiv","id":"1505.07829","version":3},"attestation_state":"computed","paper":{"title":"The role of the eROSITA all-sky survey in searches for sterile neutrino dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Christoph Weniger, Fabio Zandanel, Shin'ichiro Ando","submitted_at":"2015-05-28T20:00:29Z","abstract_excerpt":"We investigate for the first time the potential of angular auto- and cross-correlation power spectra in identifying sterile neutrino dark matter in the cosmic X-ray background. We take as reference the performance of the soon-to-be-launched eROSITA satellite. The main astrophysical background sources against sterile neutrino decays are active galactic nuclei, galaxies powered by X-ray binaries, and clusters of galaxies. While sterile neutrino decays are always subdominant in the auto-correlation power spectra, they can be efficiently enhanced when cross-correlating with tracers of the dark mat"},"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":"1505.07829","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-05-28T20:00:29Z","cross_cats_sorted":["astro-ph.HE","hep-ph"],"title_canon_sha256":"840bfda799916a7a9f69491487316bb568cb0a655038290fcde6986953085956","abstract_canon_sha256":"544f9f230ddca56d656ef5210b385d4f42e9d1f59c5dac11e5949cc3eeae9800"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:31:29.814384Z","signature_b64":"a7eLOgIFyzNOXpalXtC+BPl4Qg0R0sm6JF3iF1zxpfZ7HzPDlYxKw9cMPf0i1o8oJT5b7o1Czyb7UI+eDr7jCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"50d77d4870344fadc0471decc9b3a8a63d0a11c0317b3e7b6a46bc8d6dfafc88","last_reissued_at":"2026-05-18T01:31:29.813902Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:31:29.813902Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The role of the eROSITA all-sky survey in searches for sterile neutrino dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Christoph Weniger, Fabio Zandanel, Shin'ichiro Ando","submitted_at":"2015-05-28T20:00:29Z","abstract_excerpt":"We investigate for the first time the potential of angular auto- and cross-correlation power spectra in identifying sterile neutrino dark matter in the cosmic X-ray background. We take as reference the performance of the soon-to-be-launched eROSITA satellite. The main astrophysical background sources against sterile neutrino decays are active galactic nuclei, galaxies powered by X-ray binaries, and clusters of galaxies. While sterile neutrino decays are always subdominant in the auto-correlation power spectra, they can be efficiently enhanced when cross-correlating with tracers of the dark mat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.07829","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1505.07829","created_at":"2026-05-18T01:31:29.813970+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.07829v3","created_at":"2026-05-18T01:31:29.813970+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.07829","created_at":"2026-05-18T01:31:29.813970+00:00"},{"alias_kind":"pith_short_12","alias_value":"KDLX2SDQGRH2","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"KDLX2SDQGRH23QCH","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"KDLX2SDQ","created_at":"2026-05-18T12:29:27.538025+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.00648","citing_title":"Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter","ref_index":15,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY","json":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY.json","graph_json":"https://pith.science/api/pith-number/KDLX2SDQGRH23QCHDXWMTM5IUY/graph.json","events_json":"https://pith.science/api/pith-number/KDLX2SDQGRH23QCHDXWMTM5IUY/events.json","paper":"https://pith.science/paper/KDLX2SDQ"},"agent_actions":{"view_html":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY","download_json":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY.json","view_paper":"https://pith.science/paper/KDLX2SDQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.07829&json=true","fetch_graph":"https://pith.science/api/pith-number/KDLX2SDQGRH23QCHDXWMTM5IUY/graph.json","fetch_events":"https://pith.science/api/pith-number/KDLX2SDQGRH23QCHDXWMTM5IUY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY/action/storage_attestation","attest_author":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY/action/author_attestation","sign_citation":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY/action/citation_signature","submit_replication":"https://pith.science/pith/KDLX2SDQGRH23QCHDXWMTM5IUY/action/replication_record"}},"created_at":"2026-05-18T01:31:29.813970+00:00","updated_at":"2026-05-18T01:31:29.813970+00:00"}