{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:7KRYGOJFWVL7DQFXGF3J7CDDT7","short_pith_number":"pith:7KRYGOJF","schema_version":"1.0","canonical_sha256":"faa3833925b557f1c0b731769f88639fef9cff725695a17843d9a1d429798197","source":{"kind":"arxiv","id":"1612.03836","version":1},"attestation_state":"computed","paper":{"title":"Dark matter constraints from an observation of dSphs and the LMC with the Baikal NT200","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"A.A. Doroshenko, A.A. Sheifler, A.D. Avrorin, A.I. Panfilov, A.N. Dyachok, A.P. Koshechkin, A.R. Gafarov, A.V. Avrorin, A.V. Korobchenko, A.V. Kozhin, A.V. Skurihin, A.V. Zagorodnikov, B.A. Shaybonov, B.A. Tarashansky, D.A. Kuleshov, E.N. Pliskovsky, E.R. Osipova, E.V. Rjabov, F.K. Koshel, G.V. Domogatsky, I.A. Belolaptikov, I.A. Danilchenko, K.G. Kebkal, K.V. Golubkov, K.V. Konischev, L. Fajt, L.V. Pan'kov, M.B. Milenin, M.D. Shelepov, M.I. Rozanov, N.M. Budnev, O.G. Kebkal, O.N. Gaponenko, O.V. Suvorova, R.A. Mirgazov, R. Bannasch, R. Dvornicky, S.A. Yakovlev, S.V. Demidov, S.V. Fialkovsky, T.I. Gress, V.A. Tabolenko, V.B. Brudanin, V.F. Kulepov, V.L. Zurbanov, V.M. Aynutdinov, Zh.-A.M. Dzhilkibaev, Z. Honz","submitted_at":"2016-12-12T18:34:50Z","abstract_excerpt":"In present analysis we complete search for a dark matter signal with the Baikal neutrino telescope NT200 from potential sources in the sky. We use five years of data and look for neutrinos from dark matter annihilations in the dwarfs spheroidal galaxies in the Southern hemisphere and the Large Magellanic Cloud known as the largest and close satellite galaxy of the Milky Way. We do not find any excess in observed data over expected background from the atmospheric neutrinos towards the LMC or any of tested 22 dwarfs. We perform a joint likelihood analysis on the sample of five selected dwarfs an"},"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":"1612.03836","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-12-12T18:34:50Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"668a7708cc0bba02cc8c275c0215373674c1b1e65f91d5402aebff882bb20de3","abstract_canon_sha256":"d0a8406f0a4e463166c3678e54b267480ad902ed236d13ac5e863e0b476e4d29"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:35.160949Z","signature_b64":"SL/5xdo+styzPfuzAY4cE8b27+uFRm+n/03mpMBuA/CRJHVFbOL0U6cb5G0zEUrqdSg4aZMaV9CcU1LUnp7+Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"faa3833925b557f1c0b731769f88639fef9cff725695a17843d9a1d429798197","last_reissued_at":"2026-05-18T00:35:35.160427Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:35.160427Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark matter constraints from an observation of dSphs and the LMC with the Baikal NT200","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"A.A. Doroshenko, A.A. Sheifler, A.D. Avrorin, A.I. Panfilov, A.N. Dyachok, A.P. Koshechkin, A.R. Gafarov, A.V. Avrorin, A.V. Korobchenko, A.V. Kozhin, A.V. Skurihin, A.V. Zagorodnikov, B.A. Shaybonov, B.A. Tarashansky, D.A. Kuleshov, E.N. Pliskovsky, E.R. Osipova, E.V. Rjabov, F.K. Koshel, G.V. Domogatsky, I.A. Belolaptikov, I.A. Danilchenko, K.G. Kebkal, K.V. Golubkov, K.V. Konischev, L. Fajt, L.V. Pan'kov, M.B. Milenin, M.D. Shelepov, M.I. Rozanov, N.M. Budnev, O.G. Kebkal, O.N. Gaponenko, O.V. Suvorova, R.A. Mirgazov, R. Bannasch, R. Dvornicky, S.A. Yakovlev, S.V. Demidov, S.V. Fialkovsky, T.I. Gress, V.A. Tabolenko, V.B. Brudanin, V.F. Kulepov, V.L. Zurbanov, V.M. Aynutdinov, Zh.-A.M. Dzhilkibaev, Z. Honz","submitted_at":"2016-12-12T18:34:50Z","abstract_excerpt":"In present analysis we complete search for a dark matter signal with the Baikal neutrino telescope NT200 from potential sources in the sky. We use five years of data and look for neutrinos from dark matter annihilations in the dwarfs spheroidal galaxies in the Southern hemisphere and the Large Magellanic Cloud known as the largest and close satellite galaxy of the Milky Way. We do not find any excess in observed data over expected background from the atmospheric neutrinos towards the LMC or any of tested 22 dwarfs. We perform a joint likelihood analysis on the sample of five selected dwarfs an"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.03836","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1612.03836","created_at":"2026-05-18T00:35:35.160504+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.03836v1","created_at":"2026-05-18T00:35:35.160504+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.03836","created_at":"2026-05-18T00:35:35.160504+00:00"},{"alias_kind":"pith_short_12","alias_value":"7KRYGOJFWVL7","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"7KRYGOJFWVL7DQFX","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"7KRYGOJF","created_at":"2026-05-18T12:30:04.600751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7","json":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7.json","graph_json":"https://pith.science/api/pith-number/7KRYGOJFWVL7DQFXGF3J7CDDT7/graph.json","events_json":"https://pith.science/api/pith-number/7KRYGOJFWVL7DQFXGF3J7CDDT7/events.json","paper":"https://pith.science/paper/7KRYGOJF"},"agent_actions":{"view_html":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7","download_json":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7.json","view_paper":"https://pith.science/paper/7KRYGOJF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.03836&json=true","fetch_graph":"https://pith.science/api/pith-number/7KRYGOJFWVL7DQFXGF3J7CDDT7/graph.json","fetch_events":"https://pith.science/api/pith-number/7KRYGOJFWVL7DQFXGF3J7CDDT7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7/action/storage_attestation","attest_author":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7/action/author_attestation","sign_citation":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7/action/citation_signature","submit_replication":"https://pith.science/pith/7KRYGOJFWVL7DQFXGF3J7CDDT7/action/replication_record"}},"created_at":"2026-05-18T00:35:35.160504+00:00","updated_at":"2026-05-18T00:35:35.160504+00:00"}