{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:IJQTH6A7AXISB7F34KXLQBTG7F","short_pith_number":"pith:IJQTH6A7","schema_version":"1.0","canonical_sha256":"426133f81f05d120fcbbe2aeb80666f9404358192cca0ad48acf07c9db1d69d0","source":{"kind":"arxiv","id":"1812.05130","version":1},"attestation_state":"computed","paper":{"title":"Identifications of Faint Chandra Sources in the Globular Cluster M3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Adrienne M. Cool, Craig O. Heinke, Haldan N. Cohn, Phyillis M. Lugger, Yue Zhao","submitted_at":"2018-12-12T19:21:32Z","abstract_excerpt":"We report a $30~\\mathrm{ks}$ $Chandra$ ACIS-S survey of the globular cluster M3. Sixteen X-ray sources were detected within the half-light radius ($2.3'$) with $L_X \\gtrsim 2.3 \\times 10^{31}~\\mathrm{erg~s^{-1}}$. We used $Hubble~Space~Telescope$ WFC3/UVIS and ACS/WFC images to find 10 plausible optical/UV counterparts. We fit the spectral energy distribution of the known cataclysmic variable 1E1339.8+2837 with a blue ($T_\\mathrm{eff} = 2.10^{+1.96}_{-0.58}\\times 10^4~\\mathrm{K}$, 90% conf.) spectral component from an accretion disc, plus a red component ($T_\\mathrm{eff} = 3.75_{-0.15}^{+1.05}"},"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":"1812.05130","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-12-12T19:21:32Z","cross_cats_sorted":[],"title_canon_sha256":"4e2a623f6e3daef0409b5bb252ee42c523716deccef5ec87ef0c31735f9dd051","abstract_canon_sha256":"7cef61d5e3abd6afdadd87111154fbc83d8a763e7ced89cb71b2b4aa5af30db5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:24.474889Z","signature_b64":"0Q6vGX2fBm7ibZNWHzLGugqhb405n9teAL/KiH2Wq4/DWLvqHs9XVv30kw0phlrufZ8Jr4leRBNN9X9zwa6nBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"426133f81f05d120fcbbe2aeb80666f9404358192cca0ad48acf07c9db1d69d0","last_reissued_at":"2026-05-17T23:58:24.474165Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:24.474165Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Identifications of Faint Chandra Sources in the Globular Cluster M3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Adrienne M. Cool, Craig O. Heinke, Haldan N. Cohn, Phyillis M. Lugger, Yue Zhao","submitted_at":"2018-12-12T19:21:32Z","abstract_excerpt":"We report a $30~\\mathrm{ks}$ $Chandra$ ACIS-S survey of the globular cluster M3. Sixteen X-ray sources were detected within the half-light radius ($2.3'$) with $L_X \\gtrsim 2.3 \\times 10^{31}~\\mathrm{erg~s^{-1}}$. We used $Hubble~Space~Telescope$ WFC3/UVIS and ACS/WFC images to find 10 plausible optical/UV counterparts. We fit the spectral energy distribution of the known cataclysmic variable 1E1339.8+2837 with a blue ($T_\\mathrm{eff} = 2.10^{+1.96}_{-0.58}\\times 10^4~\\mathrm{K}$, 90% conf.) spectral component from an accretion disc, plus a red component ($T_\\mathrm{eff} = 3.75_{-0.15}^{+1.05}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.05130","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":"1812.05130","created_at":"2026-05-17T23:58:24.474286+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.05130v1","created_at":"2026-05-17T23:58:24.474286+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.05130","created_at":"2026-05-17T23:58:24.474286+00:00"},{"alias_kind":"pith_short_12","alias_value":"IJQTH6A7AXIS","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_16","alias_value":"IJQTH6A7AXISB7F3","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_8","alias_value":"IJQTH6A7","created_at":"2026-05-18T12:32:31.084164+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/IJQTH6A7AXISB7F34KXLQBTG7F","json":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F.json","graph_json":"https://pith.science/api/pith-number/IJQTH6A7AXISB7F34KXLQBTG7F/graph.json","events_json":"https://pith.science/api/pith-number/IJQTH6A7AXISB7F34KXLQBTG7F/events.json","paper":"https://pith.science/paper/IJQTH6A7"},"agent_actions":{"view_html":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F","download_json":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F.json","view_paper":"https://pith.science/paper/IJQTH6A7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.05130&json=true","fetch_graph":"https://pith.science/api/pith-number/IJQTH6A7AXISB7F34KXLQBTG7F/graph.json","fetch_events":"https://pith.science/api/pith-number/IJQTH6A7AXISB7F34KXLQBTG7F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F/action/storage_attestation","attest_author":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F/action/author_attestation","sign_citation":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F/action/citation_signature","submit_replication":"https://pith.science/pith/IJQTH6A7AXISB7F34KXLQBTG7F/action/replication_record"}},"created_at":"2026-05-17T23:58:24.474286+00:00","updated_at":"2026-05-17T23:58:24.474286+00:00"}