{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:LXVZTFESKKM4WDUHG274IR7PVA","short_pith_number":"pith:LXVZTFES","schema_version":"1.0","canonical_sha256":"5deb9994925299cb0e8736bfc447efa83c7130e0bdd38a6c8d9d67ffc39f2f68","source":{"kind":"arxiv","id":"1301.5514","version":2},"attestation_state":"computed","paper":{"title":"White Paper on GEMS Study of Polarized X-rays from Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alice Harding, Craig Markwardt, Dong Lai, Henric Krawczynski, Herman Marshall, Jean Swank, Jeffrey Martoff, Jeffrey Scargle, Jeremy Schnittman, Jessie Dotson, Joanne Hill, Julian Krolik, Juri Poutanen, Keith Jahoda, Kevin Black, Lorella Angelini, Matthew Baring, Peter Serlemitsos, Phillip Kaaret, Pranab Ghosh, Robert Petre, Robin Morris, Stephen Reynolds, Takashi Okajima, Tim Kallman, Tod Strohmayer, Toru Tamagawa, Wayne Baumgartner, Yang Soong, Y. Tawara","submitted_at":"2013-01-23T14:35:29Z","abstract_excerpt":"We examine the expected X-ray polarization properties of neutron-star X-ray sources of various types, e.g., accretion and rotation powered pulsars, magnetars, and low-mass X-ray binaries. We summarize the model calculations leading to these expected properties. We describe how a comparison of these with their observed properties, as inferred from GEMS data, will probe the essential dynamical, electromagnetic, plasma, and emission processes in neutron-star binaries, discriminate between models of these processes, and constrain model parameters. An exciting goal is the first observational demons"},"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":"1301.5514","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-23T14:35:29Z","cross_cats_sorted":[],"title_canon_sha256":"64336f92c8460151ac88a95137e7a8a8b99c1184652ee54fcd4a6da71637b585","abstract_canon_sha256":"9269cc7de539c1c62ae3bef1f424c55fca7e67800456efe64c1d9d2e86a517a8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:34:13.593762Z","signature_b64":"HANH/iTrOj/Y0LAqQ47h7LzYdXYlGqkRGD797u8dDo3+mUGJq3u7LDm9KyHx/H38d8xScMtCpzBmtnNw16U7Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5deb9994925299cb0e8736bfc447efa83c7130e0bdd38a6c8d9d67ffc39f2f68","last_reissued_at":"2026-05-18T03:34:13.593029Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:34:13.593029Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"White Paper on GEMS Study of Polarized X-rays from Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alice Harding, Craig Markwardt, Dong Lai, Henric Krawczynski, Herman Marshall, Jean Swank, Jeffrey Martoff, Jeffrey Scargle, Jeremy Schnittman, Jessie Dotson, Joanne Hill, Julian Krolik, Juri Poutanen, Keith Jahoda, Kevin Black, Lorella Angelini, Matthew Baring, Peter Serlemitsos, Phillip Kaaret, Pranab Ghosh, Robert Petre, Robin Morris, Stephen Reynolds, Takashi Okajima, Tim Kallman, Tod Strohmayer, Toru Tamagawa, Wayne Baumgartner, Yang Soong, Y. Tawara","submitted_at":"2013-01-23T14:35:29Z","abstract_excerpt":"We examine the expected X-ray polarization properties of neutron-star X-ray sources of various types, e.g., accretion and rotation powered pulsars, magnetars, and low-mass X-ray binaries. We summarize the model calculations leading to these expected properties. We describe how a comparison of these with their observed properties, as inferred from GEMS data, will probe the essential dynamical, electromagnetic, plasma, and emission processes in neutron-star binaries, discriminate between models of these processes, and constrain model parameters. An exciting goal is the first observational demons"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.5514","kind":"arxiv","version":2},"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":"1301.5514","created_at":"2026-05-18T03:34:13.593156+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.5514v2","created_at":"2026-05-18T03:34:13.593156+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.5514","created_at":"2026-05-18T03:34:13.593156+00:00"},{"alias_kind":"pith_short_12","alias_value":"LXVZTFESKKM4","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"LXVZTFESKKM4WDUH","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"LXVZTFES","created_at":"2026-05-18T12:27:51.066281+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/LXVZTFESKKM4WDUHG274IR7PVA","json":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA.json","graph_json":"https://pith.science/api/pith-number/LXVZTFESKKM4WDUHG274IR7PVA/graph.json","events_json":"https://pith.science/api/pith-number/LXVZTFESKKM4WDUHG274IR7PVA/events.json","paper":"https://pith.science/paper/LXVZTFES"},"agent_actions":{"view_html":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA","download_json":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA.json","view_paper":"https://pith.science/paper/LXVZTFES","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.5514&json=true","fetch_graph":"https://pith.science/api/pith-number/LXVZTFESKKM4WDUHG274IR7PVA/graph.json","fetch_events":"https://pith.science/api/pith-number/LXVZTFESKKM4WDUHG274IR7PVA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA/action/storage_attestation","attest_author":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA/action/author_attestation","sign_citation":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA/action/citation_signature","submit_replication":"https://pith.science/pith/LXVZTFESKKM4WDUHG274IR7PVA/action/replication_record"}},"created_at":"2026-05-18T03:34:13.593156+00:00","updated_at":"2026-05-18T03:34:13.593156+00:00"}