In this paper, we study the energy dependent pulse profiles of the high mass X-ray binary pulsar 4U 0115+63 to investigate how they are affected by cyclotron resonant scattering.
We analyze archival BeppoSAX and RXTE observations performed during the giant outburst of the source which occurred i"},"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":"1106.4930","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2011-06-24T10:08:31Z","cross_cats_sorted":[],"title_canon_sha256":"31b7d5c187c93d946da62c7f37b2d20800bbf51317e1d833038acd24c0dfbe40","abstract_canon_sha256":"f08a086f87a012763563350a1c1cb64f85279f06d9ba54085ba0ea788672a7ca"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:31.158709Z","signature_b64":"wH8j33hnh25zNf302lqnkS0e+QSQrCtIdHjtV3vSNAAzzla8v3y1vONVc1A/9zHTpp7cuQapVbuk+H2oGS8MDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"141e21452a09286189c0eaf86a13a842a99a33a5c98e4bafd6c55201e05035fb","last_reissued_at":"2026-05-18T02:01:31.158155Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:31.158155Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"4U 0115+63: phase lags and cyclotron resonant scattering","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Santangelo, C. Ferrigno, D. Klochkov, E. Bozzo, M. Falanga, P. A. Becker","submitted_at":"2011-06-24T10:08:31Z","abstract_excerpt":"High mass X-ray binaries are among the brightest objects of our Galaxy in the high energy domain (0.1-100 keV). Despite our relatively good knowledge of their basic emission mechanisms, the complex problem of understanding their time and energy dependent X-ray emission is not completely solved.
In this paper, we study the energy dependent pulse profiles of the high mass X-ray binary pulsar 4U 0115+63 to investigate how they are affected by cyclotron resonant scattering.
We analyze archival BeppoSAX and RXTE observations performed during the giant outburst of the source which occurred i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.4930","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":"1106.4930","created_at":"2026-05-18T02:01:31.158230+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.4930v2","created_at":"2026-05-18T02:01:31.158230+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.4930","created_at":"2026-05-18T02:01:31.158230+00:00"},{"alias_kind":"pith_short_12","alias_value":"CQPCCRJKBEUG","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_16","alias_value":"CQPCCRJKBEUGDCOA","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_8","alias_value":"CQPCCRJK","created_at":"2026-05-18T12:26:26.731475+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/CQPCCRJKBEUGDCOA5L4GUE5IIK","json":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK.json","graph_json":"https://pith.science/api/pith-number/CQPCCRJKBEUGDCOA5L4GUE5IIK/graph.json","events_json":"https://pith.science/api/pith-number/CQPCCRJKBEUGDCOA5L4GUE5IIK/events.json","paper":"https://pith.science/paper/CQPCCRJK"},"agent_actions":{"view_html":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK","download_json":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK.json","view_paper":"https://pith.science/paper/CQPCCRJK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.4930&json=true","fetch_graph":"https://pith.science/api/pith-number/CQPCCRJKBEUGDCOA5L4GUE5IIK/graph.json","fetch_events":"https://pith.science/api/pith-number/CQPCCRJKBEUGDCOA5L4GUE5IIK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK/action/storage_attestation","attest_author":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK/action/author_attestation","sign_citation":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK/action/citation_signature","submit_replication":"https://pith.science/pith/CQPCCRJKBEUGDCOA5L4GUE5IIK/action/replication_record"}},"created_at":"2026-05-18T02:01:31.158230+00:00","updated_at":"2026-05-18T02:01:31.158230+00:00"}