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After removing the flux from the surrounding supernova remnant CTB~37B, the radiation of CXOU J171405.7-381031 is best described by a two-component model, consisting of a blackbody and power law. We obtain a blackbody temperature of 0.58^{+0.03}_{-0.03} keV, photon index of 2.15^{+0.62}_{-0.68}, and unabsorbed 2-10 keV flux of 2.33^{+0.02}_{-0.02} x 10^{-12} erg cm^{-2} s^{-1}. These new parameters enable us to compare CXOU 171405.7-381031 with other magnetars"},"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":"1905.11561","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-05-28T01:21:26Z","cross_cats_sorted":[],"title_canon_sha256":"ebef7678d4730cbf6289dc4edc3147091f027a631626bb00e6c23ab78d1bd2eb","abstract_canon_sha256":"9479e5d181748fcc8e71b83683cd410d74fc0e8464775ecbc805a2623d5c8121"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:40:31.706247Z","signature_b64":"30UiBYQMizeNU3+Q7De4hyyz65n/xAdf3h33MtamHo+SPKoqdbS8SyO0QjK6q7d5ExGvAw3MkVkJp0YSZXv/DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"70fb06b6c432488fda63f9ca53e8c3e43360c2ddc7b7b81a8abe9aa93db5babd","last_reissued_at":"2026-05-17T23:40:31.705719Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:40:31.705719Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"XMM-Newton Spectrum of the magnetar CXOU J171405.7-381031","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Aya Bamba, Eri Watanabe, Haruka Watanabe, Shinpei Shibata","submitted_at":"2019-05-28T01:21:26Z","abstract_excerpt":"We observe the magnetar CXOU J171405.7-381031 with XMM-Newton and obtain the most reliable X-ray spectral parameters for this magnetar. 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