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Here, I investigate the effect that a magnetar (initial rotational energy of 4x10^50erg and field strength of 7x10^13G) would have on the properties of a typical Type II SN ejecta (mass of 13.35Msun, kinetic energy of 1.32x10^51erg, 0.077Msun of 56Ni) produced by the terminal explosion of an H-rich blue-supergian"},"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":"1801.05340","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-01-14T20:44:52Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"bf3d24cb59589a44568f85cffa4d023fcd3c8b96feaf489c4a0149b5ea14b7a7","abstract_canon_sha256":"ae0e919abc30f711b8c1299420030ad17e29bfc33729af56399e297c0038cb4c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:21:20.600784Z","signature_b64":"rWKSopq5f2V1GvA6iDc/CR6Eqd4YxtkDqMHEEtt+KMEQ7bSL8pLFWUHNET+CJ3Cv7kmZlu1ZxZfyTeSPW84KBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"06e43952e5c350bca09c84988ebcbf8c6c095edbc96abc53a50273f7072806a6","last_reissued_at":"2026-05-18T00:21:20.600087Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:21:20.600087Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A magnetar model for the hydrogen-rich super-luminous supernova iPTF14hls","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"CNRS, Luc Dessart (UMI 3386 - LFCA, Universidad de Chile)","submitted_at":"2018-01-14T20:44:52Z","abstract_excerpt":"Transient surveys have recently revealed the existence of H-rich super-luminous supernovae (SLSN; e.g., iPTF14hls, OGLE-SN14-073) characterized by an exceptionally large time-integrated bolometric luminosity, a sustained blue optical color, and Doppler-broadened HI lines at all times. 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