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Despite intensive optical follow-up its subclass however remained undetermined.\n  We want to further classify V405 Peg and understand its role in the CV zoo via its long-term behaviour, spectral properties, energy distribution and accretion luminosity.\n  We perform a spectral and timing analysis of \\textit{XMM-Newton} X-ray and ultra-viol"},"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":"1312.0508","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-12-02T16:33:23Z","cross_cats_sorted":[],"title_canon_sha256":"03730ff004cca6ae36be5c7fdb30e5976f46d435bd3bb9df8de773a1483e8e8d","abstract_canon_sha256":"4ca62a0a00aadc377f9f8c9bf99e3600658dcd0fc240be064be93121b74a069a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:59.816265Z","signature_b64":"MnCtu65baBShkGDNuVkWF9OP3QxW6pN8QZNH1kFQW+k7ubCq6rf08kZxPzrB7qG4eGhYChvr0sOd+RKVjztsDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3dce40b971dd8cbd60f02d50f12502b5712c3f08f12ab427c4a195b9b5bbc2f6","last_reissued_at":"2026-05-18T01:45:59.815757Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:59.815757Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"XMM-Newton observations of the low-luminosity cataclysmic variable V405 Pegasi","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A.D. 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