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Accreting ultracompact binaries contain a white dwarf that is accreting from a degenerate object and have orbital periods shorter than 65 minutes.\n  Aims. The aims of this letter are to report the discovery and the orbital period of four new eclipsing accreting ultracompact binaries found using the Zwicky Transient Facility, and to discuss their photometric properties.\n  Methods. We searched through a list of 4171 dwarf novae compiled using the Zwicky Transient Facility and used the Box Least Square method to search for periodic signals in the data.\n  Results. We found four new eclips"},"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":"2312.09980","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2023-12-15T17:46:01Z","cross_cats_sorted":[],"title_canon_sha256":"798cb7d9caeef26ec715bb359bec4ed8be68161c1ee19be6baf368c2c39c4df9","abstract_canon_sha256":"02ad56f4442c9c40503f8b5fee765f1acdfc8f2c913964feb6ef73b213a6d7b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:55:13.936833Z","signature_b64":"sg7BhBQd5f6aApYhTjiRGlg6jEn7rwFvbYHr3+eMZ7UUfKjdhVtq3P3GrW5YUhynXsrt0aP/fbkpyhnjAeBzBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"01d57cbf3adb23354c21fc216a6d1375f3bf642776367faaf9fecdcd97c93748","last_reissued_at":"2026-07-05T07:55:13.936396Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:55:13.936396Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. A. Mahabal, A. J. Drake, E. C. Bellm, J. M. Khalil, J. S. Bloom, J. van Roestel, M. J. Graham, R. Dekany, R. Riddle, R. R. Laher, S. L. Groom, S. R. Kulkarni, T. Prince","submitted_at":"2023-12-15T17:46:01Z","abstract_excerpt":"Context. Accreting ultracompact binaries contain a white dwarf that is accreting from a degenerate object and have orbital periods shorter than 65 minutes.\n  Aims. The aims of this letter are to report the discovery and the orbital period of four new eclipsing accreting ultracompact binaries found using the Zwicky Transient Facility, and to discuss their photometric properties.\n  Methods. We searched through a list of 4171 dwarf novae compiled using the Zwicky Transient Facility and used the Box Least Square method to search for periodic signals in the data.\n  Results. 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