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Using these observations we determined the rotational rates of the asteroids, with the exception of Nikulin and Renemichelsen. The distribution of rotational rates of 59 V-type asteroids in the inner main belt, including 29 members of the Vesta family that are regarded as ejecta from the asteroid (4) Ves"},"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":"1311.4653","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-11-19T08:44:47Z","cross_cats_sorted":[],"title_canon_sha256":"a7c5f1f7b04616d80489944ad02bdbaf36697787d4c4ecc3c23d37d94244aefd","abstract_canon_sha256":"dc5437617aa9e6bafcad371a703a00f484788e820714a29ccc21321530716ff0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:23.234351Z","signature_b64":"L4fhKcsYuYzrMgqPHpA6QatoONLToKRhLc29g91HayHLwnBSYB/c6edmfE0zXOtSF+VV+VlwYzcmIkC6wtk9Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0cddae3c4c7390aafb93adf7f11e7ac29ce6ae233aefee570b7cb41bb57c558","last_reissued_at":"2026-05-18T01:46:23.233878Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:23.233878Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Lightcurve Survey of V-type Asteroids in the Inner Asteroid Belt","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Akari Harada, Daisuke Kuroda, Hiroyuki Mito, Hiroyuki Toda, Kenshi Yanagisawa, Kouji Okita, Machiko Mori, Masanao Abe, Masateru Ishiguro, Michitoshi Yoshida, Nobuyuki Kawai, Seidai Miyasaka, Setsuko Nishihara, Shogo Nagayama, Sunao Hasegawa, Takumi Abe, Tomohiko Ozawa, Tomohiko Sekiguchi, Yasuhiro Shimizu, Yuki Sarugaku","submitted_at":"2013-11-19T08:44:47Z","abstract_excerpt":"We have observed the lightcurves of 13 V-type asteroids ((1933) Tinchen, (2011) Veteraniya, (2508) Alupka, (3657) Ermolova, (3900) Knezevic, (4005) Dyagilev, (4383) Suruga, (4434) Nikulin, (4796) Lewis, (6331) 1992 $\\mathrm{FZ_{1}}$, (8645) 1998 TN, (10285) Renemichelsen, and (10320) Reiland). 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