{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:5ITWZEOMTOPDJ36TQTGSUST7QJ","short_pith_number":"pith:5ITWZEOM","schema_version":"1.0","canonical_sha256":"ea276c91cc9b9e34efd384cd2a4a7f827a953caea1ad7a1f3896d313267b1ef9","source":{"kind":"arxiv","id":"2510.26889","version":2},"attestation_state":"computed","paper":{"title":"Galaxy Luminosity Function of the Coma Cluster from Deep $u'-g'-r'$ Wendelstein Imaging Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Arno Riffeser, Benjamin Seidel, Christoph Ries, Claus G\\\"ossl, Hanna Kellermann, Jan-Niklas Pippert, Luis Thomas, Matthias Kluge, Michael Schmidt, Ralf Bender, Raphael Z\\\"oller, Ulrich Hopp","submitted_at":"2025-10-30T18:00:22Z","abstract_excerpt":"We derive the $g'$ band galaxy luminosity function (GLF) of quenched resolved galaxies in the Coma cluster from a deep-imaging survey with $\\approx1.5\\,\\mathrm{deg^2}$ around the cluster center. The dataset comprises deep $u'$-, $g'$-, and $r'$-band data obtained with the Wendelstein Wide Field Imager on the $2.1\\,$m Fraunhofer Wendelstein Telescope reaching median $3\\sigma$ surface brightness limits in 10\" $\\times$ 10\" boxes of $\\mathrm{ (30.0\\,u',\\,\\,29.6\\,g',\\,\\,28.7\\,r')\\,mag\\,arcsec^{-2}}$. We measure structural parameters across a large dynamic range in galaxy brightness ($-24.5\\,g'\\,\\ma"},"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":"2510.26889","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-10-30T18:00:22Z","cross_cats_sorted":[],"title_canon_sha256":"d5432a48862060995818887828ec1a130eddc79f459a1f652ba979bde0a0e58e","abstract_canon_sha256":"65ce1a37ada0c3c32eb3ccabca48e94295206b1e54ecc4ef1ac81fe49786510b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-08T01:18:21.554796Z","signature_b64":"IyptBg2U6k5gMbQnmO55MT0hK6OiOxmsvElLBeSbE5WRuqMHJoUrMqfm+foEmFNAXRcT0MpGlCt2+tFoF2TvBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ea276c91cc9b9e34efd384cd2a4a7f827a953caea1ad7a1f3896d313267b1ef9","last_reissued_at":"2026-07-08T01:18:21.554145Z","signature_status":"signed_v1","first_computed_at":"2026-07-08T01:18:21.554145Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galaxy Luminosity Function of the Coma Cluster from Deep $u'-g'-r'$ Wendelstein Imaging Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Arno Riffeser, Benjamin Seidel, Christoph Ries, Claus G\\\"ossl, Hanna Kellermann, Jan-Niklas Pippert, Luis Thomas, Matthias Kluge, Michael Schmidt, Ralf Bender, Raphael Z\\\"oller, Ulrich Hopp","submitted_at":"2025-10-30T18:00:22Z","abstract_excerpt":"We derive the $g'$ band galaxy luminosity function (GLF) of quenched resolved galaxies in the Coma cluster from a deep-imaging survey with $\\approx1.5\\,\\mathrm{deg^2}$ around the cluster center. The dataset comprises deep $u'$-, $g'$-, and $r'$-band data obtained with the Wendelstein Wide Field Imager on the $2.1\\,$m Fraunhofer Wendelstein Telescope reaching median $3\\sigma$ surface brightness limits in 10\" $\\times$ 10\" boxes of $\\mathrm{ (30.0\\,u',\\,\\,29.6\\,g',\\,\\,28.7\\,r')\\,mag\\,arcsec^{-2}}$. We measure structural parameters across a large dynamic range in galaxy brightness ($-24.5\\,g'\\,\\ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2510.26889","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2510.26889/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2510.26889","created_at":"2026-07-08T01:18:21.554208+00:00"},{"alias_kind":"arxiv_version","alias_value":"2510.26889v2","created_at":"2026-07-08T01:18:21.554208+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2510.26889","created_at":"2026-07-08T01:18:21.554208+00:00"},{"alias_kind":"pith_short_12","alias_value":"5ITWZEOMTOPD","created_at":"2026-07-08T01:18:21.554208+00:00"},{"alias_kind":"pith_short_16","alias_value":"5ITWZEOMTOPDJ36T","created_at":"2026-07-08T01:18:21.554208+00:00"},{"alias_kind":"pith_short_8","alias_value":"5ITWZEOM","created_at":"2026-07-08T01:18:21.554208+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.26230","citing_title":"Cutting with precision -- Leveraging Collapse Volumes to generate the next generation of zoom-in initial conditions","ref_index":73,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ","json":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ.json","graph_json":"https://pith.science/api/pith-number/5ITWZEOMTOPDJ36TQTGSUST7QJ/graph.json","events_json":"https://pith.science/api/pith-number/5ITWZEOMTOPDJ36TQTGSUST7QJ/events.json","paper":"https://pith.science/paper/5ITWZEOM"},"agent_actions":{"view_html":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ","download_json":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ.json","view_paper":"https://pith.science/paper/5ITWZEOM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2510.26889&json=true","fetch_graph":"https://pith.science/api/pith-number/5ITWZEOMTOPDJ36TQTGSUST7QJ/graph.json","fetch_events":"https://pith.science/api/pith-number/5ITWZEOMTOPDJ36TQTGSUST7QJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ/action/storage_attestation","attest_author":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ/action/author_attestation","sign_citation":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ/action/citation_signature","submit_replication":"https://pith.science/pith/5ITWZEOMTOPDJ36TQTGSUST7QJ/action/replication_record"}},"created_at":"2026-07-08T01:18:21.554208+00:00","updated_at":"2026-07-08T01:18:21.554208+00:00"}