{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2023:5JCO6RCVFRPEJY5ALBMJNGMVWO","short_pith_number":"pith:5JCO6RCV","canonical_record":{"source":{"id":"2312.17459","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-29T03:52:22Z","cross_cats_sorted":[],"title_canon_sha256":"14b7d0109d4425d3961beb000349a410b59b83f74cc1f4e3a4ec60738f9c72da","abstract_canon_sha256":"937ab8ccb46a65db6a5f2c01904d1363e1c7289eaf740e4eaac8f04d191723e4"},"schema_version":"1.0"},"canonical_sha256":"ea44ef44552c5e44e3a05858969995b3ba21282b1ab7b8c794c9d66a9b5da321","source":{"kind":"arxiv","id":"2312.17459","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2312.17459","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"arxiv_version","alias_value":"2312.17459v2","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.17459","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"pith_short_12","alias_value":"5JCO6RCVFRPE","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"pith_short_16","alias_value":"5JCO6RCVFRPEJY5A","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"pith_short_8","alias_value":"5JCO6RCV","created_at":"2026-07-05T08:35:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2023:5JCO6RCVFRPEJY5ALBMJNGMVWO","target":"record","payload":{"canonical_record":{"source":{"id":"2312.17459","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-29T03:52:22Z","cross_cats_sorted":[],"title_canon_sha256":"14b7d0109d4425d3961beb000349a410b59b83f74cc1f4e3a4ec60738f9c72da","abstract_canon_sha256":"937ab8ccb46a65db6a5f2c01904d1363e1c7289eaf740e4eaac8f04d191723e4"},"schema_version":"1.0"},"canonical_sha256":"ea44ef44552c5e44e3a05858969995b3ba21282b1ab7b8c794c9d66a9b5da321","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:35:18.900992Z","signature_b64":"NK7W2f8a7BgRrSyy/y2hILmcFH3Ww/5V1wgpgLUYnuiIIw1+pfdIgQ4govP6pK+iKpjlIROn/6nckAZJbKXMAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ea44ef44552c5e44e3a05858969995b3ba21282b1ab7b8c794c9d66a9b5da321","last_reissued_at":"2026-07-05T08:35:18.900469Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:35:18.900469Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2312.17459","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-05T08:35:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"W9OTEudfn39h1oY/Uor1kRG95P/gHLb9+CX1f82jSqy4lw+J5zTNM7e+mfmijBAlH4yaneIuyqz7NpBhJqBODA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-21T11:08:20.332758Z"},"content_sha256":"a99ea3059218160bcb2669bdcbf7b9be107dc356f97a77901483a0d85c779339","schema_version":"1.0","event_id":"sha256:a99ea3059218160bcb2669bdcbf7b9be107dc356f97a77901483a0d85c779339"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2023:5JCO6RCVFRPEJY5ALBMJNGMVWO","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Measuring the conditional luminosity and stellar mass functions of galaxies by combining the DESI LS DR9, SV3 and Y1 data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron Meisner, Andrew Lambert, Antonios Katsianis, Axel de la Macorra, Benjamin Alan Weaver, Biprateep Dey, ChangHoon Hahn, Claire Poppett, David Brooks, Eusebio Sanchez, Graziano Rossi, Gregory Tarl\\'e, Haojie Xu, Hu Zou, Jaime E. Forero-Romero, Jessica Nicole Aguilar, Jiaqi Wang, Jiaxin Han, Johannes Ulf Lange, John Moustakas, Jundan Nie, Klaus Honscheid, Marc Manera, Mehdi Rezaie, Michael Schubnell, Min He, Peter Behroozi, Peter Doel, Qingyang Li, Ramon Miquel, Robert Kehoe, Shaun Cole, Steven Ahlen, Theodore Kisner, Todd Claybaugh, Wensheng Hong, Xiaohu Yang, Xiaoju Xu, Yaru Wang, Yirong Wang, Yizhou Gu, Yunliang Zheng, Yuyu Wang, Zhenlin Tan, Zhimin Zhou","submitted_at":"2023-12-29T03:52:22Z","abstract_excerpt":"In this investigation, we leverage the combination of Dark Energy Spectroscopic Instrument Legacy imaging Surveys Data Release 9 (DESI LS DR9), Survey Validation 3 (SV3), and Year 1 (Y1) data sets to estimate the conditional luminosity and stellar mass functions (CLFs & CSMFs) of galaxies across various halo mass bins and redshift ranges. To support our analysis, we utilize a realistic DESI Mock Galaxy Redshift Survey (MGRS) generated from a high-resolution Jiutian simulation. An extended halo-based group finder is applied to both MGRS catalogs and DESI observation. By comparing the r and z-ba"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.17459","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/2312.17459/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-05T08:35:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"6BgN84OtRmbnJ3/vKOY3dLc9xtIAcVDxUmCQsusAiR1xHxBFw9GZ1BayhGnCUWT+zovIBuDxq+1QkS6B62teCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-21T11:08:20.333319Z"},"content_sha256":"4743db58c5a6f9738e7e66702043bb3e46f0bca7c7e31378992d88982fe793c8","schema_version":"1.0","event_id":"sha256:4743db58c5a6f9738e7e66702043bb3e46f0bca7c7e31378992d88982fe793c8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/5JCO6RCVFRPEJY5ALBMJNGMVWO/bundle.json","state_url":"https://pith.science/pith/5JCO6RCVFRPEJY5ALBMJNGMVWO/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/5JCO6RCVFRPEJY5ALBMJNGMVWO/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-21T11:08:20Z","links":{"resolver":"https://pith.science/pith/5JCO6RCVFRPEJY5ALBMJNGMVWO","bundle":"https://pith.science/pith/5JCO6RCVFRPEJY5ALBMJNGMVWO/bundle.json","state":"https://pith.science/pith/5JCO6RCVFRPEJY5ALBMJNGMVWO/state.json","well_known_bundle":"https://pith.science/.well-known/pith/5JCO6RCVFRPEJY5ALBMJNGMVWO/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2023:5JCO6RCVFRPEJY5ALBMJNGMVWO","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"937ab8ccb46a65db6a5f2c01904d1363e1c7289eaf740e4eaac8f04d191723e4","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-29T03:52:22Z","title_canon_sha256":"14b7d0109d4425d3961beb000349a410b59b83f74cc1f4e3a4ec60738f9c72da"},"schema_version":"1.0","source":{"id":"2312.17459","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2312.17459","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"arxiv_version","alias_value":"2312.17459v2","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.17459","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"pith_short_12","alias_value":"5JCO6RCVFRPE","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"pith_short_16","alias_value":"5JCO6RCVFRPEJY5A","created_at":"2026-07-05T08:35:18Z"},{"alias_kind":"pith_short_8","alias_value":"5JCO6RCV","created_at":"2026-07-05T08:35:18Z"}],"graph_snapshots":[{"event_id":"sha256:4743db58c5a6f9738e7e66702043bb3e46f0bca7c7e31378992d88982fe793c8","target":"graph","created_at":"2026-07-05T08:35:18Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/2312.17459/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"In this investigation, we leverage the combination of Dark Energy Spectroscopic Instrument Legacy imaging Surveys Data Release 9 (DESI LS DR9), Survey Validation 3 (SV3), and Year 1 (Y1) data sets to estimate the conditional luminosity and stellar mass functions (CLFs & CSMFs) of galaxies across various halo mass bins and redshift ranges. To support our analysis, we utilize a realistic DESI Mock Galaxy Redshift Survey (MGRS) generated from a high-resolution Jiutian simulation. An extended halo-based group finder is applied to both MGRS catalogs and DESI observation. By comparing the r and z-ba","authors_text":"Aaron Meisner, Andrew Lambert, Antonios Katsianis, Axel de la Macorra, Benjamin Alan Weaver, Biprateep Dey, ChangHoon Hahn, Claire Poppett, David Brooks, Eusebio Sanchez, Graziano Rossi, Gregory Tarl\\'e, Haojie Xu, Hu Zou, Jaime E. Forero-Romero, Jessica Nicole Aguilar, Jiaqi Wang, Jiaxin Han, Johannes Ulf Lange, John Moustakas, Jundan Nie, Klaus Honscheid, Marc Manera, Mehdi Rezaie, Michael Schubnell, Min He, Peter Behroozi, Peter Doel, Qingyang Li, Ramon Miquel, Robert Kehoe, Shaun Cole, Steven Ahlen, Theodore Kisner, Todd Claybaugh, Wensheng Hong, Xiaohu Yang, Xiaoju Xu, Yaru Wang, Yirong Wang, Yizhou Gu, Yunliang Zheng, Yuyu Wang, Zhenlin Tan, Zhimin Zhou","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-29T03:52:22Z","title":"Measuring the conditional luminosity and stellar mass functions of galaxies by combining the DESI LS DR9, SV3 and Y1 data"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.17459","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:a99ea3059218160bcb2669bdcbf7b9be107dc356f97a77901483a0d85c779339","target":"record","created_at":"2026-07-05T08:35:18Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"937ab8ccb46a65db6a5f2c01904d1363e1c7289eaf740e4eaac8f04d191723e4","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-29T03:52:22Z","title_canon_sha256":"14b7d0109d4425d3961beb000349a410b59b83f74cc1f4e3a4ec60738f9c72da"},"schema_version":"1.0","source":{"id":"2312.17459","kind":"arxiv","version":2}},"canonical_sha256":"ea44ef44552c5e44e3a05858969995b3ba21282b1ab7b8c794c9d66a9b5da321","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"ea44ef44552c5e44e3a05858969995b3ba21282b1ab7b8c794c9d66a9b5da321","first_computed_at":"2026-07-05T08:35:18.900469Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-05T08:35:18.900469Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"NK7W2f8a7BgRrSyy/y2hILmcFH3Ww/5V1wgpgLUYnuiIIw1+pfdIgQ4govP6pK+iKpjlIROn/6nckAZJbKXMAw==","signature_status":"signed_v1","signed_at":"2026-07-05T08:35:18.900992Z","signed_message":"canonical_sha256_bytes"},"source_id":"2312.17459","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:a99ea3059218160bcb2669bdcbf7b9be107dc356f97a77901483a0d85c779339","sha256:4743db58c5a6f9738e7e66702043bb3e46f0bca7c7e31378992d88982fe793c8"],"state_sha256":"85bf809d95d80a87d2ccf48f54c4b6df9c559bc41434af1c9d15595eaf5f8f20"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"WXMTAQtwhzDadYdJTS+rAvgvzB/ksqryzE+v7M3Cp6wLs2BHcjpREDZtsOrFwD4vkimUP3BX53vTxTdJVue2Ag==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-21T11:08:20.337493Z","bundle_sha256":"ee6776379735e57aec35b0066f8ec45d914d3e248fd82bd722e571964dda370b"}}