{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:KTEDRIFH6B6XUS3SPSSGPPMTKP","short_pith_number":"pith:KTEDRIFH","schema_version":"1.0","canonical_sha256":"54c838a0a7f07d7a4b727ca467bd9353ed001020f546f29c11e56821f6917fdd","source":{"kind":"arxiv","id":"1106.2656","version":1},"attestation_state":"computed","paper":{"title":"Star Formation in a Stellar Mass Selected Sample of Galaxies to z=3 from the GOODS NICMOS Survey (GNS)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alice Mortlock, Amanda E. Bauer, Asa F. L. Bluck, Christopher J. Conselice, Fernando Buitrago, Pablo G. Perez-Gonzalez, Ruth Grutzbauch","submitted_at":"2011-06-14T09:51:52Z","abstract_excerpt":"We present a study of the star-forming properties of a stellar mass-selected sample of galaxies in the GOODS NICMOS Survey (GNS), based on deep Hubble Space Telescope imaging of the GOODS North and South fields. Using a stellar mass selected sample, combined with HST/ACS and Spitzer data to measure both UV and infrared derived star formation rates (SFR), we investigate the star forming properties of a complete sample of ~1300 galaxies down to log M*=9.5 at redshifts 1.5<z<3. Eight percent of the sample is made up of massive galaxies with M*>10^11 Msun. We derive optical colours, dust extinctio"},"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":"1106.2656","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-06-14T09:51:52Z","cross_cats_sorted":[],"title_canon_sha256":"f0d35859d1dd7b2855292a6e71a9ad85b18824790981ad76e08eb197efce9353","abstract_canon_sha256":"eef1d4caae72359097c136a6ae76ee1ff3d71fe13f743afac8bd3904830ee6ac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:37.562551Z","signature_b64":"Nwp4IHNDSI8L4EfmqmIcdfkGqQJimr1nkquIlFBNh+QKutV8IW++UaiEPT9yzP/lywJda7B4NSfE5wQEwpOEDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"54c838a0a7f07d7a4b727ca467bd9353ed001020f546f29c11e56821f6917fdd","last_reissued_at":"2026-05-18T02:01:37.561947Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:37.561947Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Star Formation in a Stellar Mass Selected Sample of Galaxies to z=3 from the GOODS NICMOS Survey (GNS)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alice Mortlock, Amanda E. Bauer, Asa F. L. Bluck, Christopher J. Conselice, Fernando Buitrago, Pablo G. Perez-Gonzalez, Ruth Grutzbauch","submitted_at":"2011-06-14T09:51:52Z","abstract_excerpt":"We present a study of the star-forming properties of a stellar mass-selected sample of galaxies in the GOODS NICMOS Survey (GNS), based on deep Hubble Space Telescope imaging of the GOODS North and South fields. Using a stellar mass selected sample, combined with HST/ACS and Spitzer data to measure both UV and infrared derived star formation rates (SFR), we investigate the star forming properties of a complete sample of ~1300 galaxies down to log M*=9.5 at redshifts 1.5<z<3. Eight percent of the sample is made up of massive galaxies with M*>10^11 Msun. We derive optical colours, dust extinctio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.2656","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1106.2656","created_at":"2026-05-18T02:01:37.562037+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.2656v1","created_at":"2026-05-18T02:01:37.562037+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.2656","created_at":"2026-05-18T02:01:37.562037+00:00"},{"alias_kind":"pith_short_12","alias_value":"KTEDRIFH6B6X","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_16","alias_value":"KTEDRIFH6B6XUS3S","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_8","alias_value":"KTEDRIFH","created_at":"2026-05-18T12:26:34.985390+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP","json":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP.json","graph_json":"https://pith.science/api/pith-number/KTEDRIFH6B6XUS3SPSSGPPMTKP/graph.json","events_json":"https://pith.science/api/pith-number/KTEDRIFH6B6XUS3SPSSGPPMTKP/events.json","paper":"https://pith.science/paper/KTEDRIFH"},"agent_actions":{"view_html":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP","download_json":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP.json","view_paper":"https://pith.science/paper/KTEDRIFH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.2656&json=true","fetch_graph":"https://pith.science/api/pith-number/KTEDRIFH6B6XUS3SPSSGPPMTKP/graph.json","fetch_events":"https://pith.science/api/pith-number/KTEDRIFH6B6XUS3SPSSGPPMTKP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP/action/storage_attestation","attest_author":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP/action/author_attestation","sign_citation":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP/action/citation_signature","submit_replication":"https://pith.science/pith/KTEDRIFH6B6XUS3SPSSGPPMTKP/action/replication_record"}},"created_at":"2026-05-18T02:01:37.562037+00:00","updated_at":"2026-05-18T02:01:37.562037+00:00"}