{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:AMWN56DQ7UDXYOZVGCMHBYHEHR","short_pith_number":"pith:AMWN56DQ","schema_version":"1.0","canonical_sha256":"032cdef870fd077c3b35309870e0e43c6d3abbb5c3500ef8f3bb5fe0bb4bcd5b","source":{"kind":"arxiv","id":"1607.01190","version":2},"attestation_state":"computed","paper":{"title":"Galaxy and Mass Assembly (GAMA): Exploring the WISE Cosmic Web in G12","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. M. Hopkins, B. W. Holwerda, C.C. Popescu, C. Magoulas, E.M. Sadler, E.N. Taylor, J.A. Peacock, J. Bland-Hawthorn, J. Loveday, L. Wang, M. Alpaslan, M. Bilicki, M.E. Cluver, M.J.I. Brown, P. Norberg, R.J. Tuffs, S. Brough, S. Croom, S. Driver, T.H. Jarrett","submitted_at":"2016-07-05T11:01:07Z","abstract_excerpt":"We present an analysis of the mid-infrared WISE sources seen within the equatorial GAMA G12 field, located in the North Galactic Cap. Our motivation is to study and characterize the behavior of WISE source populations in anticipation of the deep multi-wavelength surveys that will define the next decade, with the principal science goal of mapping the 3D large scale structures and determining the global physical attributes of the host galaxies. In combination with cosmological redshifts, we identify galaxies from their WISE W1 3.4um resolved emission, and by performing a star-galaxy separation u"},"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":"1607.01190","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-07-05T11:01:07Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"4dc6271baf348c109e8c23c9dac06acef44dc8130b527469f6c57f7129c1bab3","abstract_canon_sha256":"4a171d61ff6c72dca4e814e5400974aae4522ca7219db3125fb2cfbc7a3a4b30"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:19.796454Z","signature_b64":"5pZgTTJdpIaRLql0SPIEVHV5gVijFah9BtDWQKiVIPqsf092RhULHlPcrr/HdiQ/SVnkbpSRaLkhsHEnZYxqAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"032cdef870fd077c3b35309870e0e43c6d3abbb5c3500ef8f3bb5fe0bb4bcd5b","last_reissued_at":"2026-05-18T00:50:19.795744Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:19.795744Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galaxy and Mass Assembly (GAMA): Exploring the WISE Cosmic Web in G12","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. M. Hopkins, B. W. Holwerda, C.C. Popescu, C. Magoulas, E.M. Sadler, E.N. Taylor, J.A. Peacock, J. Bland-Hawthorn, J. Loveday, L. Wang, M. Alpaslan, M. Bilicki, M.E. Cluver, M.J.I. Brown, P. Norberg, R.J. Tuffs, S. Brough, S. Croom, S. Driver, T.H. Jarrett","submitted_at":"2016-07-05T11:01:07Z","abstract_excerpt":"We present an analysis of the mid-infrared WISE sources seen within the equatorial GAMA G12 field, located in the North Galactic Cap. Our motivation is to study and characterize the behavior of WISE source populations in anticipation of the deep multi-wavelength surveys that will define the next decade, with the principal science goal of mapping the 3D large scale structures and determining the global physical attributes of the host galaxies. In combination with cosmological redshifts, we identify galaxies from their WISE W1 3.4um resolved emission, and by performing a star-galaxy separation u"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.01190","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":""},"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":"1607.01190","created_at":"2026-05-18T00:50:19.795847+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.01190v2","created_at":"2026-05-18T00:50:19.795847+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.01190","created_at":"2026-05-18T00:50:19.795847+00:00"},{"alias_kind":"pith_short_12","alias_value":"AMWN56DQ7UDX","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"AMWN56DQ7UDXYOZV","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"AMWN56DQ","created_at":"2026-05-18T12:30:07.202191+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/AMWN56DQ7UDXYOZVGCMHBYHEHR","json":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR.json","graph_json":"https://pith.science/api/pith-number/AMWN56DQ7UDXYOZVGCMHBYHEHR/graph.json","events_json":"https://pith.science/api/pith-number/AMWN56DQ7UDXYOZVGCMHBYHEHR/events.json","paper":"https://pith.science/paper/AMWN56DQ"},"agent_actions":{"view_html":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR","download_json":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR.json","view_paper":"https://pith.science/paper/AMWN56DQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.01190&json=true","fetch_graph":"https://pith.science/api/pith-number/AMWN56DQ7UDXYOZVGCMHBYHEHR/graph.json","fetch_events":"https://pith.science/api/pith-number/AMWN56DQ7UDXYOZVGCMHBYHEHR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR/action/storage_attestation","attest_author":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR/action/author_attestation","sign_citation":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR/action/citation_signature","submit_replication":"https://pith.science/pith/AMWN56DQ7UDXYOZVGCMHBYHEHR/action/replication_record"}},"created_at":"2026-05-18T00:50:19.795847+00:00","updated_at":"2026-05-18T00:50:19.795847+00:00"}