{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:OXUCPOLJ4LFXH3N3VY42YBETIP","short_pith_number":"pith:OXUCPOLJ","schema_version":"1.0","canonical_sha256":"75e827b969e2cb73edbbae39ac049343ef8b5250caf69deac4a45b32a3c8f8fe","source":{"kind":"arxiv","id":"1407.7555","version":1},"attestation_state":"computed","paper":{"title":"Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron S. G. Robotham, Alister W. Graham, Amanda E. Bauer, Andrew M. Hopkins, \\'Angel R. L\\'opez-S\\'anchez, Anne E. Sansom, Benne W. Holwerda, Christopher J. Conselice, Cristina C. Popescu, Edward N. Taylor, Ivan Baldry, Jochen Liske, Jon Loveday, Joss Bland-Hawthorn, Lee S. Kelvin, Maritza A. Lara-L\\'opez, Matthew Colless, Matthew Prescott, Mehmet Alpaslan, Michael J. I. Brown, Peder Norberg, Richard J. Tuffs, Simon P. Driver, Steven P. Bamford, Steven Phillipps","submitted_at":"2014-07-28T20:20:20Z","abstract_excerpt":"We present an estimate of the galaxy stellar mass function and its division by morphological type in the local (0.025 < z < 0.06) Universe. Adopting robust morphological classifications as previously presented (Kelvin et al.) for a sample of 3,727 galaxies taken from the Galaxy And Mass Assembly survey, we define a local volume and stellar mass limited sub-sample of 2,711 galaxies to a lower stellar mass limit of M = 10^9.0 M_sun. We confirm that the galaxy stellar mass function is well described by a double Schechter function given by M* = 10^10.64 M_sun, {\\alpha}1 = -0.43, {\\phi}*1 = 4.18 de"},"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":"1407.7555","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-28T20:20:20Z","cross_cats_sorted":[],"title_canon_sha256":"7f783e5431ca61f4b92b34ef3c8cfed8990a1dedfc8d6c5ae88d16a7391e794f","abstract_canon_sha256":"84aa773a2229fcd090917b098655fb40d4c3a66a52fb554bc2248954e9704f41"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:29.103401Z","signature_b64":"/Bv0fG5N33bfQFv+23zWWXGERagI0BEgzeFKuZVZCwjQEhKhQvfVyn4sj4iKIAkM16Vl0cvotPHx/oRSoeU+Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"75e827b969e2cb73edbbae39ac049343ef8b5250caf69deac4a45b32a3c8f8fe","last_reissued_at":"2026-05-18T01:42:29.102828Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:29.102828Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron S. G. Robotham, Alister W. Graham, Amanda E. Bauer, Andrew M. Hopkins, \\'Angel R. L\\'opez-S\\'anchez, Anne E. Sansom, Benne W. Holwerda, Christopher J. Conselice, Cristina C. Popescu, Edward N. Taylor, Ivan Baldry, Jochen Liske, Jon Loveday, Joss Bland-Hawthorn, Lee S. Kelvin, Maritza A. Lara-L\\'opez, Matthew Colless, Matthew Prescott, Mehmet Alpaslan, Michael J. I. Brown, Peder Norberg, Richard J. Tuffs, Simon P. Driver, Steven P. Bamford, Steven Phillipps","submitted_at":"2014-07-28T20:20:20Z","abstract_excerpt":"We present an estimate of the galaxy stellar mass function and its division by morphological type in the local (0.025 < z < 0.06) Universe. Adopting robust morphological classifications as previously presented (Kelvin et al.) for a sample of 3,727 galaxies taken from the Galaxy And Mass Assembly survey, we define a local volume and stellar mass limited sub-sample of 2,711 galaxies to a lower stellar mass limit of M = 10^9.0 M_sun. We confirm that the galaxy stellar mass function is well described by a double Schechter function given by M* = 10^10.64 M_sun, {\\alpha}1 = -0.43, {\\phi}*1 = 4.18 de"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.7555","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":"1407.7555","created_at":"2026-05-18T01:42:29.102906+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.7555v1","created_at":"2026-05-18T01:42:29.102906+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.7555","created_at":"2026-05-18T01:42:29.102906+00:00"},{"alias_kind":"pith_short_12","alias_value":"OXUCPOLJ4LFX","created_at":"2026-05-18T12:28:43.426989+00:00"},{"alias_kind":"pith_short_16","alias_value":"OXUCPOLJ4LFXH3N3","created_at":"2026-05-18T12:28:43.426989+00:00"},{"alias_kind":"pith_short_8","alias_value":"OXUCPOLJ","created_at":"2026-05-18T12:28:43.426989+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/OXUCPOLJ4LFXH3N3VY42YBETIP","json":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP.json","graph_json":"https://pith.science/api/pith-number/OXUCPOLJ4LFXH3N3VY42YBETIP/graph.json","events_json":"https://pith.science/api/pith-number/OXUCPOLJ4LFXH3N3VY42YBETIP/events.json","paper":"https://pith.science/paper/OXUCPOLJ"},"agent_actions":{"view_html":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP","download_json":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP.json","view_paper":"https://pith.science/paper/OXUCPOLJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.7555&json=true","fetch_graph":"https://pith.science/api/pith-number/OXUCPOLJ4LFXH3N3VY42YBETIP/graph.json","fetch_events":"https://pith.science/api/pith-number/OXUCPOLJ4LFXH3N3VY42YBETIP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP/action/storage_attestation","attest_author":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP/action/author_attestation","sign_citation":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP/action/citation_signature","submit_replication":"https://pith.science/pith/OXUCPOLJ4LFXH3N3VY42YBETIP/action/replication_record"}},"created_at":"2026-05-18T01:42:29.102906+00:00","updated_at":"2026-05-18T01:42:29.102906+00:00"}