{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:YYJ5HDJATUINI6FDJLYI77KQZ2","short_pith_number":"pith:YYJ5HDJA","schema_version":"1.0","canonical_sha256":"c613d38d209d10d478a34af08ffd50ce9896937ae6e299faaea366ba26adf947","source":{"kind":"arxiv","id":"astro-ph/0405537","version":1},"attestation_state":"computed","paper":{"title":"The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Uomoto, C. A. Tremonti, D. J. Schlegel, E. W. Peng, G. Kauffmann, J. Brinchmann, J. Brinkmann, M. Fukugita, M. Seibert, S. Charlot, S. D. M. White, T. M. Heckman","submitted_at":"2004-05-27T04:02:02Z","abstract_excerpt":"We utilize Sloan Digital Sky Survey imaging and spectroscopy of ~53,000 star-forming galaxies at z~0.1 to study the relation between stellar mass and gas-phase metallicity. We derive gas-phase oxygen abundances and stellar masses using new techniques which make use of the latest stellar evolutionary synthesis and photoionization models. We find a tight (+/-0.1 dex) correlation between stellar mass and metallicity spanning over 3 orders of magnitude in stellar mass and a factor of 10 in metallicity. The relation is relatively steep from 10^{8.5} - 10^{10.5} M_sun, in good accord with known tren"},"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":"astro-ph/0405537","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-05-27T04:02:02Z","cross_cats_sorted":[],"title_canon_sha256":"81f5bab246cdc33c1beac182dfc153205b4d035d00268715f11a2aba85aa57d0","abstract_canon_sha256":"4a2019b7c57a3451252ba489970fd2895fa121f86b6cc0fad09406fccb4b48cf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:51:12.343195Z","signature_b64":"wN30JJYo4x6BOzXtvp47BgAEz3BAE2ZEMzAQAm33M/O+mtEyfsPTIlzA7OrguYMfM9ttu4lFRzcGHL61IkYSBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c613d38d209d10d478a34af08ffd50ce9896937ae6e299faaea366ba26adf947","last_reissued_at":"2026-07-04T15:51:12.342819Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:51:12.342819Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Uomoto, C. A. Tremonti, D. J. Schlegel, E. W. Peng, G. Kauffmann, J. Brinchmann, J. Brinkmann, M. Fukugita, M. Seibert, S. Charlot, S. D. M. White, T. M. Heckman","submitted_at":"2004-05-27T04:02:02Z","abstract_excerpt":"We utilize Sloan Digital Sky Survey imaging and spectroscopy of ~53,000 star-forming galaxies at z~0.1 to study the relation between stellar mass and gas-phase metallicity. We derive gas-phase oxygen abundances and stellar masses using new techniques which make use of the latest stellar evolutionary synthesis and photoionization models. We find a tight (+/-0.1 dex) correlation between stellar mass and metallicity spanning over 3 orders of magnitude in stellar mass and a factor of 10 in metallicity. The relation is relatively steep from 10^{8.5} - 10^{10.5} M_sun, in good accord with known tren"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0405537","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0405537/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":"astro-ph/0405537","created_at":"2026-07-04T15:51:12.342871+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0405537v1","created_at":"2026-07-04T15:51:12.342871+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0405537","created_at":"2026-07-04T15:51:12.342871+00:00"},{"alias_kind":"pith_short_12","alias_value":"YYJ5HDJATUIN","created_at":"2026-07-04T15:51:12.342871+00:00"},{"alias_kind":"pith_short_16","alias_value":"YYJ5HDJATUINI6FD","created_at":"2026-07-04T15:51:12.342871+00:00"},{"alias_kind":"pith_short_8","alias_value":"YYJ5HDJA","created_at":"2026-07-04T15:51:12.342871+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":51,"internal_anchor_count":31,"sample":[{"citing_arxiv_id":"2607.07818","citing_title":"The DESI View of the Faint Radio Source Population in LoTSS DR2","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2607.06933","citing_title":"Constructing a Mock Galaxy Catalog for the All-sky SPECtroscopic Survey of Nearby Galaxies (A-SPEC) Using the Machine-assisted Semi-Simulation Model","ref_index":120,"is_internal_anchor":true},{"citing_arxiv_id":"2607.05295","citing_title":"Toward Unbiased Abundance Measurements in Inhomogeneous $\\mathrm{H\\,II}$ Regions","ref_index":4,"is_internal_anchor":true},{"citing_arxiv_id":"2607.00408","citing_title":"Exploring the synergies of $[\\mathrm{O\\,II}]\\lambda 3727$ with MUSE spectroscopy in PHANGS H II regions","ref_index":83,"is_internal_anchor":true},{"citing_arxiv_id":"2606.30207","citing_title":"Operational capabilities and on-sky performance of SAMOS at the completion of science commissioning","ref_index":59,"is_internal_anchor":true},{"citing_arxiv_id":"2605.30410","citing_title":"RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9","ref_index":117,"is_internal_anchor":true},{"citing_arxiv_id":"2605.30513","citing_title":"The JADES Mass-Metallicity and Fundamental Metallicity Relations at $z\\gtrsim2$ Using New High-Redshift Metallicity Calibrations","ref_index":93,"is_internal_anchor":true},{"citing_arxiv_id":"2606.02738","citing_title":"Signature of Bursty Star Formation in the High-Redshift Galaxies Detected with JWST","ref_index":232,"is_internal_anchor":true},{"citing_arxiv_id":"2606.13781","citing_title":"CANUCS/Technicolor Data Release 2: A Catalogue of Galaxy Structural Parameters in up to 29 HST+JWST bands and a Multi-Wavelength Exploration of the Galaxy Size-Mass Relation at $0.6 < z \\leq 4$","ref_index":88,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04090","citing_title":"Mapping the nuclear environments of extreme coronal line emitting galaxies","ref_index":122,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04208","citing_title":"HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy","ref_index":79,"is_internal_anchor":true},{"citing_arxiv_id":"2606.05780","citing_title":"WISE Photometry of Galaxies within 10 Mpc","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2606.10027","citing_title":"Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2606.11345","citing_title":"JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity","ref_index":286,"is_internal_anchor":true},{"citing_arxiv_id":"2606.12254","citing_title":"Investigating the young stellar populations and hierarchies in nearby galaxies with the UVIT. II. Presenting the properties of ~25,000 UV-detected star-forming clumps","ref_index":141,"is_internal_anchor":true},{"citing_arxiv_id":"2606.12541","citing_title":"DESI as sparse Integral Field Spectrograph I: Spatially resolved chemical enrichment in star-forming galaxies at $z\\leq0.1$","ref_index":85,"is_internal_anchor":true},{"citing_arxiv_id":"2606.25995","citing_title":"The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations","ref_index":133,"is_internal_anchor":true},{"citing_arxiv_id":"2606.18244","citing_title":"PAHSPECS: Spatially Resolved PAH Spectroscopy at cosmic noon with JWST MIRI MRS","ref_index":71,"is_internal_anchor":true},{"citing_arxiv_id":"2606.22619","citing_title":"Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2606.25164","citing_title":"Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068","ref_index":138,"is_internal_anchor":true},{"citing_arxiv_id":"2606.27048","citing_title":"Optical observations of candidate host galaxies of eight fast X-ray transients","ref_index":138,"is_internal_anchor":true},{"citing_arxiv_id":"2606.25164","citing_title":"Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068","ref_index":138,"is_internal_anchor":true},{"citing_arxiv_id":"2606.25018","citing_title":"X-rays Mark the Spot: The Effects of Reduced Metallicity on X-ray AGN Obscuration at High Redshift","ref_index":64,"is_internal_anchor":true},{"citing_arxiv_id":"2605.23049","citing_title":"SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \\sim 0$-7: Mass Dependence and Redshift Evolution","ref_index":134,"is_internal_anchor":true},{"citing_arxiv_id":"2303.08149","citing_title":"Direct T_e-based Metallicities of z=2-9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon","ref_index":106,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2","json":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2.json","graph_json":"https://pith.science/api/pith-number/YYJ5HDJATUINI6FDJLYI77KQZ2/graph.json","events_json":"https://pith.science/api/pith-number/YYJ5HDJATUINI6FDJLYI77KQZ2/events.json","paper":"https://pith.science/paper/YYJ5HDJA"},"agent_actions":{"view_html":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2","download_json":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2.json","view_paper":"https://pith.science/paper/YYJ5HDJA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0405537&json=true","fetch_graph":"https://pith.science/api/pith-number/YYJ5HDJATUINI6FDJLYI77KQZ2/graph.json","fetch_events":"https://pith.science/api/pith-number/YYJ5HDJATUINI6FDJLYI77KQZ2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2/action/storage_attestation","attest_author":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2/action/author_attestation","sign_citation":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2/action/citation_signature","submit_replication":"https://pith.science/pith/YYJ5HDJATUINI6FDJLYI77KQZ2/action/replication_record"}},"created_at":"2026-07-04T15:51:12.342871+00:00","updated_at":"2026-07-04T15:51:12.342871+00:00"}