{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:NLZ2VXPJWFZLG3B4FGPR3ZAMUO","short_pith_number":"pith:NLZ2VXPJ","schema_version":"1.0","canonical_sha256":"6af3aadde9b172b36c3c299f1de40ca3b973d90021e996afbfb6d7127ac92741","source":{"kind":"arxiv","id":"1412.1482","version":1},"attestation_state":"computed","paper":{"title":"Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron A. Dutton, Aleksandar M. Diamond-Stanic, Alexie Leauthaud, Alfonso Arag\\'on-Salamanca, Anne-Marie Weijmans, Audrey Simmons, Benjamin A. Thompson, Brian Cherinka, Carles Badenes, Charlie Conroy, Cheng Li, Christy Tremonti, Claudia Maraston, Daniel Oravetz, Daniel Thomas, David A. Wake, David R. Law, David Schlegel, David Wilkinson, Dmitry Bizyaev, Elena Malanushenko, Eric Emsellem, Evelyn J. Johnston, Francesco Belfiore, Guillermo A. Blanc, Guinevere Kauffmann, Hai Fu, James E. Gunn, James Etherington, Jeremy L. Tinker, J\\'esus Falc\\'on-Barroso, Joel R. Brownstein, Johan H. Knapen, John K. Parejko, Jos\\'e R. S\\'anchez-Gallego, Joss Bland-Hawthorn, Kaike Pan, Kai Zhang, Karen Kinemuchi, Karen Masters, Karun Thanjavur, Kevin Bundy, Kyle B. Westfall, Lihwai Lin, Lodovico Coccato, Mark A. Klaene, Matthew A. Bershady, Matthias Steinmetz, Michael R. Blanton, Michael R. Merrifield, Michele Cappellari, Nell Byler, Nicholas MacDonald, Niv Drory, Oliver Steele, Paul Harding, Peter M. Frinchaboy, Remco C. E. van den Bosch, Renbin Yan, Richard M. McDermid, Robert C. Nichol, Roberto Maiolino, Sebastian F. Sanchez, Shelley Wright, Shude Mao, Ting Xiao, Viktor Malanushenko, Vladimir Avila-Reese","submitted_at":"2014-12-03T21:00:27Z","abstract_excerpt":"We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10,000 nearby galaxies. We summarize essential characteristics of the instrument and survey design in the context of MaNGA's key science goals and present prototype observations to demonstrate MaNGA's scientific potential. MaNGA em"},"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":"1412.1482","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-12-03T21:00:27Z","cross_cats_sorted":[],"title_canon_sha256":"dad1cfe36bf98906cb99e8d2ed303b1ef58e80861bdc383f70f2e06a8797772e","abstract_canon_sha256":"73af323c03e3c2da0b4865f52722e5fd2f7cad9112dd5da7eedf49f4a0cd84c0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:23.541643Z","signature_b64":"9iy0s5pSJXcaeP7onbc5E1iYrdPsMgEBFWQ7x9C3lwaqzlTIKSakeRvuimDZuYN/Vc3IJXoYc6lwXzyzVrUBCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6af3aadde9b172b36c3c299f1de40ca3b973d90021e996afbfb6d7127ac92741","last_reissued_at":"2026-05-18T01:41:23.540903Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:23.540903Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron A. Dutton, Aleksandar M. Diamond-Stanic, Alexie Leauthaud, Alfonso Arag\\'on-Salamanca, Anne-Marie Weijmans, Audrey Simmons, Benjamin A. Thompson, Brian Cherinka, Carles Badenes, Charlie Conroy, Cheng Li, Christy Tremonti, Claudia Maraston, Daniel Oravetz, Daniel Thomas, David A. Wake, David R. Law, David Schlegel, David Wilkinson, Dmitry Bizyaev, Elena Malanushenko, Eric Emsellem, Evelyn J. Johnston, Francesco Belfiore, Guillermo A. Blanc, Guinevere Kauffmann, Hai Fu, James E. Gunn, James Etherington, Jeremy L. Tinker, J\\'esus Falc\\'on-Barroso, Joel R. Brownstein, Johan H. Knapen, John K. Parejko, Jos\\'e R. S\\'anchez-Gallego, Joss Bland-Hawthorn, Kaike Pan, Kai Zhang, Karen Kinemuchi, Karen Masters, Karun Thanjavur, Kevin Bundy, Kyle B. Westfall, Lihwai Lin, Lodovico Coccato, Mark A. Klaene, Matthew A. Bershady, Matthias Steinmetz, Michael R. Blanton, Michael R. Merrifield, Michele Cappellari, Nell Byler, Nicholas MacDonald, Niv Drory, Oliver Steele, Paul Harding, Peter M. Frinchaboy, Remco C. E. van den Bosch, Renbin Yan, Richard M. McDermid, Robert C. Nichol, Roberto Maiolino, Sebastian F. Sanchez, Shelley Wright, Shude Mao, Ting Xiao, Viktor Malanushenko, Vladimir Avila-Reese","submitted_at":"2014-12-03T21:00:27Z","abstract_excerpt":"We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10,000 nearby galaxies. We summarize essential characteristics of the instrument and survey design in the context of MaNGA's key science goals and present prototype observations to demonstrate MaNGA's scientific potential. MaNGA em"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.1482","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":"1412.1482","created_at":"2026-05-18T01:41:23.541044+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.1482v1","created_at":"2026-05-18T01:41:23.541044+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.1482","created_at":"2026-05-18T01:41:23.541044+00:00"},{"alias_kind":"pith_short_12","alias_value":"NLZ2VXPJWFZL","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"NLZ2VXPJWFZLG3B4","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"NLZ2VXPJ","created_at":"2026-05-18T12:28:41.024544+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":24,"internal_anchor_count":10,"sample":[{"citing_arxiv_id":"1906.09853","citing_title":"Evidence of a fast bar in the weakly-interacting galaxy NGC 4264 with MUSE","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2605.23006","citing_title":"\\texttt{calypso}: a Parameter-Conditioned Stochastic Surrogate Model for Circumbinary Accretion Time-Series","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2502.10922","citing_title":"The Impact of Bars, Spirals and Bulge-Size on Gas-Phase Metallicity Gradients in MaNGA Galaxies","ref_index":14,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21579","citing_title":"Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration","ref_index":75,"is_internal_anchor":true},{"citing_arxiv_id":"2509.19239","citing_title":"Recalibration of the H$\\alpha$ surface brightness-radius relation for planetary nebulae using Gaia DR3: new distances and the Milky Way oxygen radial gradient","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19426","citing_title":"Dwarf and Intermediate-Mass Galaxies in MaNGA: Evidence for Different Evolutionary Trends","ref_index":5,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12973","citing_title":"A Spatially Resolved HI Survey of Seyfert Galaxies: the Role of AGN Feedback in Shaping Atomic Gas Reservoirs","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2509.04067","citing_title":"COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase","ref_index":25,"is_internal_anchor":true},{"citing_arxiv_id":"2605.08353","citing_title":"Empirical estimates of how massive galaxies can be in {\\Lambda}CDM","ref_index":173,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12596","citing_title":"Strong Progenitor Age Bias in Supernova Cosmology. III. Progenitor Age as the Physical Origin of the Type Ia Supernova Magnitude Steps with Host Properties","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12973","citing_title":"A Spatially Resolved HI Survey of Seyfert Galaxies: the Role of AGN Feedback in Shaping Atomic Gas Reservoirs","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2604.03389","citing_title":"The Role of Baryonic and Dark Matter in Bar Kinematics","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2605.10102","citing_title":"From Large Telescopes to the MUltiplexed Survey Telescope (MUST)","ref_index":63,"is_internal_anchor":false},{"citing_arxiv_id":"2605.10102","citing_title":"From Large Telescopes to the MUltiplexed Survey Telescope (MUST)","ref_index":130,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08979","citing_title":"The MaNGA Low-mass disks HUnt for CO (MaLHUCO) Survey","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08353","citing_title":"Empirical estimates of how massive galaxies can be in {\\Lambda}CDM","ref_index":173,"is_internal_anchor":false},{"citing_arxiv_id":"2604.05680","citing_title":"Stellar Population Characterisations in nearby, dusty Early-Type Galaxies","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13195","citing_title":"Galactic Rain: Cool Gas Inflows in Red Geyser Galaxies and Their Connection to AGN Activity and Interactions","ref_index":8,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14092","citing_title":"Radial Distribution of Star Formation and Gas-phase Metallicity in Spiral-Elliptical Galaxy Pairs","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18812","citing_title":"SAGUI: SED-based Segmentation of Multi-band Galaxy Images -- Application to JADES in GOODS-South","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"1607.08538","citing_title":"Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26724","citing_title":"Radial Profiles of Binary Fraction in Elliptical Galaxies","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25219","citing_title":"Spectral Evolution and Transient Broad-Line Features in the Isolated AGN UNAM-KIAS 613","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04434","citing_title":"A CNN--Transformer Denoiser for low-$S/N$ Galaxy Spectra: Stellar Population Recovery in Synthetic Tests","ref_index":2,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO","json":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO.json","graph_json":"https://pith.science/api/pith-number/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/graph.json","events_json":"https://pith.science/api/pith-number/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/events.json","paper":"https://pith.science/paper/NLZ2VXPJ"},"agent_actions":{"view_html":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO","download_json":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO.json","view_paper":"https://pith.science/paper/NLZ2VXPJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.1482&json=true","fetch_graph":"https://pith.science/api/pith-number/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/graph.json","fetch_events":"https://pith.science/api/pith-number/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/action/storage_attestation","attest_author":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/action/author_attestation","sign_citation":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/action/citation_signature","submit_replication":"https://pith.science/pith/NLZ2VXPJWFZLG3B4FGPR3ZAMUO/action/replication_record"}},"created_at":"2026-05-18T01:41:23.541044+00:00","updated_at":"2026-05-18T01:41:23.541044+00:00"}