{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:7KVEMSV4LP6ZOY6OTVN2J4QQUD","short_pith_number":"pith:7KVEMSV4","schema_version":"1.0","canonical_sha256":"faaa464abc5bfd9763ce9d5ba4f210a0c5d993074e60880b93be08292d6941c5","source":{"kind":"arxiv","id":"1603.02284","version":1},"attestation_state":"computed","paper":{"title":"The MOSDEF Survey: The strong agreement between H-alpha and UV-to-FIR star formation rates for z~2 star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alice E. Shapley, Alison L. Coil, Bahram Mobasher, Brian Siana, Charlie Conroy, Guillermo Barro, Hanae Inami, Imad Pasha, Irene Shivaei, Mariska Kriek, Mojegan Azadi, Naveen A. Reddy, Ryan Sanders, Sedona H. Price, William R. Freeman","submitted_at":"2016-03-07T21:00:17Z","abstract_excerpt":"We present the first direct comparison between Balmer line and panchromatic SED-based SFRs for z~2 galaxies. For this comparison we used 17 star-forming galaxies selected from the MOSFIRE Deep Evolution Field (MOSDEF) survey, with $3\\sigma$ detections for H$\\alpha$ and at least two IR bands (Spitzer/MIPS 24$\\mu$m and Herschel/PACS 100 and 160$\\mu$m, and in some cases Herschel/SPIRE 250, 350, and 500$\\mu$m). The galaxies have total IR (8-1000$\\mu$m) luminosities of $\\sim10^{11.4}-10^{12.4}\\,\\textrm{L}_\\odot$ and star-formation rates (SFRs) of $\\sim30-250\\,\\textrm{M}_\\odot\\,\\mathrm{yr^{-1}}$. We"},"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":"1603.02284","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-03-07T21:00:17Z","cross_cats_sorted":[],"title_canon_sha256":"c8c3c1cea534925d210d2c9492bca576eb078fdab39ca3e302e4146e1500631c","abstract_canon_sha256":"198739739ddf91ac0c552bcef4521e7aa763a4cc0177f7999112de6903929098"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:17:40.999627Z","signature_b64":"u9fOrcfJhG7LklJyEswxJ7GQIv1jjeEqIY3mgLj+vWQ0Wsog3FSIMCpSeczHuncH4l3BjwTMbPEBYcBl+ZBfCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"faaa464abc5bfd9763ce9d5ba4f210a0c5d993074e60880b93be08292d6941c5","last_reissued_at":"2026-05-18T01:17:40.998869Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:17:40.998869Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The MOSDEF Survey: The strong agreement between H-alpha and UV-to-FIR star formation rates for z~2 star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alice E. Shapley, Alison L. Coil, Bahram Mobasher, Brian Siana, Charlie Conroy, Guillermo Barro, Hanae Inami, Imad Pasha, Irene Shivaei, Mariska Kriek, Mojegan Azadi, Naveen A. Reddy, Ryan Sanders, Sedona H. Price, William R. Freeman","submitted_at":"2016-03-07T21:00:17Z","abstract_excerpt":"We present the first direct comparison between Balmer line and panchromatic SED-based SFRs for z~2 galaxies. For this comparison we used 17 star-forming galaxies selected from the MOSFIRE Deep Evolution Field (MOSDEF) survey, with $3\\sigma$ detections for H$\\alpha$ and at least two IR bands (Spitzer/MIPS 24$\\mu$m and Herschel/PACS 100 and 160$\\mu$m, and in some cases Herschel/SPIRE 250, 350, and 500$\\mu$m). The galaxies have total IR (8-1000$\\mu$m) luminosities of $\\sim10^{11.4}-10^{12.4}\\,\\textrm{L}_\\odot$ and star-formation rates (SFRs) of $\\sim30-250\\,\\textrm{M}_\\odot\\,\\mathrm{yr^{-1}}$. We"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.02284","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":"1603.02284","created_at":"2026-05-18T01:17:40.998984+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.02284v1","created_at":"2026-05-18T01:17:40.998984+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.02284","created_at":"2026-05-18T01:17:40.998984+00:00"},{"alias_kind":"pith_short_12","alias_value":"7KVEMSV4LP6Z","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"7KVEMSV4LP6ZOY6O","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"7KVEMSV4","created_at":"2026-05-18T12:30:04.600751+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/7KVEMSV4LP6ZOY6OTVN2J4QQUD","json":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD.json","graph_json":"https://pith.science/api/pith-number/7KVEMSV4LP6ZOY6OTVN2J4QQUD/graph.json","events_json":"https://pith.science/api/pith-number/7KVEMSV4LP6ZOY6OTVN2J4QQUD/events.json","paper":"https://pith.science/paper/7KVEMSV4"},"agent_actions":{"view_html":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD","download_json":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD.json","view_paper":"https://pith.science/paper/7KVEMSV4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.02284&json=true","fetch_graph":"https://pith.science/api/pith-number/7KVEMSV4LP6ZOY6OTVN2J4QQUD/graph.json","fetch_events":"https://pith.science/api/pith-number/7KVEMSV4LP6ZOY6OTVN2J4QQUD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD/action/storage_attestation","attest_author":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD/action/author_attestation","sign_citation":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD/action/citation_signature","submit_replication":"https://pith.science/pith/7KVEMSV4LP6ZOY6OTVN2J4QQUD/action/replication_record"}},"created_at":"2026-05-18T01:17:40.998984+00:00","updated_at":"2026-05-18T01:17:40.998984+00:00"}