{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:3M3V2NHH52DXVSH3E5CWGJOX4A","short_pith_number":"pith:3M3V2NHH","schema_version":"1.0","canonical_sha256":"db375d34e7ee877ac8fb27456325d7e016411bb6d6aec948762ebbd6ae85288e","source":{"kind":"arxiv","id":"1612.06082","version":1},"attestation_state":"computed","paper":{"title":"HST H{\\alpha} grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"David G. Gilbank, Karl Glazebrook, Michael L. Balogh, Richard G. Bower, Riona Ramraj, Rosalind E. Skelton, Sarah-Louise Blyth","submitted_at":"2016-12-19T09:06:41Z","abstract_excerpt":"We present measurements of star formation rates (SFRs) for dwarf galaxies (M*~10^8.5 Msun ) at z~1 using near-infrared slitless spectroscopy from the Hubble Space Telescope (HST) by targetting and measuring the luminosity of the H{\\alpha} emission line. Our sample is derived from the Redshift One LDSS3 Emission Line Survey (ROLES), which used [O II]{\\lambda} 3727 as a tracer of star formation to target very low stellar masses down to very low SFRs (~0.1 Msun yr^-1) at this epoch. Dust corrections are estimated using SED-fits and we find, by comparison with other studies using Balmer decrement "},"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":"1612.06082","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-12-19T09:06:41Z","cross_cats_sorted":[],"title_canon_sha256":"215df5869ea89e92247e6d06ef2e570d9e84981219753f0e54d775e1227f9eb5","abstract_canon_sha256":"65109169846424b9210b0267da37f4b8e6690c67beea7bd182665cd9749f20e7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:51:41.382351Z","signature_b64":"AUuBaIbceYbjeQilTbwroQIsE+HleiGn3Ze+uc3wqBzS4hGnMsyLnfKfSZna9giaBSJ8nCdW9Mkj1GfPyc7fCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"db375d34e7ee877ac8fb27456325d7e016411bb6d6aec948762ebbd6ae85288e","last_reissued_at":"2026-05-18T00:51:41.381961Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:51:41.381961Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HST H{\\alpha} grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"David G. Gilbank, Karl Glazebrook, Michael L. Balogh, Richard G. Bower, Riona Ramraj, Rosalind E. Skelton, Sarah-Louise Blyth","submitted_at":"2016-12-19T09:06:41Z","abstract_excerpt":"We present measurements of star formation rates (SFRs) for dwarf galaxies (M*~10^8.5 Msun ) at z~1 using near-infrared slitless spectroscopy from the Hubble Space Telescope (HST) by targetting and measuring the luminosity of the H{\\alpha} emission line. Our sample is derived from the Redshift One LDSS3 Emission Line Survey (ROLES), which used [O II]{\\lambda} 3727 as a tracer of star formation to target very low stellar masses down to very low SFRs (~0.1 Msun yr^-1) at this epoch. Dust corrections are estimated using SED-fits and we find, by comparison with other studies using Balmer decrement "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.06082","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":"1612.06082","created_at":"2026-05-18T00:51:41.382027+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.06082v1","created_at":"2026-05-18T00:51:41.382027+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.06082","created_at":"2026-05-18T00:51:41.382027+00:00"},{"alias_kind":"pith_short_12","alias_value":"3M3V2NHH52DX","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_16","alias_value":"3M3V2NHH52DXVSH3","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_8","alias_value":"3M3V2NHH","created_at":"2026-05-18T12:29:55.572404+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/3M3V2NHH52DXVSH3E5CWGJOX4A","json":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A.json","graph_json":"https://pith.science/api/pith-number/3M3V2NHH52DXVSH3E5CWGJOX4A/graph.json","events_json":"https://pith.science/api/pith-number/3M3V2NHH52DXVSH3E5CWGJOX4A/events.json","paper":"https://pith.science/paper/3M3V2NHH"},"agent_actions":{"view_html":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A","download_json":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A.json","view_paper":"https://pith.science/paper/3M3V2NHH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.06082&json=true","fetch_graph":"https://pith.science/api/pith-number/3M3V2NHH52DXVSH3E5CWGJOX4A/graph.json","fetch_events":"https://pith.science/api/pith-number/3M3V2NHH52DXVSH3E5CWGJOX4A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A/action/storage_attestation","attest_author":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A/action/author_attestation","sign_citation":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A/action/citation_signature","submit_replication":"https://pith.science/pith/3M3V2NHH52DXVSH3E5CWGJOX4A/action/replication_record"}},"created_at":"2026-05-18T00:51:41.382027+00:00","updated_at":"2026-05-18T00:51:41.382027+00:00"}