{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:DGQE5KSG5KOCKANSFUDHYARQXA","short_pith_number":"pith:DGQE5KSG","schema_version":"1.0","canonical_sha256":"19a04eaa46ea9c2501b22d067c0230b82e8f03fdbb0daedb588d041e63ad18df","source":{"kind":"arxiv","id":"1807.02952","version":1},"attestation_state":"computed","paper":{"title":"Shocked POststarburst Galaxy Survey. III. The Ultraviolet Properties of SPOGs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anne M. Medling, C. Meg Urry, Felipe Ardila, Jeffrey A. Rich, Jes\\'us Falc\\'on-Barroso, John S. Mulchaey, Katherine Alatalo, Kristina Nyland, Lauranne Lanz, Lisa J. Kewley, Philip N. Appleton, Rachael L. Beaton, Sabrina L. Cales, Theodoros Bitsakis","submitted_at":"2018-07-09T05:57:36Z","abstract_excerpt":"The Shocked POststarburst Galaxy Survey (SPOGS) aims to identify galaxies in the transitional phase between actively star-forming and quiescence with nebular lines that are excited from shocks rather than star formation processes. We explored the ultraviolet (UV) properties of objects with near-ultraviolet (NUV) and far-ultraviolet (FUV) photometry from archival GALEX data; 444 objects were detected in both bands, 365 in only NUV, and 24 in only FUV, for a total of 833 observed objects. We compared SPOGs to samples of Star-forming galaxies (SFs), Quiescent galaxies (Qs), classical E+A post-sta"},"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":"1807.02952","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-07-09T05:57:36Z","cross_cats_sorted":[],"title_canon_sha256":"25890de0df9ca808dc516e9bddf98815de7c3ccf036656368f30d19ae1c86b07","abstract_canon_sha256":"2be0b0c066f2127e8b19aad76d230b4d775a80d5fa74c341ce90867ea90171c9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:08:35.511345Z","signature_b64":"1/HmZdRawVjg1V+OnSTy8st/J24Cl9QDTrmOTlnnlyYwLyhy1kcZHbT95hb4lhspMaXZPTGnHbZaIH3PQ14ZCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"19a04eaa46ea9c2501b22d067c0230b82e8f03fdbb0daedb588d041e63ad18df","last_reissued_at":"2026-05-18T00:08:35.510639Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:08:35.510639Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Shocked POststarburst Galaxy Survey. III. The Ultraviolet Properties of SPOGs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anne M. Medling, C. Meg Urry, Felipe Ardila, Jeffrey A. Rich, Jes\\'us Falc\\'on-Barroso, John S. Mulchaey, Katherine Alatalo, Kristina Nyland, Lauranne Lanz, Lisa J. Kewley, Philip N. Appleton, Rachael L. Beaton, Sabrina L. Cales, Theodoros Bitsakis","submitted_at":"2018-07-09T05:57:36Z","abstract_excerpt":"The Shocked POststarburst Galaxy Survey (SPOGS) aims to identify galaxies in the transitional phase between actively star-forming and quiescence with nebular lines that are excited from shocks rather than star formation processes. We explored the ultraviolet (UV) properties of objects with near-ultraviolet (NUV) and far-ultraviolet (FUV) photometry from archival GALEX data; 444 objects were detected in both bands, 365 in only NUV, and 24 in only FUV, for a total of 833 observed objects. We compared SPOGs to samples of Star-forming galaxies (SFs), Quiescent galaxies (Qs), classical E+A post-sta"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.02952","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":"1807.02952","created_at":"2026-05-18T00:08:35.510749+00:00"},{"alias_kind":"arxiv_version","alias_value":"1807.02952v1","created_at":"2026-05-18T00:08:35.510749+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.02952","created_at":"2026-05-18T00:08:35.510749+00:00"},{"alias_kind":"pith_short_12","alias_value":"DGQE5KSG5KOC","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"DGQE5KSG5KOCKANS","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"DGQE5KSG","created_at":"2026-05-18T12:32:19.392346+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/DGQE5KSG5KOCKANSFUDHYARQXA","json":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA.json","graph_json":"https://pith.science/api/pith-number/DGQE5KSG5KOCKANSFUDHYARQXA/graph.json","events_json":"https://pith.science/api/pith-number/DGQE5KSG5KOCKANSFUDHYARQXA/events.json","paper":"https://pith.science/paper/DGQE5KSG"},"agent_actions":{"view_html":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA","download_json":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA.json","view_paper":"https://pith.science/paper/DGQE5KSG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1807.02952&json=true","fetch_graph":"https://pith.science/api/pith-number/DGQE5KSG5KOCKANSFUDHYARQXA/graph.json","fetch_events":"https://pith.science/api/pith-number/DGQE5KSG5KOCKANSFUDHYARQXA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA/action/storage_attestation","attest_author":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA/action/author_attestation","sign_citation":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA/action/citation_signature","submit_replication":"https://pith.science/pith/DGQE5KSG5KOCKANSFUDHYARQXA/action/replication_record"}},"created_at":"2026-05-18T00:08:35.510749+00:00","updated_at":"2026-05-18T00:08:35.510749+00:00"}