{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:7SF2BT7DUR57TT4JHTTCCHK6IT","short_pith_number":"pith:7SF2BT7D","schema_version":"1.0","canonical_sha256":"fc8ba0cfe3a47bf9cf893ce6211d5e44c2587b1462b703c2b3ab1b783cef43ae","source":{"kind":"arxiv","id":"1210.2362","version":1},"attestation_state":"computed","paper":{"title":"Cosmic Evolution of Star-Formation Enhancement in Close Major-Merger Galaxy Pairs Since z = 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Conley, A. Cooray, A. Franceschini, B. Magnelli, B. Schulz, C. Bridge, C. K. Xu, D. Elbaz, D. L. Shupe, D. Lutz, E. Le Floc'h, F. Pozzi, G. Marsden, H. Aussel, J. Bock, J. D. Vieira, L. Riguccini, L. Wang, M. B'ethermin, M. Vaccari, M. Zemcov, N. Lu, N. Scoville, S. Berta, S. J. Oliver","submitted_at":"2012-10-08T17:50:05Z","abstract_excerpt":"The infrared (IR) emission of M_* galaxies (10^{10.4} < M_{star} < 10^{11.0} M_\\sun) in galaxy pairs, derived using data obtained in Herschel (PEP/HerMES) and Spitzer (S-COSMOS) surveys, is compared to that of single disk galaxies in well matched control samples to study the cosmic evolution of the star-formation enhancement induced by galaxy-galaxy interaction. Both the mean IR SED and mean IR luminosity of star-forming galaxies (SFGs) in SFG+SFG (S+S) pairs in the redshift bin of 0.6 < z < 1 are consistent with no star-formation enhancement. SFGs in S+S pairs in a lower redshift bin of 0.2 <"},"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":"1210.2362","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-10-08T17:50:05Z","cross_cats_sorted":[],"title_canon_sha256":"87736e21ffc604996712e39afc1a6e904a1f788b34528ff8b3bf39f1c56a4b03","abstract_canon_sha256":"5c158e76159c2574a2f8865005530fb6c3852518af1baafba22a1d5ec21e6867"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:04.473164Z","signature_b64":"RxeG5R+WHV0Q+84tz3H5gX5rcHv7AhhCn7/n2JgsrWBo3nHTs9Tp8fxDO0+Cu11vGVaP2JF6HFGohq8DPOz8BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fc8ba0cfe3a47bf9cf893ce6211d5e44c2587b1462b703c2b3ab1b783cef43ae","last_reissued_at":"2026-05-18T01:54:04.472765Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:04.472765Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic Evolution of Star-Formation Enhancement in Close Major-Merger Galaxy Pairs Since z = 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Conley, A. Cooray, A. Franceschini, B. Magnelli, B. Schulz, C. Bridge, C. K. Xu, D. Elbaz, D. L. Shupe, D. Lutz, E. Le Floc'h, F. Pozzi, G. Marsden, H. Aussel, J. Bock, J. D. Vieira, L. Riguccini, L. Wang, M. B'ethermin, M. Vaccari, M. Zemcov, N. Lu, N. Scoville, S. Berta, S. J. Oliver","submitted_at":"2012-10-08T17:50:05Z","abstract_excerpt":"The infrared (IR) emission of M_* galaxies (10^{10.4} < M_{star} < 10^{11.0} M_\\sun) in galaxy pairs, derived using data obtained in Herschel (PEP/HerMES) and Spitzer (S-COSMOS) surveys, is compared to that of single disk galaxies in well matched control samples to study the cosmic evolution of the star-formation enhancement induced by galaxy-galaxy interaction. Both the mean IR SED and mean IR luminosity of star-forming galaxies (SFGs) in SFG+SFG (S+S) pairs in the redshift bin of 0.6 < z < 1 are consistent with no star-formation enhancement. SFGs in S+S pairs in a lower redshift bin of 0.2 <"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.2362","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":"1210.2362","created_at":"2026-05-18T01:54:04.472825+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.2362v1","created_at":"2026-05-18T01:54:04.472825+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.2362","created_at":"2026-05-18T01:54:04.472825+00:00"},{"alias_kind":"pith_short_12","alias_value":"7SF2BT7DUR57","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"7SF2BT7DUR57TT4J","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"7SF2BT7D","created_at":"2026-05-18T12:26:58.693483+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/7SF2BT7DUR57TT4JHTTCCHK6IT","json":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT.json","graph_json":"https://pith.science/api/pith-number/7SF2BT7DUR57TT4JHTTCCHK6IT/graph.json","events_json":"https://pith.science/api/pith-number/7SF2BT7DUR57TT4JHTTCCHK6IT/events.json","paper":"https://pith.science/paper/7SF2BT7D"},"agent_actions":{"view_html":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT","download_json":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT.json","view_paper":"https://pith.science/paper/7SF2BT7D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.2362&json=true","fetch_graph":"https://pith.science/api/pith-number/7SF2BT7DUR57TT4JHTTCCHK6IT/graph.json","fetch_events":"https://pith.science/api/pith-number/7SF2BT7DUR57TT4JHTTCCHK6IT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT/action/storage_attestation","attest_author":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT/action/author_attestation","sign_citation":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT/action/citation_signature","submit_replication":"https://pith.science/pith/7SF2BT7DUR57TT4JHTTCCHK6IT/action/replication_record"}},"created_at":"2026-05-18T01:54:04.472825+00:00","updated_at":"2026-05-18T01:54:04.472825+00:00"}