{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:E4QJBD52NZIAJXC5PYORMAHZJW","short_pith_number":"pith:E4QJBD52","schema_version":"1.0","canonical_sha256":"2720908fba6e5004dc5d7e1d1600f94d8dc15acab5e93b3310b046486eabdd3f","source":{"kind":"arxiv","id":"2002.03818","version":4},"attestation_state":"computed","paper":{"title":"Molecular gas and star formation activity in LIRGs in clusters at intermediate redshifts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C.P. Haines, D. Sp\\'erone-Longin, E. Egami, E. Schinnerer, F. Bigiel, F. Combes, G. Castignani, M. Arnaud, M. Jauzac, M. Krips, P. Jablonka, S. Garc\\'ia-Burillo, T. Rawle","submitted_at":"2020-02-10T14:45:54Z","abstract_excerpt":"We investigate the role of dense Mpc-scale environments in processing molecular gas of cluster galaxies as they fall into the cluster cores. We consider $\\sim20$ luminous infrared galaxies (LIRGs) in intermediate-$z$ clusters, from the Hershel Lensing Survey and the Local Cluster Substructure Survey. They include MACS J0717.5+3745 at $z=0.546$ and Abell 697, 963, 1763, and 2219 at $z=0.2-0.3$. We have performed far infrared to ultraviolet spectral energy distribution modeling of the LIRGs, which span cluster-centric distances within $r/r_{200}\\simeq0.2-1.6$. We have observed the LIRGs in CO(1$"},"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":"2002.03818","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-02-10T14:45:54Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"998e1fc34403be94f68ac400c8ccabfbb26b2cd11c02797bc93b2c4a585ca927","abstract_canon_sha256":"eb6894387511f6d1aebeb9117e9bb710a0f8ea040125631d0cec01464e673c6e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:28:06.907119Z","signature_b64":"6G60ovh2phx05gEE8bmFoxUpYpwwnEZhmvZ2rPq8wqx/M8d138BaanWVDN4x5nok/a6/63tNrbtcpm5NDRTLCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2720908fba6e5004dc5d7e1d1600f94d8dc15acab5e93b3310b046486eabdd3f","last_reissued_at":"2026-07-05T01:28:06.906655Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:28:06.906655Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Molecular gas and star formation activity in LIRGs in clusters at intermediate redshifts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C.P. Haines, D. Sp\\'erone-Longin, E. Egami, E. Schinnerer, F. Bigiel, F. Combes, G. Castignani, M. Arnaud, M. Jauzac, M. Krips, P. Jablonka, S. Garc\\'ia-Burillo, T. Rawle","submitted_at":"2020-02-10T14:45:54Z","abstract_excerpt":"We investigate the role of dense Mpc-scale environments in processing molecular gas of cluster galaxies as they fall into the cluster cores. We consider $\\sim20$ luminous infrared galaxies (LIRGs) in intermediate-$z$ clusters, from the Hershel Lensing Survey and the Local Cluster Substructure Survey. They include MACS J0717.5+3745 at $z=0.546$ and Abell 697, 963, 1763, and 2219 at $z=0.2-0.3$. We have performed far infrared to ultraviolet spectral energy distribution modeling of the LIRGs, which span cluster-centric distances within $r/r_{200}\\simeq0.2-1.6$. We have observed the LIRGs in CO(1$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2002.03818","kind":"arxiv","version":4},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2002.03818/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2002.03818","created_at":"2026-07-05T01:28:06.906712+00:00"},{"alias_kind":"arxiv_version","alias_value":"2002.03818v4","created_at":"2026-07-05T01:28:06.906712+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2002.03818","created_at":"2026-07-05T01:28:06.906712+00:00"},{"alias_kind":"pith_short_12","alias_value":"E4QJBD52NZIA","created_at":"2026-07-05T01:28:06.906712+00:00"},{"alias_kind":"pith_short_16","alias_value":"E4QJBD52NZIAJXC5","created_at":"2026-07-05T01:28:06.906712+00:00"},{"alias_kind":"pith_short_8","alias_value":"E4QJBD52","created_at":"2026-07-05T01:28:06.906712+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.28257","citing_title":"When Jets Don't Quench: Near-Infrared H$_{2}$ in Star Forming Low-Excitation Radio Galaxies","ref_index":210,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW","json":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW.json","graph_json":"https://pith.science/api/pith-number/E4QJBD52NZIAJXC5PYORMAHZJW/graph.json","events_json":"https://pith.science/api/pith-number/E4QJBD52NZIAJXC5PYORMAHZJW/events.json","paper":"https://pith.science/paper/E4QJBD52"},"agent_actions":{"view_html":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW","download_json":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW.json","view_paper":"https://pith.science/paper/E4QJBD52","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2002.03818&json=true","fetch_graph":"https://pith.science/api/pith-number/E4QJBD52NZIAJXC5PYORMAHZJW/graph.json","fetch_events":"https://pith.science/api/pith-number/E4QJBD52NZIAJXC5PYORMAHZJW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW/action/storage_attestation","attest_author":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW/action/author_attestation","sign_citation":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW/action/citation_signature","submit_replication":"https://pith.science/pith/E4QJBD52NZIAJXC5PYORMAHZJW/action/replication_record"}},"created_at":"2026-07-05T01:28:06.906712+00:00","updated_at":"2026-07-05T01:28:06.906712+00:00"}