{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:OASJSKHLBNFCKZIMPJJM6GAN43","short_pith_number":"pith:OASJSKHL","schema_version":"1.0","canonical_sha256":"70249928eb0b4a25650c7a52cf180de6d5ce6b292f7d98bbec6f2d433d8822d5","source":{"kind":"arxiv","id":"2310.01601","version":1},"attestation_state":"computed","paper":{"title":"Uncovering the MIR emission of quiescent galaxies with $JWST$","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. G\\'omez-Guijarro, David Bl\\'anquez-Ses\\'e, D. Langeroodi, D. Rigopoulou, E.-D. Paspaliaris, F. Valentino, G. Brammer, G.E. Magdis, J. Hjorth, M. Lee, M. Shuntov, N.B. Sillassen, R. Gobat, S. Gillman, S. Jin, T. D\\'iaz-Santos, T.R. Greve, V. Kokorev","submitted_at":"2023-10-02T19:50:51Z","abstract_excerpt":"We present a study of the mid-IR (MIR) emission of quiescent galaxies (QGs) beyond the local universe. Using deep $JWST$ imaging in the SMACS-0723 cluster field we identify a mass limited ($M_{*} >10^{9}$M$_{\\odot}$) sample of intermediate redshift QGs ($0.2<z<0.7$) and perform modeling of their rest-frame UV to MIR photometry. We find that QGs exhibit a range of MIR spectra that are composed of a stellar continuum and a dust component that is 1-2 orders of magnitude fainter to that of star-forming galaxies. The observed scatter in the MIR spectra, especially at $\\lambda_{\\rm rest} > 5 \\mu$m, "},"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":"2310.01601","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-10-02T19:50:51Z","cross_cats_sorted":[],"title_canon_sha256":"bf0754828e45bd0778aa3852c311e20081c4d342c6f42ec382303eae4921cf55","abstract_canon_sha256":"f07a9f059a0b406171ee0cf47b6f95bacb2126396d4ad1b2c9a42d4a52515a40"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:07:17.349886Z","signature_b64":"MRmYLWEF2Umq+DjU0gO6tMUASIRLRI0++BFs8LJdQGRTKAz0k5EeOAff3555d2HWSMmI+R9tghq4pfBH4oP5Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"70249928eb0b4a25650c7a52cf180de6d5ce6b292f7d98bbec6f2d433d8822d5","last_reissued_at":"2026-07-05T07:07:17.349361Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:07:17.349361Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Uncovering the MIR emission of quiescent galaxies with $JWST$","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. G\\'omez-Guijarro, David Bl\\'anquez-Ses\\'e, D. Langeroodi, D. Rigopoulou, E.-D. Paspaliaris, F. Valentino, G. Brammer, G.E. Magdis, J. Hjorth, M. Lee, M. Shuntov, N.B. Sillassen, R. Gobat, S. Gillman, S. Jin, T. D\\'iaz-Santos, T.R. Greve, V. Kokorev","submitted_at":"2023-10-02T19:50:51Z","abstract_excerpt":"We present a study of the mid-IR (MIR) emission of quiescent galaxies (QGs) beyond the local universe. Using deep $JWST$ imaging in the SMACS-0723 cluster field we identify a mass limited ($M_{*} >10^{9}$M$_{\\odot}$) sample of intermediate redshift QGs ($0.2<z<0.7$) and perform modeling of their rest-frame UV to MIR photometry. We find that QGs exhibit a range of MIR spectra that are composed of a stellar continuum and a dust component that is 1-2 orders of magnitude fainter to that of star-forming galaxies. The observed scatter in the MIR spectra, especially at $\\lambda_{\\rm rest} > 5 \\mu$m, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.01601","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2310.01601/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":"2310.01601","created_at":"2026-07-05T07:07:17.349448+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.01601v1","created_at":"2026-07-05T07:07:17.349448+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.01601","created_at":"2026-07-05T07:07:17.349448+00:00"},{"alias_kind":"pith_short_12","alias_value":"OASJSKHLBNFC","created_at":"2026-07-05T07:07:17.349448+00:00"},{"alias_kind":"pith_short_16","alias_value":"OASJSKHLBNFCKZIM","created_at":"2026-07-05T07:07:17.349448+00:00"},{"alias_kind":"pith_short_8","alias_value":"OASJSKHL","created_at":"2026-07-05T07:07:17.349448+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/OASJSKHLBNFCKZIMPJJM6GAN43","json":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43.json","graph_json":"https://pith.science/api/pith-number/OASJSKHLBNFCKZIMPJJM6GAN43/graph.json","events_json":"https://pith.science/api/pith-number/OASJSKHLBNFCKZIMPJJM6GAN43/events.json","paper":"https://pith.science/paper/OASJSKHL"},"agent_actions":{"view_html":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43","download_json":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43.json","view_paper":"https://pith.science/paper/OASJSKHL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.01601&json=true","fetch_graph":"https://pith.science/api/pith-number/OASJSKHLBNFCKZIMPJJM6GAN43/graph.json","fetch_events":"https://pith.science/api/pith-number/OASJSKHLBNFCKZIMPJJM6GAN43/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43/action/storage_attestation","attest_author":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43/action/author_attestation","sign_citation":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43/action/citation_signature","submit_replication":"https://pith.science/pith/OASJSKHLBNFCKZIMPJJM6GAN43/action/replication_record"}},"created_at":"2026-07-05T07:07:17.349448+00:00","updated_at":"2026-07-05T07:07:17.349448+00:00"}