{"paper":{"title":"ReveaLLAGN 0: First Look at JWST MIRI data of Sombrero and NGC 1052","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(10) Peking U, (11) U of Amsterdam, (12) U of Nevada, (13) IAC, (14) George Mason U, (15) U of Vienna, (16) TAMU, (17) CAS, (18) U of Southampton, (19) University of Kansas, (20) Montana State U, (21) Michigan State U, (22) U of Connecticut, (23) U of Strasbourg), (2) Vanderbilt U, (3) ESA/ STScI, (4) Cardiff U, (5) MPIA, (6) Penn State U, (7) INAF-IAPS, (8) U of Michigan, (9) Princeton, A. D. Goulding (9), A. Dumont (5), A. E. Reines (20), A. Feldmeier-Krause (5), A. Kirkpatrick (19), A. Prieto (13), A. Seth (1), D. Ohlson (1), E. Gallo (8), F. Yuan (17), G. Van De Ven (15), J. A. Fern\\'andez-Ontiveros (7), J. C. Runnoe (2), J. E. Greene (9), J. L. Walsh (16), J. R. Trump (22), J. Strader (21), K. Goold (1), K. G\\\"ultekin (8), K. T. Voggel (23) ((1) U of Utah, L. C. Ho (10), M. Eracleous (6), M. Molina (1), N. L\\\"utzgendorf (3), N. Neumayer (5), R. Plotkin (12), S. B. Markoff (11), S. Hoenig (18), S. Satyapal (14), T. A. Davis (4), T. Boeker (3)","submitted_at":"2023-07-03T18:00:01Z","abstract_excerpt":"We present the first results from the Revealing Low-Luminosity Active Galactic Nuclei (ReveaLLAGN) survey, a JWST survey of seven nearby LLAGN. We focus on two observations with the Mid-Infrared Instrument's (MIRI) Medium Resolution Spectrograph (MRS) of the nuclei of NGC 1052 and Sombrero (NGC 4594 / M104). We also compare these data to public JWST data of a higher-luminosity AGN, NGC 7319 and NGC 7469. JWST clearly separates the AGN spectrum from the galaxy light even in Sombrero, the faintest target in our survey; the AGN components have very red spectra. We find that the emission-line widt"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.01252","kind":"arxiv","version":2},"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/2307.01252/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"}