{"paper":{"title":"Multiwavelength Observations of one Galaxy in Marano Field","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"2), China; (2) GEPI, C. J. Cesarsky (5) ((1) NAOC, D. Elbaz (3), D. Marcillac (3), F. Assemat (2), F. Hammer (2), France; (3) CEA, France; (4) Department of Astronomy, Germany), H. Flores (2), L. C. Deng (1), N. Gruel (4), Obs. de Paris-Meudon, Saclay-Service d'Astrophysique, University of Florida, USA; (5) ESO, X. Z. Zheng (2), Y. C. Liang (1","submitted_at":"2005-09-29T03:38:33Z","abstract_excerpt":"We report the multiwavelength observations of one intermediate redshift (z=0.3884) galaxy in the Marano Field. These data include ISOCAM middle infrared, VLT/FORS2 spectroscopic and photometric data, associated with the ATCA 1.4 GHz radio and ROSAT PSPC X-ray observations from literature. The Spectral Energy Distribution obtained by VLT spectroscopy exhibits its early-type galaxy property, while, in the same time, it has obvious [OIII]5007 emission line. The diagnostic diagram from the optical emission line ratios shows its Seyfert galaxy property. Its infrared-radio relation follows the corre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0509867","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"}