{"paper":{"title":"Recent star formation in the inner Galactic Bulge seen by ISOGAL. I - Classification of bright mid-IR sources in a test field","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"2), (2) MPIfR, (3) SAAO, 4), (4) Obs. Besancon, (5) AFRL, (6) AFRL, A. Omont (1), France, F. Schuller (1, Germany, I. S. Glass (3), M. P. Egan (5), M. Schultheis (1, ODASD, S. D. Price (6) ((1) IAP, South Africa, SVD, USA, USA)","submitted_at":"2006-03-21T18:57:00Z","abstract_excerpt":"Context: The stellar populations in the central region of the Galaxy are poorly known because of the high visual extinction and very great source density in this direction.\n  Aims: To use recent infrared surveys for studying the dusty stellar objects in this region.\n  Methods: We analyse the content of a 20x20 arcmin^2 field centred at (l,b)=(-0.27,-0.06) observed at 7 and 15 microns as part of the ISOGAL survey. These ISO observations are more than an order of magnitude better in sensitivity and spatial resolution than the IRAS observations. The sources are cross-associated with other catalog"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0603576","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"}