{"paper":{"title":"From the Top to the Bottom of the Main Sequence: A Complete Mass Function of the Young Open Cluster M35","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"((1) Max-Planck-Institut f\\\"ur Astronomie. (2) Universidad Autonoma de Madrid, 2), (3) Harvard--Smithsonian Center for Astrophysics, 4), (4) IPAC, (5) Grenoble (6) Institute for Astronomy, D. Barrado y Navascu\\'es (1, Eduardo L. Mart\\'in (6), Jerome Bouvier (5), John R. Stauffer (3, University of Hawaii)","submitted_at":"2000-11-07T12:00:52Z","abstract_excerpt":"We present very deep and accurate photometry of the open cluster M35 (VRIc filters). We have covered a region of 27.5x27.5 square arcmin.\n  The data range from Ic=12.5 to 23.5 mag, and the color intervals are 0.4\\le(V-I)c\\le3.0, 0.5\\le(R-I)c\\le2.5. Roughly, these values span from 1.6 M_\\odot down to the substellar limit. By using the location of the stars on color-magnitude and color-color diagrams, we have selected candidate members of this cluster. We have merged our sample with previously published data and obtained a color-magnitude diagram for the complete stellar population of the cluste"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0011136","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"}