{"paper":{"title":"Dust in three dimensions in the Galactic Plane","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. A. L. Bailer-Jones, C. Waters, J. L. Tonry, K. C. Chambers, K. W. Hodapp, N. Kaiser, R. J. Hanson, R. J. Wainscoat, W. S. Burgett","submitted_at":"2016-09-11T16:15:09Z","abstract_excerpt":"We present three dimensional maps in monochromatic extinction $A_{\\rm 0}$ and the extinction parameter $R_0$ within a few degrees of the Galactic plane. These are inferred using photometry from the Pan-STARRS1 and Spitzer Glimpse surveys of nearly $20$ million stars located in the region $l = 0-250^{\\circ}$ and from $b = -4.5^{\\circ}$ to $b=4.5^{\\circ}$. Given the available stellar number density, we use an angular resolution of $7' \\times 7'$ and steps of $1{\\rm mag}$ in distance modulus. We simultaneously estimate distance modulus and effective temperature $T_{\\rm eff}$ alongside the other p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.03177","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":""},"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"}