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Interstellar extinction towards the inner Galactic Bulge

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arxiv astro-ph/9908349 v1 pith:G3GYTH2M submitted 1999-08-31 astro-ph

M. Schultheis , S. Ganesh , G. Simon , A. Omont , C. Alard , J. Borsenberger , E. Copet , N. Epchtein
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P. Fouque H. Habing
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classification astro-ph
keywords bulgeextinctiongalacticinnermicronagreementapproxbands
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DENIS observations in the J (1.2 micron) and K_S (2.15 micron) bands together with isochrones calculated for the RGB and AGB phase are used to draw an extinction map of the inner Galactic Bulge. The uncertainty in this method is mainly limited by the optical depth of the Bulge itself. A comparison with fields of known extinction shows a very good agreement. We present an extinction map for the inner Galactic Bulge (approx. 20 sq. deg.)

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Cited by 1 Pith paper

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  1. GSED: The Galactic Stellar Extinction Database

    astro-ph.GA 2026-06 unverdicted novelty 5.0 of 10

    GSED unifies six heterogeneous 3D extinction datasets into a single homogenized catalogue of over 1.9 billion entries via a six-layer MLP and provides a real-time coordinate-based query service.

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