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The Galactic Extinction Horizon with Present and Future Surveys

Published online by Cambridge University Press:  13 February 2024

Dante Minniti Open the ORCID record for Dante Minniti [Opens in a new window]
Dante Minniti*
Affiliation:
Institute of Astrophysics, Faculty of Exact Sciences, Universidad Andres Bello, Santiago, Chile. Vatican Observatory, V00120 Vatican City State, Italy Departamento de Física, Univ. Federal de Santa Catarina, Trindade 88040-900, Florianópolis, SC, Brazil
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Abstract

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We have made a lot of progress in the study of the MW. In spite of this, much of our Galaxy remains unknown, and amazing breakthroughs await to be made in the exploration of the far side of the Galaxy. Focussing on the Galactic extinction horizon problem with current surveys like the Two Micron All-Sky Survey (2MASS) and the Vista Variables in the Via Lactea Survey (VVV) and its extension VVVX, the extinction horizon is a fundamental difficulty, and it is my intention here to reveal how profound is our ignorance, and also to try to suggest ways for improvement with future near-IR Galactic surveys.

Keywords

Milky WayNear-IR surveysStar ClustersInterstellar Medium
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S377: Early Disk-Galaxy Formation from JWST to the Milky Way , December 2022 , pp. 107 - 114
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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