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ULLYSES and Complementary Surveys of Massive Stars in the Magellanic Clouds

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arxiv 2207.08690 v1 pith:AE6S36AM submitted 2022-07-18 astro-ph.SR astro-ph.GA

classification astro-ph.SRastro-ph.GA
keywords magellanicullysescloudscomplementarymassivespectroscopicstarstogether
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An overview is provided of the scientific goals of the Magellanic Cloud component of the STScI Directors Discretionary UV initiative ULLYSES, together with the complementary spectroscopic survey XShootU (VLT/Xshooter) and other ancillary datasets. Together, ULLYSES and XShootU permit the first comprehensive, homogeneous study of wind densities and velocities in metal-poor massive stars, plus UV/optical spectroscopic libraries for population synthesis models and a large number of interstellar sight-lines towards the Magellanic Clouds.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. SDSS-IV MaStar: Quantification and Abatement of Interstellar Absorption in the Largest Empirical Stellar Spectral Library

    astro-ph.GA 2025-02 conditional novelty 6.0 of 10

    Interstellar calcium and sodium absorption in MaStar is modeled and removed, yielding corrected spectra and simple stellar population templates that reduce a systematic bias in galaxy stellar population analyses.

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