1337-MCD, Fort Davis, TX 79734, USA\
    $^{3}$Department of Astronomy, University of Washington Seattle, Seattle, WA 98195, USA\
    $^{4}$University of Wisconsin Oshkosh, Oshkosh, WI 54901, USA\
    $^{5}$NRC Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada
title: 'Chemical abundances in the globular clusters NGC 5024 and NGC 5466 from optical[^2] and infrared spectroscopy'
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stars: abundances – techniques: spectroscopic – globular clusters: individual(NGC 5024) – globular clusters: individual(NGC 5466).

Introduction
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The discovery of the accretion of globular clusters from the Sagittarius dwarf galaxy [@b85], has to the question as to how many globular clusters have been captured by the Milky Way. Multiple studies have looked at the globular cluster systems of the Milky Way to derive an age-metallicity relationship and have come to different conclusions as to which clusters have likely been accreted [@b32; @b33; @b34; @b82]. The question is still open as to which type of clusters are accreted and which form in situ; and furthermore what the fraction of each type is within the Milky Way.

Globular clusters (GC) formed in dwarf galaxies may differ from those found in the Galactic halo, depending on their age and metallicity. Dwarf galaxies show a wide 