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Overview of the SDSS-V Magellanic Genesis Survey

  • Authors: David L. Nidever, Danny Horta, Steven R. Majewski, Andres Almeida, Joshua T. Povick, Slater J. Oden, Óscar Jiménez-Arranz, Guy Stringfellow, S. Drew Chojnowski, Roeland van der Marel, Lara Cullinane, Bruno Dias, Jennifer Johnson, John Donor, Maria-Rosa Cioni, Chandreyee Maitra, Juna Kollmeier, Andrew Tkachenko

David L. Nidever et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

Map of the SDSS-IV/APOGEE-2S MC survey fields (blue) shown on top of the V. A. Belokurov & D. Erkal (2019) RGB star density map (grayscale), projected in the Magellanic Stream coordinate system (D. L. Nidever et al. 2008). While the SDSS-IV data sample a large radial and azimuthal range in the MCs, they only fill 33% of the area in the LMC and SMC main bodies. Conversely, the MGS covers the entire Magellanic system.

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