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robostrategy: Field and Target Assignment Optimization in the Sloan Digital Sky Survey V

  • Authors: Michael R. Blanton, Joleen K. Carlberg, Tom Dwelly, Ilija Medan, S. Drew Chojnowski, Kevin Covey, Megan C. Davis, John Donor, Pramod Gupta, Alexander P. Ji, Jennifer A. Johnson, Juna A. Kollmeier, José Sanchez-Gallego, Conor Sayres, Eleonora Zari

Michael R. Blanton et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 8.

Field coverage in equatorial coordinates, including the all-sky tiling plus specially defined fields. R.A. = 270° is at the center, and R.A. increases to the left. The difference in size between the LCO fields (in the south) and the APO fields (in the north) is apparent. Blue fields have constraints on their cadence imposed by BHM; from lightest to darkest below they are AQMES Wide dark_1x4 fields, AQMES Wide dark_2x4 fields, AQMES Medium dark_10x4 fields, and RM fields.

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