| Program | 
      Principal Investigator | 
      Program Title | 
    
    
      | Science Observations Scheduled | 
    
    
      | 16747 | 
      Karl Misselt, University of Arizona | 
      FUV-Optical Spectroscopic Mapping of the PDRs in NGC7023 and The Horsehead | 
    
    
      | 17072 | 
      Matti Dorsch, Universitat Potsdam | 
      From atomic physics to stellar evolution: decoding the heavy-metal subdwarfs with HST | 
    
    
      | 17098 | 
      Adam Riess, The Johns Hopkins University | 
      HST and Gaia, with Light and Distances, a Foundational Legacy of the Distance Ladder | 
    
    
      | 17110 | 
      David Setton, University of Pittsburgh | 
      Post-starbursts from DESI: Timing quenching and morphological transformation at 1 < z < 1.3 | 
    
    
      | 17112 | 
      Nicole Reindl, Universitat Potsdam | 
      A Treasury FUV Survey of the Hottest White Dwarfs | 
    
    
      | 17236 | 
      Matt Nicholl, The Queen's University of Belfast | 
      Tidal disruption events unveiled: understanding their long-term accretion with Chandra and HST | 
    
    
      | 17294 | 
      Amy Simon, NASA Goddard Space Flight Center | 
      Hubble 2020: Outer Planet Atmospheres Legacy (OPAL) Program | 
    
    
      | Calibration Observations Scheduled | 
    
    
      | 16948 | 
      Sophia Medallon, Space Telescope Science Institute | 
      STIS CCD Dark Monitor Part 3 | 
    
    
      | 16950 | 
      Sean Lockwood, Space Telescope Science Institute | 
      STIS CCD Bias and Read Noise Monitor Part 2 | 
    
    
      | 16974 | 
      Meaghan McDonald, Space Telescope Science Institute | 
      CCD Hot Pixel Annealing | 
    
    
      | 17005 | 
      Aidan Pidgeon, Space Telescope Science Institute | 
      WFC3 UVIS CCD Daily Monitor Part 3 | 
    
    
      | 17010 | 
      Mariarosa Marinelli, Space Telescope Science Institute | 
      WFC3 Characterization of UVIS Traps with Charge Injection | 
    
    
      | 17016 | 
      Annalisa Calamida, Space Telescope Science Institute | 
      WFC3 UVIS Time Dependent Sensitivity |