| Program | 
      Principal Investigator | 
      Program Title | 
    
    
      | Science Observations Scheduled | 
    
    
      | 16489 | 
      Noel Castro Segura, University of Southampton | 
      Outflow Legacy Accretion Survey: unveiling the wind driving mechanism in BHXRBs | 
    
    
      | 17092 | 
      Kimberly Ward-Duong, Smith College | 
      Calibrating STIS Coronagraphic Spectroscopy for High Contrast Observations | 
    
    
      | 17110 | 
      David Setton, University of Pittsburgh | 
      Post-starbursts from DESI: Timing quenching and morphological transformation at 1 < z < 1.3 | 
    
    
      | 17115 | 
      David Bowen, Princeton University | 
      The Circumgalactic Medium of Dwarf Galaxy Pairs | 
    
    
      | 17147 | 
      Claudia Scarlata, University of Minnesota - Twin Cities | 
      The Parallel Ionizing Emissivity Survey | 
    
    
      | 17308 | 
      Cameron Lemon, Ecole Polytechnique Federale de Lausanne | 
      An HST Gap Program for lensed Quasars | 
    
    
      | 17310 | 
      Michael Koss, Eureka Scientific Inc. | 
      A Blue Gap Survey of Nearby Active Galaxies | 
    
    
      | 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 | 
    
    
      | 17002 | 
      Harish Khandrika, Space Telescope Science Institute | 
      WFC3 UVIS Bowtie Monitor | 
    
    
      | 17005 | 
      Aidan Pidgeon, Space Telescope Science Institute | 
      WFC3 UVIS CCD Daily Monitor Part 3 | 
    
    
      | 17006 | 
      Aidan Pidgeon, Space Telescope Science Institute | 
      WFC3 UVIS CCD Unflashed (CTE) Monitor | 
    
    
      | 17011 | 
      Frederick Dauphin, Space Telescope Science Institute | 
      WFC3 IR Dark Monitor | 
    
    
      | 17022 | 
      Frederick Dauphin, Space Telescope Science Institute | 
      WFC3 CSM Monitor with Earth Flats |