Freed, R; Harshaw, R; Genet, Russell M
                            (Ed.)
                        
                    
            
                            We used the Las Cumbres Observatory telescopes to take images of three star systems: WDS 19576+3454, WDS 06043+2327, and WDS 06076+2457, on April 3rd, April 8th, and April 4th, 2024 respectively. We analyzed their astronomical measurements using Afterglow Workbench. For WDS 19576+3454, the position angle was measured to be 265.2° ± 0.12° with an angular separation of 7.38” ± 0.022”. For WDS 06043+2327, the position angle was measured to be 298.5° ± 0.28° with an angular separation of 9.83” ± 0.036”. The new data show that both WDS 19576+3454 and WDS 06043+2327 are consistent with being physical binaries but the parallax distances from the GAIA data suggest the stars in these pairs are too far apart to be gravitationally bound. Thus we conclude these two pairs are likely optical doubles. For WDS 06076+2457, the position angle was measured to be 348.1° ± 0.10° with an angular separation of 7.96” ± 0.023”. The new data we observed, combined with available GAIA data, give evidence that WDS 06076+2457 may be a physical double. 
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