(A) The GALEX NUV image of NGC 4141 (color scale; D. C. Martin et al. 2005), overlaid on the GMRT H I 21 cm moment-0 image at an angular resolution of ﹩3\mathop{.}\limits^{^{\prime\prime} }0﹩ (contours). (B) A zoom-in on the maroon dashed square shown in (A), without the H I contours. The location of the eBOSS spectrum is indicated by the arrow. It is clear that only weak NUV emission is detected at this location. In panel (A) and (B), the gray circle in the inset at the bottom left indicates the GMRT synthesized beam.