Astronomers expect neutron stars—dense cores left behind after massive stars explode—to be common across the Milky Way. However, most neutron stars are difficult to observe because they are effectively invisible under typical observing conditions. A new study published in *Astronomy & Astrophysics* argues that NASA’s upcoming Nancy Grace Roman Space Telescope could improve detection of these elusive objects. The work uses detailed simulations to evaluate how Roman’s observing capabilities could reveal neutron stars that otherwise remain hidden. Rather than changing the underlying expectation of where neutron stars reside in the galaxy, the study focuses on observational strategy and instrument performance, exploring whether Roman’s data could identify neutron stars despite their faintness. NASA’s coverage of the research frames the results as a potential step change for neutron-star surveys, with Roman helping to expand the census of these remnants. Overall, both outlets report that the findings are based on simulations and that the conclusion is tied to Roman’s future mission capabilities, pending actual telescope observations.