Image Details
Caption: Figure 9.
Demonstrating Specter’s significant RV signal in the H3 data set. Top: equatorial PMs of CMD-selected giants in H3 within 25° of Specter, with nine selection regions overlaid near Specter’s mean PM. Bottom: galactocentric RV distributions in each PM selection region. Specter stands out as a sharp spike in the RV distribution, and there are no similar spurious spikes in other PM-selected regions.
© 2022. The Author(s). Published by the American Astronomical Society.