Image Details
Caption: Figure 5.
Top: 1σ–3σ confidence contours derived by fitting a grid of MIST isochrones to the six non-BHB spectroscopic members in Specter. The mean H3 spectroscopic metallicity is overlaid. Bottom: Pan-STARRS CMD of PM-selected members in the inner region of the stream, with the spectroscopic members highlighted as red stars. The overdensity of turnoff stars is best matched by a ∼13 Gyr isochrone and is inconsistent with an isochrone younger than ∼12 Gyr at this metallicity.
© 2022. The Author(s). Published by the American Astronomical Society.