A spectroscopic survey of EC4, an Extended Cluster in Andromeda's halo
M. L. M. Collins, S. C. Chapman, M. Irwin, R. Ibata, N. F. Martin, A., M. N. Ferguson, A. Huxor, G. F. Lewis, A. D. Mackey, A. W. McConnachie, N., Tanvir

TL;DR
This study spectroscopically characterizes EC4, an extended star cluster in Andromeda's halo, revealing its properties and suggesting it is an extended globular cluster likely associated with Stream Cp.
Contribution
First detailed spectroscopic analysis of EC4, providing insights into its metallicity, kinematics, and possible origin as an extended globular cluster linked to Stream Cp.
Findings
EC4 has a velocity of -287.9 km/s and a low velocity dispersion.
EC4 is metal-poor with [Fe/H] ≈ -1.6.
EC4's properties closely resemble those of Stream Cp.
Abstract
We present a spectroscopic survey of candidate red giant branch stars in the extended star cluster, EC4, discovered in the halo of M31 from our CFHT/MegaCam survey, overlapping the tidal streams, Stream Cp and Stream Cr. These observations used the DEep Imaging Multi-Object Spectrograph (DEIMOS) mounted on the Keck II telescope to obtain spectra around the CaII triplet region with ~1.3 Angstroms resolution. Six stars lying on the red giant branch within 2 core-radii of the centre of EC4 are found to have an average vr=-287.9^{+1.9}_{-2.4}km/s and velocity dispersion of 2.7^{+4.2}_{-2.7}km/s, taking instrumental errors into account. The resulting mass-to-light ratio for EC4 is M/L=6.7^{+15}_{-6.7}Msun/Lsun, a value that is consistent with a globular cluster within the 1 sigma errors we derive. From the summed spectra of our member stars, we find EC4 to be metal-poor, with…
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