SIMBAD references

We present the discovery of a faint, resolved stellar system, BLISS J0321+0438 (BLISS 1), found in Dark Energy Camera data from the first observing run of the Blanco Imaging of the Southern Sky (BLISS) survey. BLISS J0321+0438 (BLISS 1) is located at (α₂₀₀₀,δ₂₀₀₀)=(177○ / . 511,-41○ / . 772) with a heliocentric distance of D_☉=23.7_–1.0^+1.9kpc. It is a faint, M_V=0.0_–0.7^+1.7mag, and compact, r_h=4.1_–1⁺¹pc, system consistent with previously discovered faint halo star clusters. Using data from the second data release of the Gaia satellite, we measure a proper motion of (µ_αcosδ,µ_δ)=(-2.37±0.06,0.16±0.04) mas yr^–1. Combining the available positional and velocity information with simulations of the accreted satellite population of the Large Magellanic Cloud (LMC), we find that it is unlikely that BLISS J0321+0438 (BLISS 1) originated with the LMC.