Using modern isochrones with customized physics and carefully considered statistical
techniques, we recompute the age distribution for a sample of 91 microlensed dwarfs in the …

Context. The astrometry towards the Galactic bulge is hampered by high stellar crowding
and patchy extinction. This effect is particularly severe for optical surveys such as the …

We present photometric evidence for multiple stellar populations (MPs) in 14 globular
clusters (GCs) toward the southern Galactic bulge. The photometric data come as part of the …

Patchick 99 is a candidate globular cluster located in the direction of the Galactic bulge, with
a proper motion almost identical to the field and extreme field star contamination. A recent …

Abstract The Milky Way Bulge extra-tidal star survey is a spectroscopic survey with the goal
of identifying stripped globular cluster stars from inner Galaxy clusters. In this way, an …

In the context of a project aimed at characterizing the properties of star clusters in the
Galactic bulge, here we present the determination of the internal kinematics and structure of …

We present wide-field, high resolution maps of the color excess for 14 globular clusters
toward the Southern Galactic bulge. The maps were derived using Gaia EDR3 astrometry …

Context. The inner Galaxy is a complex environment, and the relative contributions of
different formation scenarios to its observed morphology and stellar properties are still …

The Blanco DECam Bulge Survey (BDBS) provides near-ultraviolet to near-infrared
photometry for~ 250 million unique stars. By combining BDBS photometry with the latest …

We examined the double red clump (RC) observed in the Galactic bulge, interpreted as a
difference in distance (" X-shaped bulge scenario") or in chemical composition (" multiple …