We present structural parameters from a wide-field homogeneous imaging survey of Milky Way satellites carried out with the MegaCam imagers on the 3.6 m Canada-France-Hawaii Telescope and 6.5 m Magellan-Clay telescope. Our survey targets an unbiased sample of "outer halo" satellites (i.e., substructures having galactocentric distances greater than 25 kpc) and includes classical dSph galaxies, ultra-faint dwarfs, and remote globular clusters. We combine deep, panoramic gr imaging for 44 satellites and archival gr imaging for 14 additional objects (primarily obtained with the DECam instrument as part of the Dark Energy Survey) to measure photometric and structural parameters for 58 outer halo satellites. This is the largest and most uniform an...
We infer the normalization and the radial and angular distributions of the number density of satelli...
Photometric data from the Xuyi Schmidt Telescope Photometric Survey of the Galactic Anticentre (XSTP...
Strong gravitational lensing by groups or clusters of galaxies provides a powerful technique to meas...
We present structural parameters from a wide-field homogeneous imaging survey of Milky Way satellite...
We present structural parameters from a wide-field homogeneous imaging survey of Milky Way satellite...
We describe a deep, systematic imaging study of satellites in the outer halo of the Milky Way. Our s...
We describe a deep, systematic imaging study of satellites in the outer halo of the Milky Way. Our s...
In this work, we use structural properties of the Milky Way's outer halo (R G > 25 kpc) satellite...
Abstract: This study presents a tomographic survey of a subset of the outer halo (10-40 kpc) drawn f...
We present a large area photometric survey of the Ursa Minor dSph. We identify UMi giant star candid...
We present a homogeneous study of blue straggler stars across 10 outer halo globular clusters, 3 cla...
We have measured the amount of kinematic substructure in the Galactic halo using the final data set ...
We derive the structural parameters of the recently discovered very low luminosity Milky Way satelli...
We report the results of a systematic photometric survey of the peripheral regions of a sample of 14...
We have measured the amount of kinematic substructure in the Galactic halo using the final data set ...
We infer the normalization and the radial and angular distributions of the number density of satelli...
Photometric data from the Xuyi Schmidt Telescope Photometric Survey of the Galactic Anticentre (XSTP...
Strong gravitational lensing by groups or clusters of galaxies provides a powerful technique to meas...
We present structural parameters from a wide-field homogeneous imaging survey of Milky Way satellite...
We present structural parameters from a wide-field homogeneous imaging survey of Milky Way satellite...
We describe a deep, systematic imaging study of satellites in the outer halo of the Milky Way. Our s...
We describe a deep, systematic imaging study of satellites in the outer halo of the Milky Way. Our s...
In this work, we use structural properties of the Milky Way's outer halo (R G > 25 kpc) satellite...
Abstract: This study presents a tomographic survey of a subset of the outer halo (10-40 kpc) drawn f...
We present a large area photometric survey of the Ursa Minor dSph. We identify UMi giant star candid...
We present a homogeneous study of blue straggler stars across 10 outer halo globular clusters, 3 cla...
We have measured the amount of kinematic substructure in the Galactic halo using the final data set ...
We derive the structural parameters of the recently discovered very low luminosity Milky Way satelli...
We report the results of a systematic photometric survey of the peripheral regions of a sample of 14...
We have measured the amount of kinematic substructure in the Galactic halo using the final data set ...
We infer the normalization and the radial and angular distributions of the number density of satelli...
Photometric data from the Xuyi Schmidt Telescope Photometric Survey of the Galactic Anticentre (XSTP...
Strong gravitational lensing by groups or clusters of galaxies provides a powerful technique to meas...