The DECam local volume exploration survey: Overview and first data release

A Drlica-Wagner, JL Carlin, DL Nidever… - The Astrophysical …, 2021 - iopscience.iop.org
Abstract The DECam Local Volume Exploration survey (DELVE) is a 126-night survey
program on the 4 m Blanco Telescope at the Cerro Tololo Inter-American Observatory in …

Gaia early DR3 systemic motions of Local Group dwarf galaxies and orbital properties with a massive Large Magellanic Cloud

G Battaglia, S Taibi, GF Thomas, TK Fritz - Astronomy & Astrophysics, 2022 - aanda.org
Aims. We perform a comprehensive determination of the systemic proper motions of 74
dwarf galaxies and dwarf galaxy candidates in the Local Group based on Gaia early data …

DELVE 6: An Ancient, Ultra-faint Star Cluster on the Outskirts of the Magellanic Clouds

W Cerny, A Drlica-Wagner, TS Li… - The Astrophysical …, 2023 - iopscience.iop.org
We present the discovery of DELVE 6, an ultra-faint stellar system identified in the second
data release of the DECam Local Volume Exploration (DELVE) survey. Based on a …

Measuring the Milky Way mass distribution in the presence of the LMC

L Correa Magnus, E Vasiliev - Monthly Notices of the Royal …, 2022 - academic.oup.com
The ongoing interaction between the Milky Way (MW) and its largest satellite–the Large
Magellanic Cloud (LMC)–creates a significant perturbation in the distribution and kinematics …

Resolved Dwarf Galaxy Searches within∼ 5 Mpc with the Vera Rubin Observatory and Subaru Hyper Suprime-Cam

B Mutlu-Pakdil, DJ Sand, D Crnojević… - The Astrophysical …, 2021 - iopscience.iop.org
We present a preview of the faint dwarf galaxy discoveries that will be possible with the Vera
C. Rubin Observatory and Subaru Hyper Suprime-Cam in the next decade. In this work, we …

Small-scale stellar haloes: detecting low surface brightness features in the outskirts of Milky Way dwarf satellites

J Jensen, CR Hayes, F Sestito… - Monthly Notices of …, 2024 - academic.oup.com
Dwarf galaxies are valuable laboratories for dynamical studies related to dark matter and
galaxy evolution, yet it is currently unknown just how physically extended their stellar …

Pegasus IV: Discovery and spectroscopic confirmation of an ultra-faint dwarf galaxy in the constellation Pegasus

W Cerny, JD Simon, TS Li… - The Astrophysical …, 2023 - iopscience.iop.org
Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the
Constellation Pegasus - IOPscience This site uses cookies. By continuing to use this site you …

ELVES. IV. The Satellite Stellar-to-halo Mass Relation Beyond the Milky Way

S Danieli, JE Greene, S Carlsten, F Jiang… - The Astrophysical …, 2023 - iopscience.iop.org
Quantifying the connection between galaxies and their host dark matter halos has been key
for testing cosmological models on various scales. Below M⋆∼ 10 9 M⊙, such studies have …

Forward-modelling the luminosity, distance, and size distributions of the Milky Way satellites

V Manwadkar, AV Kravtsov - Monthly Notices of the Royal …, 2022 - academic.oup.com
We use GRUMPY, a simple regulator-type model for dwarf galaxy formation and evolution,
to forward model the dwarf galaxy satellite population of the Milky Way (MW) using the …

Pegasus V/Andromeda XXXIV–a newly discovered ultrafaint dwarf galaxy on the outskirts of Andromeda

MLM Collins, EJE Charles… - Monthly Notices of …, 2022 - academic.oup.com
We report the discovery of an ultrafaint dwarf in the constellation of Pegasus. Pegasus V
(Peg V)/Andromeda XXXIV was initially identified in the public imaging data release of the …