activity
19942023
most citedA Universal Density Profile from Hierarchical Clustering

9.9k citations · 53.9k across the 254 of their papers we have counts for

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Showing 2020Show all

15 papers · 1 filter

astro-ph.GA2020★ 39 cited

The Pristine survey -- XII: Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy

Collin L. Kielty, Kim A. Venn, Federico Sestito +16

High-resolution optical spectra of 30 metal-poor stars selected from the \Pristine\ survey are presented, based on observations taken with the Gemini Observatory GRACES spectrograp…

astro-ph.GA2020★ 77 cited

Revisiting the tension between fast bars and the CDM paradigm

Francesca Fragkoudi, Robert J. J. Grand, Ruediger Pakmor +5

The pattern speed with which galactic bars rotate is intimately linked to the amount of dark matter in the inner regions of their host galaxies. In particular, dark matter haloes a…

astro-ph.GA2020★ 42 cited

Magellanic satellites in CDM cosmological hydrodynamical simulations of the Local Group

Isabel M. E. Santos-Santos, Azadeh Fattahi, Laura V. Sales +1

We use the APOSTLE CDM cosmological hydrodynamical simulations of the Local Group to study the recent accretion of massive satellites into the halo of Milky Way (MW)-sized galax…

astro-ph.GA2020★ 95 cited

The asymptotic tidal remnants of cold dark matter subhalos

Raphaël Errani, Julio F. Navarro

We use N-body simulations to study the evolution of cuspy cold dark matter (CDM) halos in the gravitational potential of a massive host. Tidal mass losses reshape CDM halos, leavin…

astro-ph.GA2020★ 36 cited

Globular clusters as tracers of the dark matter content of dwarfs in galaxy clusters

Jessica E. Doppel, Laura V. Sales, Julio F. Navarro +3

Globular clusters (GCs) are often used to estimate the dark matter content of galaxies, especially dwarfs, where other kinematic tracers are lacking. These estimates typically assu…

astro-ph.GA2020★ 62 cited

Exploring the origin of low-metallicity stars in Milky Way-like galaxies with the NIHAO-UHD simulations

Federico Sestito, Tobias Buck, Else Starkenburg +6

The kinematics of the most metal-poor stars provide a window into the early formation and accretion history of the Milky Way. Here, we use 5~high-resolution cosmological zoom-in si…

astro-ph.GA2020★ 33 cited

The hidden past of M92: Detection and characterization of a newly formed 17° long stellar stream using the Canada-France Imaging Survey

Guillaume F. Thomas, Jaclyn Jensen, Alan McConnachie +17

We present an analysis of the structure, kinematics and orbit of a newly found stellar stream emanating from the globular cluster M92 (NGC 6341). This stream was discovered in an i…

astro-ph.SR2020★ 117 cited

The -Process Alliance: Fourth Data Release from the Search for -Process-Enhanced Stars in the Galactic Halo

Erika M. Holmbeck, Terese T. Hansen, Timothy C. Beers +22

This compilation is the fourth data release from the -Process Alliance (RPA) search for -process-enhanced stars, and the second release based on "snapshot" high-resolution ($…

astro-ph.GA2020★ 57 cited

The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way

Anke Arentsen, Else Starkenburg, Nicolas F. Martin +19

Metal-poor stars are important tools for tracing the early history of the Milky Way, and for learning about the first generations of stars. Simulations suggest that the oldest meta…

astro-ph.GA2020★ 5 cited

Observational constraints on the slope of the radial acceleration relation at low accelerations

Kyle A. Oman, Margot M. Brouwer, Aaron D. Ludlow +1

The radial acceleration relation (RAR) locally relates the `observed' acceleration inferred from the dynamics of a system to the acceleration implied by its baryonic matter distrib…

astro-ph.GA2020★ 34 cited

The Pristine Dwarf-Galaxy survey -- III. Revealing the nature of the Milky Way globular cluster Sagittarius II

Nicolas Longeard, Nicolas Martin, Rodrigo Ibata +13

We present a new spectroscopic study of the faint Milky Way satellite Sagittarius II. Using multi-object spectroscopy from the Fibre Large Array Multi Element Spectrograph, we supp…

astro-ph.GA2020★ 32 cited

The RAdial Velocity Experiment (RAVE): Parameterisation of RAVE spectra based on convolutional neural networks

G. Guiglion, G. Matijevic, A. B. A. Queiroz +22

In the context of large spectroscopic surveys of stars, data-driven methods are key in deducing physical parameters for millions of spectra in a short time. Convolutional neural ne…

astro-ph.GA2020★ 62 cited

The Edge of the Galaxy

Alis J. Deason, Azadeh Fattahi, Carlos S. Frenk +5

We use cosmological simulations of isolated Milky Way-mass galaxies, as well as Local Group analogues, to define the "edge" -- a caustic manifested in a drop in density or radial v…

astro-ph.SR2020★ 167 cited

The Sixth Data Release of the Radial Velocity Experiment (RAVE) -- II: Stellar Atmospheric Parameters, Chemical Abundances and Distances

Matthias Steinmetz, Guillaume Guiglion, Paul J. McMillan +58

We present part 2 of the 6th and final Data Release (DR6 or FDR) of the Radial Velocity Experiment (RAVE), a magnitude-limited (9<I<12) spectroscopic survey of Galactic stars rando…

astro-ph.SR2020★ 165 cited

The Sixth Data Release of the Radial Velocity Experiment (RAVE) -- I: Survey Description, Spectra and Radial Velocities

Matthias Steinmetz, Gal Matijevic, Harry Enke +59

The Radial Velocity Experiment (RAVE) is a magnitude-limited (9<I<12) spectroscopic survey of Galactic stars randomly selected in the southern hemisphere. The RAVE medium-resolutio…