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20142026
most citedDetection of the LMC-induced sloshing of the Galactic halo

99 citations · 463 across the 20 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.GA2020★ 9 cited

Understanding the velocity distribution of the Galactic Bulge with APOGEE and Gaia

Yingying Zhou, Zhao-Yu Li, Iulia Simion +5

We revisit the stellar velocity distribution in the Galactic bulge/bar region with APOGEE DR16 and {\it Gaia} DR2, focusing in particular on the possible high-velocity (HV) peaks a…

astro-ph.GA2020★ 13 cited

Mapping the tilt of the Milky Way bulge velocity ellipsoids with ARGOS and DR2

Iulia T. Simion, Juntai Shen, Sergey E. Koposov +4

Until the recent advent of Data Release 2 (DR2) and deep multi-object spectroscopy, it has been difficult to obtain 6-D phase space information for large numbers of stars be…

astro-ph.GA2020★ 99 cited

Detection of the LMC-induced sloshing of the Galactic halo

Denis Erkal, Alis J. Deason, Vasily Belokurov +8

A wealth of recent studies have shown that the LMC is likely massive, with a halo mass . One consequence of having such a nearby and massive neighbour is that the…

astro-ph.GA2020★ 22 cited

The Blanco DECam Bulge Survey. I. The Survey Description and Early Results

R. Michael Rich, Christian I. Johnson, Michael Young +18

The Blanco Dark Energy Camera (DECam) Bulge survey is a Vera Rubin Observatory (LSST) pathfinder imaging survey, spanning sq. deg. of the Southern Galactic bulge, $-2^\c…

astro-ph.GA2020★ 34 cited

Blanco DECam Bulge Survey (BDBS) II: Project Performance, Data Analysis, and Early Science Results

Christian I. Johnson, R. Michael Rich, Michael D. Young +7

The Blanco DECam Bulge Survey (BDBS) imaged more than 200 square degrees of the Southern Galactic bulge using the ugrizY filters of the Dark Energy Camera, and produced point sprea…

astro-ph.GA2020★ 30 cited

Is NGC 5824 the Core of the Progenitor of the Cetus Stream?

Jiang Chang, Zhen Yuan, Xiang-Xiang Xue +5

A large number of new members (150) of the Cetus Stream (CS) were identified from their clustering features in dynamical space using 6D kinematic data by combining LAMOST DR5…