activity
20132026
most citedThe Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey

450 citations · 1.7k across the 32 of their papers we have counts for

collaborators

33 papers

astro-ph.GA2026

Galaxy mergers and disk angular momentum evolution: stellar halos as a critical test

Eric F. Bell, Richard D'Souza, Monica Valluri +1

We investigate the role of hierarchical assembly in the angular momentum (AM) evolution of galaxies using a sample of 471 Milky Way-mass galaxies from the TNG-50 simulation. While…

astro-ph.GA2026★ 1 cited

The role of mass loss in constraining quenching time in dwarf galaxies from AGB and RGB star counts

Paolo Ventura, Richard D'Souza, Flavia Dell'Agli +4

The capability of reconstructing the past star formation history of dwarf elliptical galaxies out of the Local Volume relies on modelling bright stellar populations currently evolv…

astro-ph.GA2025

An integral field spectroscopic study of stellar and ionized gas properties around edge-on disk galaxies in the stellar mass range 9<log M*<11

Guinevere Kauffmann, Richard D'Souza, Antonela Monachesi

We analyze the stellar light, 4000 Angstrom break and emission line profiles of 82 edge-on disk galaxies from the MaNGA survey. We characterize the stellar light profiles perpendic…

astro-ph.GA2025

The Star Formation History and Evolution of the Ultra-Diffuse M81 Satellite F8D1

Adam Smercina, Eric F. Bell, Benjamin F. Williams +15

We present deep HST imaging of one of the nearest ultra-diffuse galaxies (UDGs) outside of the Local Group: F8D1, a satellite of M81 known to be tidally disrupting. UDGs are an eni…

astro-ph.GA2025★ 3 cited

Andromeda XXXV: The Faintest Dwarf Satellite of the Andromeda Galaxy

Jose Marco Arias, Eric F. Bell, Katya Gozman +8

We present the discovery of Andromeda XXXV, the faintest Andromeda satellite galaxy discovered to date, identified as an overdensity of stars in the Pan-Andromeda Archaeological Su…

astro-ph.GA2024★ 4 cited

Exploring the Diversity of Faint Satellites in the M81 Group

Katya Gozman, Eric F. Bell, In Sung Jang +9

In the last decade, we have been able to probe further down the galaxy luminosity function than ever before and expand into the regime of ultra-faint dwarfs (UFDs), which are some…

astro-ph.GA2024

A Timeline of the M81 Group: Properties of the Extended Structures of M82 and NGC 3077

Benjamin N. Velguth, Eric F. Bell, Adam Smercina +8

Mergers of and interactions between galaxies imprint a wide diversity of morphological, dynamical, and chemical characteristics in stellar halos and tidal streams. Measuring these…

astro-ph.GA2024★ 4 cited

First resolved stellar halo kinematics of a MW-mass galaxy outside the Local Group: A flat counter-rotating halo in NGC 4945

Camila Beltrand, Antonela Monachesi, Richard D'Souza +6

Stellar halos of galaxies, primarily formed through the accretion of smaller objects, are important to understand the hierarchical mass assembly of galaxies. However, the inner reg…

astro-ph.GA2024★ 38 cited

The VISTA Variables in the Vía Láctea eXtended (VVVX) ESO public survey: Completion of the observations and legacy

R. K. Saito, M. Hempel, J. Alonso-García +143

The ESO public survey VISTA Variables in the Vía Láctea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from . Upon its conclusion, the c…

astro-ph.GA2024★ 12 cited

Star formation beyond galaxies: widespread in-situ formation of intra-cluster stars

Niusha Ahvazi, Laura V. Sales, Julio F. Navarro +3

We study the fraction of the intra-cluster light (ICL) formed in-situ in the three most massive clusters of the TNG50 simulation, with virial masses M. We…

astro-ph.GA2023

The progenitors of the intra-cluster light and intra-cluster globular clusters in galaxy groups and clusters

Niusha Ahvazi, Laura V. Sales, Jessica E. Doppel +3

We use the IllustrisTNG50 cosmological hydrodynamical simulation, complemented by a catalog of tagged globular clusters, to investigate the properties and build up of two extended…

astro-ph.GA2023

Constraining the assembly time of the stellar haloes of nearby Milky Way-mass galaxies through AGB populations

Benjamin Harmsen, Eric F. Bell, Richard D'Souza +5

The star formation histories (SFHs) of galactic stellar haloes offer crucial insights into the merger history of the galaxy and the effects of those mergers on their hosts. Such me…

astro-ph.GA2023★ 11 cited

Origins of the Evil Eye: M64's Stellar Halo Reveals the Recent Accretion of an SMC-mass Satellite

Adam Smercina, Eric F. Bell, Paul A. Price +9

M64, often called the "Evil Eye" galaxy, is unique among local galaxies. Beyond its dramatic, dusty nucleus, it also hosts an outer gas disk that counter-rotates relative to its st…

astro-ph.GA2023★ 12 cited

Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe

Katya Gozman, Eric F. Bell, Adam Smercina +7

It is not yet settled how the combination of secular processes and merging gives rise to the bulges and pseudobulges of galaxies. The nearby ( 4.2 Mpc) disk galaxy M94 (NGC…

astro-ph.GA2022★ 16 cited

Ultrafaint Dwarf Galaxy Candidates in the M81 Group: Signatures of Group Accretion

Eric F. Bell, Adam Smercina, Paul A. Price +8

The faint and ultrafaint dwarf galaxies in the Local Group form the observational bedrock upon which our understanding of small-scale cosmology rests. In order to understand whethe…

astro-ph.GA2022★ 6 cited

New Globular Cluster Candidates in the M81 group

Jiaming Pan, Eric F. Bell, Adam Smercina +7

The study of outer halo globular cluster (GC) populations can give insight into galaxy merging, globular cluster accretion and the origin of GCs. We use archival Subaru Hyper Supri…

astro-ph.GA2022★ 168 cited

The Global Dynamical Atlas of the Milky Way mergers: Constraints from Gaia EDR3 based orbits of globular clusters, stellar streams and satellite galaxies

Khyati Malhan, Rodrigo A. Ibata, Sanjib Sharma +7

The Milky Way halo was predominantly formed by the merging of numerous progenitor galaxies. However, our knowledge of this process is still incomplete, especially in regard to the…

astro-ph.GA2022★ 40 cited

Uncertainties associated with the backward integration of dwarf satellites using simple parametric potentials

Richard D'Souza, Eric F. Bell

In order to backward integrate the orbits of Milky Way (MW) dwarf galaxies, much effort has been invested in recent years to constrain their initial phase-space coordinates. Yet eq…

astro-ph.GA2021★ 27 cited

Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies

Adam Smercina, Eric F. Bell, Jenna Samuel +1

We investigate whether the considerable diversity in the satellite populations of nearby Milky Way (MW)-mass galaxies is connected with the diversity in their host's merger histori…

astro-ph.GA2021★ 38 cited

The infall of dwarf satellite galaxies are influenced by their host's massive accretions

Richard D'Souza, Eric F. Bell

Recent progress in constraining the massive accretions (>1:10) experienced by the Milky Way (MW) and the Andromeda galaxy (M31) offers an opportunity to understand the dwarf galaxy…

astro-ph.GA2020★ 11 cited

Is NGC 300 a pure exponential disk galaxy?

In Sung Jang, Roelof S. de Jong, I. Minchev +6

NGC 300 is a low-mass disk galaxy in the Sculptor group. In the literature, it has been identified as a pure exponential disk galaxy, as its luminosity profile could be well fitted…

astro-ph.GA2019★ 40 cited

The Saga of M81: Global View of a Massive Stellar Halo in Formation

Adam Smercina, Eric F. Bell, Paul A. Price +7

Recent work has shown that Milky Way-mass galaxies display an incredible range of stellar halo properties, yet the origin of this diversity is unclear. The nearby galaxy M81 cu…

astro-ph.GA2019

Astro2020 Science White Paper: Construction of an L* Galaxy: the Transformative Power of Wide Fields for Revealing the Past, Present and Future of the Great Andromeda System

Karoline M. Gilbert, Erik J. Tollerud, Jay Anderson +34

The Great Andromeda Galaxy (M31) is the nexus of the near-far galaxy evolution connection and a principal data point for near-field cosmology. Due to its proximity (780 kpc), M31 c…

astro-ph.GA2018★ 103 cited

A Lonely Giant: The Sparse Satellite Population of M94 Challenges Galaxy Formation

Adam Smercina, Eric F. Bell, Paul A. Price +5

The dwarf satellites of `giant' Milky Way (MW)-mass galaxies are our primary probes of low-mass dark matter halos. The number and velocities of the satellite galaxies of the MW and…