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20002023
most citedThe SDSS-IV MaNGA Sample: Design, Optimization, and Usage Considerations

380 citations · 2.6k across the 60 of their papers we have counts for

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62 papers · 1 filter

astro-ph.GA2023

HI Rich but Low Star Formation galaxies in MaNGA: Physical Properties and Comparison to Control Samples

Anubhav Sharma, Karen L. Masters, David V. Stark +4

Gas rich galaxies are typically star-forming. We make use of HI-MaNGA, a program of HI follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey of the S…

astro-ph.GA2023

Galaxy Zoo DESI: Detailed Morphology Measurements for 8.7M Galaxies in the DESI Legacy Imaging Surveys

Mike Walmsley, Tobias Géron, Sandor Kruk +13

We present detailed morphology measurements for 8.67 million galaxies in the DESI Legacy Imaging Surveys (DECaLS, MzLS, and BASS, plus DES). These are automated measurements made b…

astro-ph.GA2023★ 26 cited

Post-Starburst Properties of Post-Merger Galaxies

Wenhao Li, Preethi Nair, Kate Rowlands +10

Post-starburst galaxies (PSBs) are transition galaxies showing evidence of recent rapid star formation quenching. To understand the role of galaxy mergers in triggering quenching,…

astro-ph.GA2023

Mass and Color Dependence of the Hubble Spiral Sequence

Petra Mengistu, Karen Masters

In the classic Hubble spiral sequence, arm windiness correlates with bulge size; Sa type spiral galaxies with larger bulges also have the most tightly wound spirals. Exceptions to…

astro-ph.GA2023★ 15 cited

The most luminous, merger-free AGN show only marginal correlation with bar presence

Izzy L. Garland, Matthew J. Fahey, Brooke D. Simmons +13

The role of large-scale bars in the fuelling of active galactic nuclei (AGN) is still debated, even as evidence mounts that black hole growth in the absence of galaxy mergers cumul…

astro-ph.GA2023★ 7 cited

Harnessing the Hubble Space Telescope Archives: A Catalogue of 21,926 Interacting Galaxies

David O'Ryan, Bruno Merín, Brooke D. Simmons +13

Mergers play a complex role in galaxy formation and evolution. Continuing to improve our understanding of these systems require ever larger samples, which can be difficult (even im…