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20102026
most citedThe Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library

356 citations · 4.9k across the 111 of their papers we have counts for

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Showing 2018Show all

11 papers · 1 filter

astro-ph.GA2018★ 54 cited

Anomalously low metallicity regions in MaNGA star-forming galaxies: Accretion Caught in Action?

Hsiang-Chih Hwang, Jorge K. Barrera-Ballesteros, Timothy M. Heckman +14

We use data from 1222 late-type star-forming galaxies in the SDSS IV MaNGA survey to identify regions in which the gas-phase metallicity is anomalously-low compared to expectations…

astro-ph.IM2018★ 356 cited

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library

D. S. Aguado, Romina Ahumada, Andres Almeida +230

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years o…

astro-ph.IM2018★ 201 cited

Marvin: A Toolkit for Streamlined Access and Visualization of the SDSS-IV MaNGA Data Set

Brian Cherinka, Brett H. Andrews, José Sánchez-Gallego +11

The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, one of three core programs of the fourth-generation Sloan Digital Sky Survey (SDSS-IV), is producing a massi…

astro-ph.GA2018★ 13 cited

ALMA observations of massive molecular gas reservoirs in dusty early-type galaxies

A. E. Sansom, D. H. W. Glass, G. J. Bendo +9

Unresolved gas and dust observations show a surprising diversity in the amount of interstellar matter in early-type galaxies. Using ALMA observations we resolve the ISM in z0…

astro-ph.GA2018★ 15 cited

Compact star-forming galaxies preferentially quenched to become PSBs in clusters

Miguel Socolovsky, David T. Maltby, Nina A. Hatch +5

We analyse the structure of galaxies with high specific star formation rate (SSFR) in cluster and field environments in the redshift range . Recent studies have shown th…

astro-ph.GA2018★ 33 cited

The relationship between dust and [CI] at z=1 and beyond

N. Bourne, J. S. Dunlop, J. M. Simpson +3

Measuring molecular gas mass is vital for understanding the evolution of galaxies at high redshifts (z1). Most measurements rely on CO as a tracer, but dependences on metalli…