activity
20102024
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations · 12k across the 67 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 40 cited

SDSS IV MaNGA: Deep observations of extra-planar, diffuse ionized gas around late-type galaxies from stacked IFU spectra

A. Jones, G. Kauffmann, R. D'Souza +16

We have conducted a study of extra-planar diffuse ionized gas using the first year data from the MaNGA IFU survey. We have stacked spectra from 49 edge-on, late-type galaxies as a…

astro-ph.IM2016★ 450 cited

The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey

David R. Law, Brian Cherinka, Renbin Yan +26

Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs in the four…

astro-ph.GA2016★ 360 cited

SDSS-IV MaNGA IFS Galaxy Survey --- Survey Design, Execution, and Initial Data Quality

Renbin Yan, Kevin Bundy, David R. Law +47

The MaNGA Survey (Mapping Nearby Galaxies at Apache Point Observatory) is one of three core programs in the Sloan Digital Sky Survey IV. It is obtaining integral field spectroscopy…

astro-ph.GA2016★ 115 cited

Equilibrium and Sudden Events in Chemical Evolution

David H. Weinberg, Brett H. Andrews, Jenna Freudenburg

We present new analytic solutions for one-zone (fully mixed) chemical evolution models and explore their implications. In contrast to existing analytic models, we incorporate a rea…

astro-ph.GA2016★ 171 cited

Inflow, Outflow, Yields, and Stellar Population Mixing in Chemical Evolution Models

Brett H. Andrews, David H. Weinberg, Ralph Schönrich +1

Chemical evolution models are powerful tools for interpreting stellar abundance surveys and understanding galaxy evolution. However, their predictions depend heavily on the treatme…

astro-ph.GA2016★ 58 cited

A Recalibration of Strong Line Oxygen Abundance Diagnostics via the Direct Method and Implications for the High Redshift Universe

Jonathan S. Brown, Paul Martini, Brett H. Andrews

We use direct method oxygen abundances in combination with strong optical emission lines, stellar masses (), and star formation rates (SFRs) to recalibrate the N2, O3N2,…