most citedCHAOS I: Direct Chemical Abundances for HII Regions in NGC 628

181 citations · 466 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2015181 cited

CHAOS I: Direct Chemical Abundances for HII Regions in NGC 628

Danielle A. Berg, Kevin V. Croxall, Evan D. Skillman +3

The CHemical Abundances of Spirals (CHAOS) project leverages the combined power of the Large Binocular Telescope (LBT) with the broad spectral range and sensitivity of the Multi Ob…

astro-ph.GA2014115 cited

Dust continuum emission as a tracer of gas mass in galaxies

Brent A. Groves, Eva Schinnerer, Adam Leroy +8

We use a sample of 36 galaxies from the KINGFISH (Herschel IR), HERACLES (IRAM CO), and THINGS (VLA HI) surveys to study empirical relations between Herschel infrared (IR) luminosi…

astro-ph.GA201431 cited

The Survey of Lines in M31 (SLIM): Investigating the Origins of [CII] Emission

M. J. Kapala, K. Sandstrom, B. Groves +7

The [CII] 158 micron line is one of the strongest emission lines observed in star-forming galaxies, and has been empirically measured to correlate with the star formation rate (SFR…

astro-ph.GA201435 cited

The metallicity of void dwarf galaxies

K. Kreckel, K. Croxall, B. Groves +2

The current Lambda CDM cosmological model predicts that galaxy evolution proceeds more slowly in lower density environments, suggesting that voids are a prime location to search fo…

astro-ph.GA201473 cited

Cool dust heating and temperature mixing in nearby star-forming galaxies

L. K. Hunt, B. T. Draine, S. Bianchi +20

Physical conditions of the interstellar medium in galaxies are closely linked to the ambient radiation field and the heating of dust grains. In order to characterize dust propertie…

astro-ph.GA201431 cited

Discovery of an Overdensity of Lyman-alpha Emitters Around a QSO with the Large Binocular Telescope

Scott M. Adams, Paul Martini, Kevin V. Croxall +2

Measurements of QSO clustering in the SDSS show that QSOs are some of the most highly biased objects in the universe. Their large correlation lengths of $r_0 \sim 20…