activity
20112023
most citedCalibrating Extinction-Free Star Formation Rate Diagnostics with 33GHz Free-Free Emission in NGC6946

859 citations · 2.1k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2023★ 115 cited

PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar

Ryan Chown, Ameek Sidhu, Els Peeters +136

(Abridged) Mid-infrared observations of photodissociation regions (PDRs) are dominated by strong emission features called aromatic infrared bands (AIBs). The most prominent AIBs ar…

astro-ph.IM2022★ 1 cited

Analysis of the ALMA Cycle 8 Distributed Peer Review Process

Jennifer Donovan Meyer, Andrea Corvillón, John M. Carpenter +6

In response to the challenges presented by high reviewer workloads in traditional panel reviews and increasing numbers of submitted proposals, ALMA implemented distributed peer rev…

astro-ph.IM2022★ 1 cited

Update on the Systematics in the ALMA Proposal Review Process after Cycle 8

John M. Carpenter, Andrea Corvillon, Jennifer Donovan Meyer +4

We present an updated analysis of systematics in the Atacama Large Millimeter/submillimeter Array (ALMA) proposal ranks from Carpenter (2020) to include the last two ALMA cycles, w…

astro-ph.GA2020★ 34 cited

Systematic Variations of CO J=2-1/1-0 Ratio in The Barred Spiral Galaxy M83

J. Koda, T. Sawada, K. Sakamoto +18

We present spatial variations of the CO J=2-1/1-0 line ratio in M83 using Total Power array data from ALMA. While the intensities of these two lines correlate tightly, the ratio va…

astro-ph.IM2019★ 6 cited

The CASA software for radio astronomy: status update from ADASS 2019

B. Emonts, R. Raba, G. Moellenbrock +28

CASA, the Common Astronomy Software Applications package, is the primary data processing software for the Atacama Large Millimeter/submillimeter Array (ALMA) and NSF's Karl G. Jans…

astro-ph.GA2019★ 92 cited

Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: The KINGFISH Sample

G. Aniano, B. T. Draine, L. K. Hunt +30

Dust and starlight are modeled for the KINGFISH project galaxies. With data from 3.6 micron to 500 micron, models are strongly constrained. For each pixel in each galaxy we estimat…