activity
20052025
most citedCalibrating Extinction-Free Star Formation Rate Diagnostics with 33GHz Free-Free Emission in NGC6946

859 citations · 2.5k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.IM2025

ADARI: Visualizing the quality of VLT data

C. E. García-Dabó, P. Beirao, Z. Kostrzewa +9

ADARI (Astronomical DAta Reporting Infrastructure) is a system designed for creating graphical reports of astronomical data so that the quality of these products can be assessed. I…

astro-ph.GA2019★ 33 cited

Using [CII] 158 micron Emission From Isolated ISM Phases as a Star-Formation Rate Indicator

Jessica Sutter, Daniel A. Dale, Kevin V. Croxall +17

The brightest observed emission line in many star-forming galaxies is the [CII] 158 micron line, making it detectable up to z~7. In order to better understand and quantify the [CII…

astro-ph.GA2016★ 112 cited

The Spatially Resolved [CII] Cooling Line Deficit in Galaxies

J. D. T. Smith, Kevin Croxall, Bruce Draine +17

We present [CII] 158um measurements from over 15,000 resolved regions within 54 nearby galaxies of the KINGFISH program to investigate the so-called [CII] "line cooling deficit" lo…

astro-ph.GA2016★ 79 cited

The Ionized Gas in Nearby Galaxies as Traced by the [NII] 122 and 205 μm Transitions

R. Herrera-Camus, A. Bolatto, J. D. Smith +20

The [NII] 122 and 205 μm transitions are powerful tracers of the ionized gas in the interstellar medium. By combining data from 21 galaxies selected from the Herschel KINGFISH and…

astro-ph.GA2015

Spatially Resolved Spitzer-IRS Spectral Maps of the Superwind in M82

P. Beirão, L. Armus, M. D. Lehnert +12

We have mapped the superwind/halo region of the nearby starburst galaxy M82 in the mid-infrared with . The spectral regions covered include the H, [NeII]…

astro-ph.GA2015★ 12 cited

Heating and cooling of the neutral ISM in the NGC4736 circumnuclear ring

T. P. R. van der Laan, L. Armus, P. Beirao +12

The manner in which gas accretes and orbits within circumnuclear rings has direct implications for the star formation process. In particular, gas may be compressed and shocked at t…