activity
20032023
most citedDust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

1.1k citations · 15.3k across the 193 of their papers we have counts for

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Showing 2017Show all

15 papers · 1 filter

astro-ph.GA2017★ 85 cited

CHANG-ES IX: Radio scale heights and scale lengths of a consistent sample of 13 spiral galaxies seen edge-on and their correlations

Marita Krause, Judith Irwin, Theresa Wiegert +14

The vertical halo scale height is a crucial parameter to understand the transport of cosmic-ray electrons (CRE) and their energy loss mechanisms in spiral galaxies. Until now, the…

astro-ph.GA2017★ 246 cited

Galaxy growth in a massive halo in the first billion years of cosmic history

D. P. Marrone, J. S. Spilker, C. C. Hayward +34

According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in reg…

astro-ph.IM2017★ 1 cited

Host galaxies and relativistic ejecta of compact binary mergers in the ngVLA era

A. Corsi, D. A. Frail, B. J. Owen +3

We present the results of a community study aimed at exploring some of the scientific opportunities that the next generation Very Large Array (ngVLA) could open in the field of mul…

astro-ph.GA2017★ 32 cited

The Star Formation in Radio Survey: Jansky Very Large Array 33 GHz Observations of Nearby Galaxy Nuclei and Extranuclear Star-Forming Regions

E. J. Murphy, D. Dong, E. Momjian +5

We present 33 GHz imaging for 112 pointings towards galaxy nuclei and extranuclear star-forming regions at 2" resolution using the Karl G. Jansky Very Large Array (VLA) as…

astro-ph.HE2017★ 48 cited

The Radio Synchrotron Background: Conference Summary and Report

J. Singal, J. Haider, M. Ajello +20

We summarize the radio synchrotron background workshop that took place July 19-21, 2017 at the University of Richmond. This first scientific meeting dedicated to the topic was conv…

astro-ph.GA2017★ 5 cited

Galaxies into the Dark Ages

C. L. Carilli, E. J. Murphy, A. Ferrara +1

We consider the capabilities of current and future large facilities operating at 2\,mm to 3\,mm wavelength to detect and image the [CII] 158\,m line from galaxies into the cosmi…