26 citations · 26 across the 7 of their papers we have counts for
7 papers
Cool dark gas in Cygnus X: The first large-scale mapping of low-frequency carbon recombination lines
Kimberly L. Emig, Pedro Salas, Loren D. Anderson +14
Understanding the transition from atomic gas to molecular gas is critical to explain the formation and evolution of molecular clouds. However, the gas phases involved, cold HI and…
Low-frequency absorption and radio recombination line features of the Galactic Center Lobe
Natasha Hurley-Walker, L. D. Anderson, M. Luisi +6
The Galactic center lobe (GCL) is a object located north of the Galactic center. In the mid-infrared (MIR), the GCL appears as two 8.0-micron filaments that roughly…
The Galactic Center Lobe as an HII Region
L. D. Anderson, Matteo Luisi, B. Liu +5
The Galactic center lobe (GCL) is an object ~1° across that is located north of the Galactic center. In the mid-infrared (MIR) the GCL appears as two 8.0m filaments between whic…
Methods for Averaging Spectral Line Data
L. D. Anderson, B. Liu, Dana S. Balser +5
The ideal spectral averaging method depends on one's science goals and the available information about one's data. Including low-quality data in the average can decrease the signal…
The GBT Diffuse Ionized Gas Survey (GDIGS): Discrete Sources
Dylan J. Linville, Matteo Luisi, L. D. Anderson +6
The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) traces ionized gas in the Galactic midplane by observing radio recombination line (RRL) emission from 4-8 GHz. The…
Stellar feedback and triggered star formation in the prototypical bubble RCW 120
Matteo Luisi, Loren D. Anderson, Nicola Schneider +17
Radiative and mechanical feedback of massive stars regulates star formation and galaxy evolution. Positive feedback triggers the creation of new stars by collecting dense shells of…
The GBT Diffuse Ionized Gas Survey (GDIGS): Survey Overview and First Data Release
L. D. Anderson, Matteo Luisi, Bin Liu +6
The Green Bank Telescope (GBT) Diffuse Ionized Gas Survey (GDIGS) traces ionized gas in the Galactic midplane by measuring GHz radio recombination line (RRL) emission. The nom…