ADS arXiv A minor work as part of the Herschel Hi-Gal early science special issue.
Articles in the publications category
The Bolocam Galactic Plane Survey IV: λ = 1.1 and 0.35 mm Dust Continuum Emission in the Galactic Center Region
The Bolocam Galactic Plane Survey. III. Characterizing Physical Properties of Massive Star-forming Regions in the Gemini OB1 Molecular Cloud
ADS arXiv As with the other Bolocam papers, I reduced the data. All of the analysis work was done by Miranda. Because of Gem OB1's known distance (~2 kpc), it was possible to derive the physical properties of all of the 34 BGPS sources. NH3 temperatures and line widths were combined to measure total dust mass, density, and virial parameter. This paper is the best characterization of "typical" BGPS sources, at least for the outer galaxy.
The Bolocam Galactic Plane Survey. II. Catalog of the Image Data
ADS arXiv My primary contribution to this work was reducing the data from which catalogs were derived. As part of this process, I also made the noise maps that were part of the Bolocat process and did some of the by-eye verification work. Bolocat extracted >8000 sources from the BGPS using a watershed decomposition method. Most of these sources have now been observed with the HHT in HCO+ and N2H+ to determine their velocity and kinematic distance.
The Bolocam Galactic Plane Survey: Survey Description and Data Reduction
ADS arXiv I wrote about half of this paper and did the majority of the work described, including writing the data pipeline and reducing all of the data. However, there was a good deal of work done on the project before I showed up on the scene. The paper describes the methods by which we reduced the Bolocam observations of the Northern Galactic Plane and the tests we ran to determine how well we recovered the "true" sky structure.
A spatially resolved study of photoelectric heating and [C II] cooling in the LMC. Comparison with dust emission as seen by SAGE
Kinematics and H2 morphology of the multipolar post-AGB star IRAS 16594-4656
ADS arXiv An interesting examination of the morphology of the circumstellar material around IRAS 16594-4656. I did this work with Toshiya Ueta at the University of Denver. My contribution was azimuthally interpolating the 7 high-resolution long-slit spectra onto a 3-dimensional grid, creating a full 3D position-velocity cube. I used the Perl Data Language, which I have since abandoned.
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