activity
19952024
most citedFirst Results from SPARO: Evidence for Large-Scale Toroidal Magnetic Fields in the Galactic Center

103 citations · 510 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.IM2024★ 5 cited

The BLAST Observatory: A Sensitivity Study for Far-IR Balloon-borne Polarimeters

The BLAST Observatory Collaboration, Gabriele Coppi, Simon Dicker +21

Sensitive wide-field observations of polarized thermal emission from interstellar dust grains will allow astronomers to address key outstanding questions about the life cycle of ma…

astro-ph.GA2017★ 3 cited

Measuring filament orientation: a new quantitative, local approach

C. -E. Green, J. R. Dawson, M. R. Cunningham +3

The relative orientation between filamentary structures in molecular clouds and the ambient magnetic field provides insight into filament formation and stability. To calculate the…

astro-ph.IM2017★ 9 cited

Removing visual bias in filament identification: a new goodness-of-fit measure

C. -E. Green, M. R. Cunningham, J. R. Dawson +3

Different combinations of input parameters to filament identification algorithms, such as Disperse and FilFinder, produce numerous different output skeletons. The skeletons are a o…

astro-ph.GA2014★ 15 cited

Tracing H2 column density with atomic carbon (CI) and CO isotopologues

N. Lo, M. R. Cunningham, P. A. Jones +6

We present first results of neutral carbon ([CI], 3P1 - 3P0 at 492 GHz) and carbon monoxide (13CO, J = 1 - 0) mapping in the Vela Molecular Ridge cloud C (VMR-C) and G333 giant mol…

astro-ph.GA2011★ 69 cited

Magnetic Field Structure around Low-Mass Class 0 Protostars: B335, L1527 and IC348-SMM2

J. A. Davidson, G. Novak, T. G. Matthews +6

We report new 350 micron polarization observations of the thermal dust emission from the cores surrounding the low-mass, Class 0 YSOs L1527, IC348-SMM2 and B335. We have inferred m…

astro-ph.GA2011★ 22 cited

A Constraint on the Organization of the Galactic Center Magnetic Field Using Faraday Rotation

C. J. Law, M. A. Brentjens, G. Novak

We present new 6 and 20 cm Very Large Array (VLA) observations of polarized continuum emission of roughly 0.5 square degrees of the Galactic center (GC) region. The 6 cm observatio…