activity
20092020
most citedThe Sydney-AAO Multi-object Integral field spectrograph (SAMI)

570 citations · 1.3k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2020★ 17 cited

HAWC+ Far-Infrared Observations of the Magnetic Field Geometry in M51 and NGC 891

Terry Jay Jones, Jin-Ah Kim, C. Darren Dowell +29

SOFIA HAWC+ polarimetry at $154~\micron$ is reported for the face-on galaxy M51 and the edge-on galaxy NGC 891. For M51, the polarization vectors generally follow the spiral patter…

astro-ph.GA2019★ 23 cited

SOFIA/HAWC+ traces the magnetic fields in NGC 1068

E. Lopez-Rodriguez, C. D. Dowell, T. J. Jones +21

We report the first detection of galactic spiral structure by means of thermal emission from magnetically aligned dust grains. Our 89 m polarimetric imaging of NGC 1068 with the…

astro-ph.GA2019★ 48 cited

The far-infrared polarization spectrum of Rho Ophiuchi A from HAWC+/SOFIA observations

Fabio P. Santos, David T. Chuss, C. Darren Dowell +23

We report on polarimetric maps made with HAWC+/SOFIA toward Rho Oph A, the densest portion of the Rho Ophiuchi molecular complex. We employed HAWC+ bands C (89 m) and D (154 …

astro-ph.GA2018★ 38 cited

SOFIA Far Infrared Imaging Polarimetry of M82 and NGC 253: Exploring the Super-Galactic Wind

Terry Jay Jones, C. Darren Dowell, Enrique Lopez Rodriguez +22

We present Far-Infrared polarimetry observations of M82 at 53 and and NGC 253 at , which were taken with HAWC+ in polarimetry mode on the Stratospheric Ob…

astro-ph.GA2018★ 107 cited

HAWC+/SOFIA Multiwavelength Polarimetric Observations of OMC-1

David T. Chuss, B-G Andersson, John Bally +35

We report new polarimetric and photometric maps of the massive star-forming region OMC-1 using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy (SOFIA).…

astro-ph.EP2018★ 5 cited

Dust Production Rates in the Fomalhaut Debris Disk from SOFIA/FORCAST Mid-infrared Imaging

J. D. Adams, T. L. Herter, R. M. Lau +2

We present the first spatially resolved mid-infrared (37.1 m) image of the Fomalhaut debris disk. We use PSF fitting and subtraction to distinctly measure the flux from the unre…