559 citations
- California Institute of TechnologyUS20 papers
- The University of SydneyAU15 papers
- ARC Centre of Excellence for All-sky AstrophysicsAU13 papers
- Australian Astronomical ObservatoryAU13 papers
- International Centre for Radio Astronomy ResearchAU13 papers
- Macquarie UniversityAU13 papers
- The University of Western AustraliaAU13 papers
- Ames Research CenterUS12 papers
- Australian National UniversityAU12 papers
- Jet Propulsion LaboratoryUS12 papers
- UNSW SydneyAU11 papers
- Johns Hopkins UniversityUS10 papers
34 papers
Speckle Interferometry of 25 Gaia Two-Parameter Potential Binaries
Paul McCudden, Russell Genet, John Major +20
Gaia two-parameter (G2P) stars have cumulative errors in parallax and proper motion so great that only their mean positions were reported in DR3. One potential cause of these high…
Evolution of Neptune at Near-Infrared Wavelengths from 1994 through 2022
Erandi Chavez, Imke de Pater, Erin Redwing +15
Using archival near-infrared observations from the Keck and Lick Observatories and the Hubble Space Telescope, we document the evolution of Neptune's cloud activity from 1994 to 20…
Drift Rates of Major Neptunian Features between 2018 and 2021
Erandi Chavez, Erin Redwing, Imke de Pater +13
Using near-infrared observations of Neptune from the Keck and Lick Observatories, and the Hubble Space Telescope in combination with amateur datasets, we calculated the drift rates…
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…
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…
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 …