629 citations · 4.6k across the 83 of their papers we have counts for
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Infra-Red Emission from Cold Gas Dusty Disks in Massive Ellipticals
Zhaoming Gan, Brandon S. Hensley, Jeremiah P. Ostriker +3
What is the expected infrared output of elliptical galaxies? Here we report the latest findings obtained in this high time resolution (~10 years) and high spatial resolution (2.5 p…
Resolved observations at 31 GHz of spinning dust emissivity variations in Oph
Carla Arce-Tord, Matias Vidal, Simon Casassus +9
The Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the Cosmic Background Imager (CBI). Here we present 4.5 arcmin observations wit…
Mapping the Magnetic Interstellar Medium in Three Dimensions Over the Full Sky with Neutral Hydrogen
S. E. Clark, Brandon S. Hensley
Recent analyses of 21-cm neutral hydrogen (HI) emission have demonstrated that HI gas is organized into linear filamentary structures that are preferentially aligned with the local…
An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission
Brandon S. Hensley, Cheng Zhang, James J. Bock
It is well known that aligned, aspherical dust grains emit polarized radiation and that the degree of polarization depends on the angle between the interstellar magnetic field…
PICO: Probe of Inflation and Cosmic Origins
S. Hanany, M. Alvarez, E. Artis +79
The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. W…
Astro2020 APC White Paper: The need for better tools to design future CMB experiments
G. Rocha, A. J. Banday, R. Belen Barreiro +27
This white paper addresses key challenges for the design of next-decade Cosmic Microwave Background (CMB) experiments, and for assessing their capability to extract cosmological in…
The Simons Observatory: Astro2020 Decadal Project Whitepaper
The Simons Observatory Collaboration, Maximilian H. Abitbol, Shunsuke Adachi +280
The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough…
A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments
Guochao Sun, Brandon S. Hensley, Tzu-Ching Chang +2
Line intensity mapping (LIM) is a promising approach to study star formation and the interstellar medium (ISM) in galaxies by measuring the aggregate line emission from the entire…
Extreme Starlight Polarization in a Region with Highly Polarized Dust Emission
G. V. Panopoulou, B. S. Hensley, R. Skalidis +2
Galactic dust emission is polarized at unexpectedly high levels, as revealed by Planck. The origin of the observed polarization fractions can be identified by charact…
Studying Magnetic Fields in Star Formation and the Turbulent Interstellar Medium
Laura Fissel, Charles L. H. Hull, Susan E. Clark +10
Understanding the physics of how stars form is a highly-prioritized goal of modern Astrophysics, in part because star formation is linked to both galactic dynamics on large scales…
PICO: Probe of Inflation and Cosmic Origins
Shaul Hanany, Marcelo Alvarez, Emmanuel Artis +79
The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce f…