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David Chuss

Professor/Chair

Villanova University

United States

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About

Professor David Chuss is a faculty member at Villanova University in the United States. His research primarily focuses on astrophysics, with recent articles exploring topics such as magnetic fields in molecular zones, the analysis of polycyclic aromatic hydrocarbons, and advancements in far-infrared polarimetry. He is also involved in projects related to cosmic microwave background polarization and the design of missions aimed at understanding primordial inflation.

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Collaborators (15)

J Michail

Harvard-Smithsonian Center for Astrophysics

UNITED STATES

David Chuss

Research Interests

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About

Articles (30)

The Effects of Cosmic-Ray Protons on Galactic Nonthermal Filaments

Erratum: “Statistical Analysis of Polycyclic Aromatic Hydrocarbons as a Tracer of Anomalous Microwave Emission Using DIRBE Data” (2025, ApJ, 990, 192)

Analyzing Polycyclic Aromatic Hydrocarbons as a Tracer of Anomalous Microwave Emission near the Galactic Plane Using the COSMOGLOBE DIRBE Reduction

Parallel Alignments between Magnetic Fields and Dense Structures in the Central Molecular Zone

Statistical Analysis of Polycyclic Aromatic Hydrocarbons as a Tracer of Anomalous Microwave Emission Using DIRBE Data

SOFIA/HAWC+ Far-infrared Polarimetric Large Area CMZ Exploration Survey. V. The Magnetic Field Strength and Morphology in the Sagittarius C Complex

A Measurement of the Largest-scale CMB E-mode Polarization with CLASS

High-efficiency and Low-noise Detectors for the Upgraded CLASS 90 GHz Focal Plane

The Primordial Inflation Explorer (PIXIE): mission design and science goals

SOFIA Polarization Spectrum of Three Star-forming Clouds

SOFIA/HAWC+ Far-infrared Polarimetric Large-area CMZ Exploration Survey. IV. Relative Magnetic Field Orientation throughout the CMZ

Modeling the Far-infrared Polarization Spectrum of a High-mass Star-forming Cloud

Sensitivity-improved Polarization Maps at 40 GHz with CLASS and WMAP Data

SOFIA/HAWC+ Far-infrared Polarimetric Large-area CMZ Exploration Survey. III. Full Survey Data Set

SOFIA/HAWC+ Far-infrared Polarimetric Large Area CMZ Exploration Survey. II. Detection of a Magnetized Dust Ring in the Galactic Center

CLASS Angular Power Spectra and Map-component Analysis for 40 GHz Observations through 2022

SOFIA/HAWC+ Far-Infrared Polarimetric Large Area CMZ Exploration Survey. I. General Results from the Pilot Program

On-Sky Performance of New 90 GHz Detectors for the Cosmology Large Angular Scale Surveyor (CLASS)

The Origin of Dust Polarization in the Orion Bar

The Strength of the Sheared Magnetic Field in the Galactic’s Circumnuclear Disk

Testing Cosmic Microwave Background Anomalies in E-mode Polarization with Current and Future Data

CLASS Observations of Atmospheric Cloud Polarization at millimeter Wavelengths

CLASS Data Pipeline and Maps for 40 GHz Observations through 2022

Systematic error mitigation for the PIXIE Fourier transform spectrometer

Tracing PAH Emission in λ-Orionis Using COBE/DIRBE Data

Calibration of Transition-edge Sensor (TES) Bolometer Arrays with Application to CLASS

Four-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: On-sky Receiver Performance at 40, 90, 150, and 220 GHz Frequency Bands

SiAl composite feedhorn arrays for astrophysical applications: Cryogenic material properties

Two Year Cosmology Large Angular Scale Surveyor (CLASS) Observations: Long Timescale Stability Achieved with a Front-end Variable-delay Polarization Modulator at 40 GHz

Venus Observations at 40 and 90 GHz with CLASS

Collaborators (15)

J Michail

Brandon S Hensley

Bruno Maffei

Matthew Hankins

Qizhou Zhang

Tobias Marriage

Jens Chluba

John Appel

Charles Bennett

Joseph Eimer

Zhi-Yun Li

Joan Schmelz

Kevin Denis

Mark Morris

Rahul Datta

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