collaborators

7 papers

astro-ph.GA2026

SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane

Giulia Murgia, Ari J. Cukierman, Brandon S. Hensley +29

We present preliminary SPHEREx maps of diffuse Galactic emission tracing polycyclic aromatic hydrocarbons (PAHs) and ionized hydrogen gas, and we study their relationship across th…

astro-ph.GA2026

Searching for the Shortest-wavelength Aromatic Infrared Bands: No Evidence for the Predicted 1.05 m Polycyclic Aromatic Hydrocarbon Feature

Dennis Lee, Brandon S. Hensley, Tzu-Ching Chang +1

Polycyclic aromatic hydrocarbons (PAHs) are responsible for a variety of near- and mid-infrared spectral features in Galactic and extragalactic sources. A feature at 1.05 m ari…

astro-ph.GA2026

SPHEREx Wide-Field Infrared Spectral Mapping of Interstellar Ices and Polycyclic Aromatic Hydrocarbons

Joseph L. Hora, Jinyoung K. Noh, Gary J. Melnick +32

We present some of the first infrared spectral maps acquired by SPHEREx. These maps, which to our knowledge are the largest of their type ever compiled in the near-infrared, reveal…

astro-ph.GA2026

A Detection of Circumgalactic Dust at Megaparsec Scales with Maximum Likelihood Estimation

Jacqueline E. McCleary, Eric M. Huff, James W. Bartlett +1

One of the more surprising astrophysical discoveries of the last decade has been the presence of enormous quantities of dust at megaparsec distances from galaxies, which has import…

astro-ph.CO2025

Feature Intensity Mapping: Polycyclic Aromatic Hydrocarbon Emission from All Galaxies Across Cosmic Time

Yun-Ting Cheng, Brandon S. Hensley, Thomas S. -Y. Lai

Line intensity mapping (LIM) is an emerging technique for probing the aggregate emission of a spectral line from all sources, without requiring individual detections. Through the w…

astro-ph.GA2025

The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance

Dennis Lee, Brandon S. Hensley, Tzu-Ching Chang +1

Accurate correction for extinction by Galactic dust is essential for studying the extragalactic sky. In the low-extinction regions of the Ursa Major molecular cloud complex, we dem…