collaborators

12 papers

astro-ph.EP2026

A Statistical Mechanics Model for Stable Rings Outside the Roche Limit

Jack T. Dinsmore

Stellar occultations have revealed two rings around the dwarf planet Quaoar outside the Roche limit. Simulations suggest that the rings are sustained by large velocity dispersions.…

astro-ph.IM2026

The Lightspeed project: high-speed, ultra-low read noise imaging and polarimetry for the Magellan telescopes

Christopher Layden, Kevin Burdge, John J. Piotrowski +12

Lightspeed will be an ultra-fast (> kHz), ultra-low read noise, multicolor (ugriz + IR) imager for the 6.5 meter Magellan Clay telescope. In a single-channel configuration, Lightsp…

astro-ph.HE2026

Kes 75 with IXPE: Detection of Nebular X-ray Polarization and Change in Pulsar Lightcurve

Josephine Wong, Jack T. Dinsmore, Roger W. Romani +16

We present the first X-ray polarization measurements of the PSR/PWN complex within SNR Kes 75. Two IXPE observations were conducted in October/November 2024 a…

astro-ph.IM2026

proto-Lightspeed: a high-speed, ultra-low read noise imager on the Magellan Clay Telescope

Christopher Layden, Kevin Burdge, Gabor Furesz +9

proto-Lightspeed is a new instrument that has been commissioned on the Nasmyth East port of the Magellan Clay Telescope at Las Campanas Observatory to deliver high-speed optical im…

astro-ph.HE2026

IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

Jack T. Dinsmore, Roger W. Romani, S. Zhang +9

The Lighthouse pulsar (PSR J11016101) sports a bright X-ray trail and filament. The synchrotron emission from both structures is expected to be polarized, with electric vector p…

astro-ph.HE2026

A Physical Model of Pulsar X-ray Filaments

Jack T. Dinsmore, Roger W. Romani

We present a model for pulsar filaments - a class of narrow X-ray nebulae misaligned with the proper motion, powered by pulsar-generated . We suggest that cosmic ray-enhance…