activity
20242026
collaborators

26 papers

astro-ph.SR2026

A survey of ultra-compact high-state AM CVn binaries with ZTF and Gaia: New discoveries and observational constraints on Galactic space density

Ilkham Galiullin, Antonio C. Rodriguez, Kareem El-Badry +9

Ultra-compact AM CVn binaries in the high-state of stable mass transfer () are expected to be among the loudest persistent sources for upcomin…

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.EP2026

The KPF SURFS-UP Survey I: Transmission Spectroscopy of WASP-76 b

Aaron Householder, Fei Dai, Aurora Kesseli +25

We introduce the KPF SURFS-UP (Spectroscopy of the Upper-atmospheres and ReFractory Species in Ultra-hot Planets) Survey, a high-resolution survey to investigate the atmospheric co…

astro-ph.IM2026

Optimal mitigation of random telegraph noise for improved photometry at high frame rates

Christopher Layden, Daniel-Rolf Harbeck, Tejus Deo-Dixit +3

Random telegraph noise (RTN) is a major contributor to read noise in many CMOS image sensors considered for astronomical use. While scientific CMOS image sensors deliver lower read…

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.SR2026

The Physics of Mass Transfer in Substellar and Low-Mass Binaries

Samuel Whitebook, Jim Fuller, Kevin Burdge +3

Several dozen binary ultracool and brown dwarf systems have been identified to date. These systems represent valuable probes of star and planet formation at the lowest mass scales.…