activity
20032026
most citedExperimental evidence for a surface distribution of two-level systems in superconducting lithographed microwave resonators

366 citations · 2.6k across the 67 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2023★ 20 cited

Surveying Nearby Brown Dwarfs with HGCA: Direct Imaging Discovery of a Faint, High-Mass Brown Dwarf Orbiting HD 176535 A

Yiting Li, Timothy D. Brandt, G. Mirek Brandt +16

Brown dwarfs with well-measured masses, ages and luminosities provide direct benchmark tests of substellar formation and evolutionary models. We report the first results from a dir…

astro-ph.SR2022★ 11 cited

SCExAO and Keck Direct Imaging Discovery of a Low-Mass Companion Around the Accelerating F5 Star HIP 5319

Noah Swimmer, Thayne Currie, Sarah Steiger +26

We present the direct imaging discovery of a low-mass companion to the nearby accelerating F star, HIP 5319, using SCExAO coupled with the CHARIS, VAMPIRES, and MEC instruments in…

astro-ph.SR2021★ 3 cited

Orbital Parameters and Binary Properties of 37 FGK stars in the Cores of Open Clusters NGC 2516 and NGC 2422

Isabel Lipartito, John I. Bailey, Timothy D. Brandt +4

We present orbits for 24 binaries in the field of open cluster NGC 2516 (~150 Myr) and 13 binaries in the field of open cluster NGC 2422 (~130 Myr) using results from a multi-year…

astro-ph.SR2021★ 24 cited

SCExAO/MEC and CHARIS Discovery of a Low Mass, 6 AU-Separation Companion to HIP 109427 using Stochastic Speckle Discrimination and High-Contrast Spectroscopy

Sarah Steiger, Thayne Currie, Timothy D. Brandt +28

We report the direct imaging discovery of a low-mass companion to the nearby accelerating A star, HIP 109427, with the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrum…

astro-ph.SR2013★ 26 cited

Direct Detection of SDSS J0926+3624 Orbital Expansion with ARCONS

P. Szypryt, G. E. Duggan, B. A. Mazin +10

AM Canum Venaticorum (AM CVn) stars belong to a class of ultra-compact, short period binaries with spectra dominated largely by helium. SDSS J0926+3624 is of particular interest as…