activity
19982023
most citedA Giant Planet Candidate near a Young Brown Dwarf

666 citations · 2.5k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.SR2023★ 13 cited

Disk or Companion: Characterizing Excess Infrared Flux in Seven White Dwarf Systems with Near-Infrared Spectroscopy

Dylan Owens, Siyi Xu, Elena Manjavacas +7

Excess infrared flux from white dwarf stars is likely to arise from a dusty debris disk or a cool companion. In this work, we present near-infrared spectroscopic observations with…

astro-ph.SR2023★ 32 cited

New chondritic bodies identified in eight oxygen-bearing white dwarfs

Alexandra E. Doyle, Beth L. Klein, Patrick Dufour +8

We present observations and analyses of eight white dwarf stars that have accreted rocky material from their surrounding planetary systems. The spectra of these helium-atmosphere w…

astro-ph.SR2022★ 54 cited

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.EP2022★ 25 cited

Unusual Abundances from Planetary System Material Polluting the White Dwarf G238-44

Ted M Johnson, Beth L. Klein, D. Koester +3

Ultraviolet and optical spectra of the hydrogen-dominated atmosphere white dwarf star G238-44 obtained with FUSE, Keck/HIRES, HST/COS, and HST/STIS reveal ten elements heavier than…

astro-ph.SR2022★ 6 cited

Infrared and Optical Detectability of Dyson Spheres at White Dwarf Stars

B. Zuckerman

It has been hypothesized that advanced technological civilizations will construct giant space colonies and supporting infrastructures to orbit about their home stars. With data fro…

astro-ph.EP2021★ 3 cited

V488 Per revisited: no strong mid-infrared emission features and no evidence for stellar/sub-stellar companions

Swetha Sankar, Carl Melis, Beth L. Klein +4

We present characterization of the planetary system architecture for V488 Per, the dustiest main sequence star known with a fractional infrared luminosity of ~16%. Far-infrared ima…