activity
19982023
most citedA Survey of z>5.8 Quasars in the Sloan Digital Sky Survey I: Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z~6

954 citations · 8.6k across the 75 of their papers we have counts for

collaborators

75 papers

astro-ph.SR2023★ 33 cited

JWST/NIRCam discovery of the first Y+Y brown dwarf binary: WISE J033605.05014350.4

Per Calissendorff, Matthew De Furio, Michael Meyer +25

We report the discovery of the first brown dwarf binary system with a Y dwarf primary, WISE J033605.05014350.4, observed with NIRCam on JWST with the F150W and F480M filters. We…

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.SR2022★ 48 cited

A Spectro-photometric Analysis of Cool White Dwarfs in the Gaia and Pan-STARRS Footprint

Alexandre Caron, Pierre Bergeron, Simon Blouin +1

We present a spectro-photometric analysis of 2880 cool white dwarfs within 100 pc of the Sun and cooler than Teff = 10,000 K, with grizy Pan-STARRS photometry and Gaia trigonometri…

astro-ph.SR2022★ 33 cited

On the Nature of Ultracool White Dwarfs: Not so Cool Afterall

P. Bergeron, Mukremin Kilic, Simon Blouin +3

A recent analysis of the 100 pc white dwarf sample in the SDSS footprint demonstrated for the first time the existence of a well defined ultracool -- or IR-faint -- white dwarf seq…

astro-ph.EP2021★ 14 cited

Gemini/GMOS Transmission Spectroscopy of the Grazing Planet Candidate WD 1856+534 b

Siyi Xu, Hannah Diamond-Lowe, Ryan J. MacDonald +12

WD 1856+534 b is a Jupiter-sized, cool giant planet candidate transiting the white dwarf WD 1856+534. Here, we report an optical transmission spectrum of WD 1856+534 b obtained fro…

astro-ph.SR2021★ 15 cited

Ultracool Dwarfs Observed with the Spitzer Infrared Spectrograph. I. An Accurate Look at the L-to-T Transition at 300 Myr from Optical through Mid-infrared Spectrophotometry

Genaro Suárez, Stanimir Metchev, Sandy K. Leggett +2

We present IRS 5--14 m spectra and 16 m and 22 m photometry of the T2.5 companion to the 300 Myr-old G0V star HN Peg. We incorporate previous 0.8--5 m o…