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researcher

J. Stone

50 papers hereh-index 191.3k citations69 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author7
  • middle author27
  • last author8

Across the 42 of 50 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR16
  • astro-ph.IM15
  • astro-ph.EP13
  • astro-ph.GA4
  • astro-ph.HE2
same name
  • J. Stone — 164 papers, h 83
  • J. Stone — 96 papers, h 68
  • J. Stone — 39 papers, h 22
  • J. Stone — 32 papers, h 20
  • J. Stone — 15 papers, h 6
  • J. Stone — 12 papers, h 8

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20122026
most citedThe JWST Early Release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b

176 citations · 1.3k across the 48 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.SR2014★ 10 cited

Time-monitoring Observations of Brγ Emission from Young Stars

J. A. Eisner, G. H. Rieke, M. J. Rieke +9

We present multiple epochs of near-IR spectroscopy for a sample of 25 young stars, including T Tauri, Herbig Ae/Be, and FU Ori objects. Using the FSPEC instrument on the Bok 90-inc…

astro-ph.SR2014★ 4 cited

Variable Accretion Processes in the Young Binary-Star System UY Aur

Jordan M. Stone, J. A. Eisner, Colette Salyk +2

We present new K-band spectroscopy of the UY Aur binary star system. Our data are the first to show H2​ emission in the spectrum of UY Aur A and the first to spectrally resolve…

astro-ph.SR2014★ 56 cited

Constraining the Sub-AU-Scale Distribution of Hydrogen and Carbon Monoxide Gas around Young Stars with the Keck Interferometer

J. A. Eisner, L. A. Hillenbrand, Jordan M. Stone

We present Keck Interferometer observations of T Tauri and Herbig Ae/Be stars with a spatial resolution of a few milliarcseconds and a spectral resolution of ~2000. Our observation…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.