◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

D. Charbonneau

40 papers hereh-index 10716 citations48 works total

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

author position
  • sole author1
  • first author1
  • middle author31
  • last author2

Across the 35 of 40 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP29
  • astro-ph4
  • astro-ph.IM3
  • astro-ph.SR3
  • physics.optics1
same name
  • D. Charbonneau — 315 papers, h 95
  • D. Charbonneau — 18 papers, h 10
  • D. Charbonneau — 3 papers, h 2
  • D. Charbonneau — 1 paper, h 19
  • D. Charbonneau — 1 paper, h 1
  • D. Charbonneau — 1 paper

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
20022026
most citedMasses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets

497 citations · 1.1k across the 39 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026

Radial and Rotational Velocities of a Volume-Complete Sample of M Dwarfs with Masses 0.1-0.3 Msun within 15 parsecs

Jennifer G. Winters, Emily K. Pass, David Charbonneau +7

We present the results from a five-year campaign to gather multi-epoch, high-resolution spectra of a volume-complete sample of 413 M dwarfs with masses 10-30% that of the Sun that…

astro-ph.SR2025

Metallicities from High-Resolution TRES Spectra with uberMS: Performance Benchmarks and Literature Comparison

Emily K. Pass, Phillip A. Cargile, Victoria DiTomasso +7

As the field of exoplanetary astronomy has matured, demand has grown for precise stellar abundances to probe subtle correlations between stellar compositions and planetary demograp…

astro-ph.SR2024

The Mass Dependence of Hα Emission and Stellar Spindown for Fully Convective M Dwarfs

Emily K. Pass, David Charbonneau, David W. Latham +4

Fully convective M dwarfs typically remain rapidly rotating and magnetically active for billions of years, followed by an abrupt and mass-dependent transition to slow rotation and…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.