David Kipping

Physics and Astronomy · Physical Sciences

38h-index5.9kcitations246works1.82yr avg
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Research Topics

Stellar, planetary, and galactic studies(163), Astronomy and Astrophysical Research(96), Astro and Planetary Science(84), Astrophysics and Star Formation Studies(52), Gamma-ray bursts and supernovae(27)

Publications245 total

Mapping the Orbital Landscape of Perturbing Planet Solutions for Single-planet Systems with TTVs
The Astrophysical Journal·2026· 1 citedOpen Access
The Eschatian Hypothesis
Research Notes of the AAS·2025Open Access
A JWST Transit of a Jupiter Analog I: Constraints on the Oblateness of Kepler-167e
arXiv (Cornell University)·2025Open Access
Solar Hegemony: M-Dwarfs Are Unlikely to Host Observers Such as Ourselves
arXiv (Cornell University)·2025Open Access
Exoplaneteers Keep Overestimating Sigma Significances
arXiv (Cornell University)·2025Open Access
Concerning the possible exomoons around Kepler-1625 b and Kepler-1708 b
Nature Astronomy·2025· 3 cited
The Exoplanet Edge: Planets Do Not Induce Observable Transit Timing Variations with a Dominant Transit Timing Variation Period Faster than Half Their Orbital Period
The Astrophysical Journal Letters·2025· 2 citedOpen Access
Near-circular orbits for planets with Earth-like sizes and instellations around M and K dwarf stars
Nature Astronomy·2025· 4 cited
Strong Evidence that Abiogenesis Is a Rapid Process on Earth Analogs
Astrobiology·2025· 3 cited
Strong Evidence That Abiogenesis Is a Rapid Process on Earth Analogs
arXiv (Cornell University)·2025Open Access
Near-circular orbits for planets around M/K-type stars with Earth-like sizes and instellations
arXiv (Cornell University)·2025Open Access
Do SETI optimists have a fine-tuning problem?
International Journal of Astrobiology·2025· 4 citedOpen Access
The democratic detrender: Ensemble-Based Removal of the Nuisance Signal in Stellar Time-Series Photometry
arXiv (Cornell University)·2024Open Access
The Exoplanet Edge: Planets Don't Induce Observable TTVs with a Dominant TTV Period Faster than Half their Orbital Period
arXiv (Cornell University)·2024· 1 citedOpen Access
squishyplanet: modeling transits of non-sphericalexoplanets in JAX
The Journal of Open Source Software·2024· 7 citedOpen Access
The SNR of idealized radial velocity signals
Monthly Notices of the Royal Astronomical Society·2024· 3 citedOpen Access
Do SETI Optimists Have a Fine-Tuning Problem?
arXiv (Cornell University)·2024Open Access
The SNR of idealised radial velocity signals
arXiv (Cornell University)·2024Open Access
Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets
The Astrophysical Journal Supplement Series·2024· 7 citedOpen Access
A Reply to: Large Exomoons unlikely around Kepler-1625 b and Kepler-1708 b
arXiv (Cornell University)·2024· 2 citedOpen Access
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Frequent Co-authors

G. Á. Bakos(11), J. D. Hartman(9), Lars A. Buchhave(9), David W. Latham(7), David Nesvorný(6), Mark E. Everett(5), Allan R. Schmitt(5), Guillermo Torres(5), Andrew W. Howard(5), Alex Teachey(5), John Asher Johnson(4), G. Kovács(4), Geoffrey W. Marcy(4), Dimitar Sasselov(4), S. J. Fossey(4), Emily Sandford(4), David R. Ciardi(3), R. W. Noyes(3), Debra A. Fischer(3), Gilbert A. Esquerdo(3)