activity
20192026
most citedLoose Ends for the Exomoon Candidate Host Kepler-1625b

31 citations · 53 across the 24 of their papers we have counts for

collaborators

26 papers

astro-ph.EP2026

Singles in Disguise: Kepler's Low-SNR Single-Transiting Systems as Incompletely Detected Multis

Daniel A. Yahalomi, David Nesvorny, David Kipping +2

NASA's Kepler mission found more systems with one transiting planet (``singles'') than expected from those with several (``multis''). This excess was first taken as evidence for a…

astro-ph.EP2026

JWST Excludes Exomoons Down to 0.1 Earth Radii Around a Rocky, Temperate Exoplanet

David Kipping

To date, even with JWST, it has not been possible to test for exomoons as small as the Moon. Only two reported searches for exomoons around bound planets have been attempted with J…

astro-ph.EP2026

ExoMOD II. A Statistical Model of Transit Timing Variations in Kepler Multi-Planet Systems

David Nesvorny, Daniel A. Yahalomi, David Kipping +2

In Paper I (Nesvorný et al. 2026), we forward modeled transit observations of the Kepler telescope to characterize the orbital properties of close-in planetary systems. The new pop…

astro-ph.EP2026

ExoMOD I. A Forward Model for the Orbital Architecture of Kepler Multi-Planet Systems

David Nesvorny, Daniel A. Yahalomi, David Kipping +1

Transit observations only detect planets with favorable, near edge-on orientation of orbits as seen by a distant observer, which leaves much freedom for various interpretations in…

astro-ph.CO2026

The Cosmological Hart-Tipler Conjecture

David Kipping

Self-reproducing automata, so-called von Neumann machines, have been repeatedly estimated to be capable of traversing the Galaxy many times given its age. Our mere existence thus s…

astro-ph.EP2026

What to make of the Earth's curiously intermediate land fraction?

David Kipping

Approximately two-thirds of the Earth, the only known inhabited planet, is covered in ocean. Why not 0.01% or 99.99%? It has been previously suggested that this may represent a cer…

astro-ph.EP2026★ 2 cited

TIC-65910228 b / NGTS-38 b, a 180 day transiting warm super-Jupiter

Toby Rodel, Solène Ulmer-Moll, Samuel Gill +63

We present the discovery of TIC-65910228 b / NGTS-38 b, a giant exoplanet with a radius of R and a mass of M on a long-…

physics.pop-ph2025

The Eschatian Hypothesis

David Kipping

The history of astronomical discovery shows that many of the most detectable phenomena, especially detection firsts, are not typical members of their broader class, but rather rare…

astro-ph.EP2025★ 2 cited

A JWST Transit of a Jupiter Analog: II. A Search for Exomoons

David Kipping, Ben Cassese, Quentin Changeat +3

We present a search for exomoons around the Jupiter-like exoplanet Kepler-167e using a NIRSpec JWST transit. Our 60 hour time series clearly reveals the enormous impact of long-ter…

astro-ph.EP2025

A JWST Transit of a Jupiter Analog I: Constraints on the Oblateness of Kepler-167e

Ben Cassese, David Kipping, Quentin Changeat +5

In October 2024 JWST observed a transit of Kepler-167e, a Jupiter-analog planet on a 1000+ day orbit. These observations, recorded over a long baseline of nearly 60 hours, were des…

astro-ph.IM2025

Solar Hegemony: M-Dwarfs Are Unlikely to Host Observers Such as Ourselves

David Kipping

With no firm evidence for life beyond our solar system, inferences about the population observers such as ourselves rests upon the Earth as a single input, at least for now. Whilst…

physics.space-ph2025

Torqued Accelerator using Radiation from the Sun (TARS) for Interstellar Payloads

David Kipping, Kathryn Lampo

The concept of exploring space using solar power is energetically appealing, but interstellar solar sails typically require extremely low areal densities (~g/m^2). This work explor…

astro-ph.EP2025

Strong Evidence That Abiogenesis Is a Rapid Process on Earth Analogs

David Kipping

The early start to life naively suggests that abiogenesis is a rapid process on Earth-like planets. However, if evolution typically takes ~4Gyr to produce intelligent life-forms li…

astro-ph.EP2025

Near-circular orbits for planets around M/K-type stars with Earth-like sizes and instellations

David Kipping, Diana Solano-Oropeza, Daniel A. Yahalomi +3

Recent advances have enabled the discovery of a population of potentially Earth-like planets, yet their orbital eccentricity, which governs their climate and provides clues about t…

astro-ph.EP2024★ 3 cited

Mapping the Orbital Landscape of Perturbing Planet Solutions for Single-Planet Systems with TTVs

Daniel A. Yahalomi, David Kipping

There are now thousands of single-planet systems observed to exhibit transit timing variations (TTVs), yet we largely lack any interpretation of the implied masses responsible for…

astro-ph.EP2024

The democratic detrender: Ensemble-Based Removal of the Nuisance Signal in Stellar Time-Series Photometry

Daniel A. Yahalomi, David Kipping, Diana Solano-Oropeza +10

Accurate, precise, and computationally efficient removal of unwanted activity that exists as a combination of periodic, quasi-periodic, and non-periodic systematic trends in time-s…

astro-ph.EP2024★ 3 cited

The Exoplanet Edge: Planets Don't Induce Observable TTVs with a Dominant TTV Period Faster than Half their Orbital Period

Daniel A. Yahalomi, David Kipping, Eric Agol +1

Transit timing variations (TTVs) are observed for exoplanets at a range of amplitudes and periods, yielding an ostensibly degenerate forest of possible explanations. We offer some…

astro-ph.IM2024★ 8 cited

squishyplanet: Modeling Transits of Non-spherical Exoplanets in JAX

Ben Cassese, Justin Vega, Tiger Lu +3

While astronomers often assume that exoplanets are perfect spheres when analyzing observations, the subset of these distant worlds that are subject to strong tidal forces and/or ra…

astro-ph.IM2024

Do SETI Optimists Have a Fine-Tuning Problem?

David Kipping, Geraint Lewis

In ecological systems, be it a petri dish or a galaxy, populations evolve from some initial value (say zero) up to a steady state equilibrium, when the mean number of births and de…

astro-ph.EP2024★ 2 cited

A Reply to: Large Exomoons unlikely around Kepler-1625 b and Kepler-1708 b

David Kipping, Alex Teachey, Daniel A. Yahalomi +7

Recently, Heller & Hippke argued that the exomoon candidates Kepler-1625 b-i and Kepler-1708 b-i were allegedly 'refuted'. In this Matters Arising, we address these claims. For Kep…

astro-ph.EP2024

Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets

Paul A. Dalba, Stephen R. Kane, Howard Isaacson +29

Discovering and characterizing exoplanets at the outer edge of the transit method's sensitivity has proven challenging owing to geometric biases and the practical difficulties asso…

astro-ph.IM2023

Deconstructing Alien Hunting

David Kipping, Jason Wright

The search for extraterrestrial (alien) life is one of the greatest scientific quests yet raises fundamental questions about just what we should be looking for and how. We approach…

astro-ph.EP2023

The giant nature of WD 1856 b implies that transiting rocky planets are rare around white dwarfs

David Kipping

White dwarfs (WDs) have roughly Earth-sized radii - a fact long recognized to facilitate the potential discovery of sub-Earth sized planets via transits, as well atmospheric charac…

astro-ph.EP2023

Not So Fast Kepler-1513: A Perturbing Planetary Interloper in the Exomoon Corridor

Daniel A. Yahalomi, David Kipping, David Nesvorný +9

Transit Timing Variations (TTVs) can be induced by a range of physical phenomena, including planet-planet interactions, planet-moon interactions, and stellar activity. Recent work…