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D. Kessler

4 papers hereh-index 233 citations7 works total

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

author position
  • first author3
  • middle author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO1
  • astro-ph.GA1
  • gr-qc1
  • stat.ME1
same name
  • D. Kessler — 111 papers, h 38
  • D. Kessler — 6 papers, h 7
  • D. Kessler — 3 papers, h 2
  • D. Kessler — 2 papers, h 4
  • D. Kessler — 1 paper
  • D. Kessler — 1 paper, h 1

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

most citedEffects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization

5 citations · 5 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.CO2026

Reconstructing dark energy with fewer assumptions

Daniel A. Kessler, Eleonora Di Valentino, Luis A. Escamilla +1

We perform minimalistic reconstructions of the dark energy density and equation of state using late-time distance measurements. Our methodology avoids assumptions that correlate th…

stat.ME2025

False Discovery Controlled Regions for Excursion Sets

Howon Ryu, Thomas Maullin-Sapey, Armin Schwartzman +1

Identifying areas where the signal is prominent is an important task in image analysis, with particular applications in brain mapping. In this work, we develop False Discovery Cont…

astro-ph.GA2025★ 5 cited

Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization

Boyuan Liu, Daniel Kessler, Thomas Gessey-Jones +6

The first generation of stars, known as Population III (Pop III), played a crucial role in the early Universe through their unique formation environment and metal-free composition.…

gr-qc2025

Gravitational Wave Scattering From the Sun and Planets

Daniel A. Kessler, Craig J. Copi, Glenn D. Starkman

General relativity predicts that massless waves should scatter from the Riemann curvature of their backgrounds. These scattered waves are sometimes called tails and have…

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