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Tristan L. Smith

4 papers hereh-index 7564 citations13 works total

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

author position
  • first author1
  • middle author1
  • last author2

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

fields
  • astro-ph.CO3
  • gr-qc1
same name
  • Tristan L. Smith — 28 papers, h 34
  • Tristan L. Smith — 8 papers
  • Tristan L. Smith — 2 papers, h 4

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
20242026
collaborators

4 papers

gr-qc2026

Addressing leakage and mode suppression in angular power spectrum estimation for gravitational-wave backgrounds using pulsar timing arrays

Deepali Agarwal, Joseph D. Romano, Yacine Ali-Haïmoud +1

Mapping gravitational-wave background (GWB) anisotropy with pulsar timing arrays (PTAs) is affected by harmonic-space mode suppression and mode coupling arising from an array's non…

astro-ph.CO2025

Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension

Vivian Poulin, Tristan L. Smith, Rodrigo Calderón +1

The data release six of the Atacama Cosmology Telescope (ACT DR6) and the second data release from the Dark Energy Spectroscopic Instrument (DESI DR2) recently became available. In…

astro-ph.CO2025

Predictions for new physics in the CMB damping tail

Tristan L. Smith, Nils Schöneberg

Ever since the Planck satellite measured the the cosmic microwave background (CMB) down to arcminute angular scales, the mismatch between the CMB-inferred value of the Hubble const…

astro-ph.CO2024

Towards alleviating the H0​ and S8​ tensions with Early Dark Energy - Dark Matter drag

Théo Simon, Tal Adi, José Luis Bernal +3

Early dark energy, an additional component of dark energy active in the decade of redshift before recombination, has emerged as one of the most effective models at reducing the $H_…

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