Paul Martini
Physics and Astronomy · The Ohio State University
Publications
549
Citations
34,614
Est. group size
~21
Recurring co-author estimate
Active years
59
Publishing since 1968
Paul Martini works in observational cosmology and extragalactic astronomy, contributing to large sky-survey collaborations that map the distribution of galaxies and quasars to study the universe's expansion history and dark energy. Much of the recent work is tied to the DESI (Dark Energy Spectroscopic Instrument) survey, using techniques like baryon acoustic oscillations, galaxy clustering, and the Lyman-alpha forest (light patterns from distant quasars) to measure cosmic growth and structure. He also contributes to related work on active galactic nuclei (supermassive black holes at galaxy centers) and supernovae as tools for measuring cosmic distances.
Publication output has grown over the last decade, dipping around 2021 but rising notably from 2023 through 2025.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- The DESI DR1 peculiar velocity survey: growth rate measurements from the maximum likelihood fields method
Journal of Cosmology and Astroparticle Physics · 2026
- Detection of supernova magnitude fluctuations induced by large-scale structure
The Open Journal of Astrophysics · 2026
- Supplementary data for: Probing the limits of cosmological information from the Lyman-alpha forest 2-point correlation functions
DIGITAL.CSIC (Spanish National Research Council (CSIC)) · 2026
- OzDES reverberation mapping of Active Galactic Nuclei: Final data release, black-hole mass results, and scaling relations
Publications of the Astronomical Society of Australia · 2026
- Supplementary data for DESI DR1 Lyα 1D power spectrum: Validation of estimators
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Supplementary data for DESI DR1 Lyα 1D power spectrum: Validation of estimators
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Supplementary data for: Clustering of high-redshift quasars with DESI DR2
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Supplementary data for: Clustering of high-redshift quasars with DESI DR2
Zenodo (CERN European Organization for Nuclear Research) · 2026
- DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations
Journal of Cosmology and Astroparticle Physics · 2025
- DESI 2024 III: baryon acoustic oscillations from galaxies and quasars
Journal of Cosmology and Astroparticle Physics · 2025
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman alpha forest
Journal of Cosmology and Astroparticle Physics · 2025
- DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data
Physical review. D/Physical review. D. · 2025
- DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics
Journal of Cosmology and Astroparticle Physics · 2025
- DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars
Journal of Cosmology and Astroparticle Physics · 2025
- ASTRA-DESI DR1 Release v0.12
DIGITAL.CSIC (Spanish National Research Council (CSIC)) · 2025
- Monthly Notices of the Royal Astronomical Society×86
- arXiv (Cornell University)×59
- Journal of Cosmology and Astroparticle Physics×38
- Physical review. D/Physical review. D.×28
- The Astrophysical Journal×15
- M. Lima
Physics and Astronomy · The Ohio State University
- Hui Kong
Physics and Astronomy · The Ohio State University
- Ashley J. Ross
Physics and Astronomy · The Ohio State University
- C. To
Physics and Astronomy · The Ohio State University
- David H. Weinberg
Physics and Astronomy · The Ohio State University
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 19, 2026.
Claim or correct this profile