R. Miquel
Physics and Astronomy · The Ohio State University
Publications
1,123
Citations
73,613
Est. group size
~18
Recurring co-author estimate
Active years
57
Publishing since 1970
R. Miquel works in observational cosmology and galaxy survey science, contributing to large collaborations such as the PAU Survey and DESI that map millions of galaxies and stars to study galaxy formation, the structure of the Milky Way, and the large-scale structure of the universe. Much of the work involves photometric and spectroscopic redshift measurements, galaxy classification, and using survey data to test models of how galaxies and cosmic structures form and evolve. This research relies heavily on large collaborative teams, statistical and machine-learning methods, and public astronomical survey datasets.
Publication output grew substantially from around 39 papers per year in 2017 to over 100 per year in 2023-2024, reflecting a marked increase in collaborative survey-based output over the last decade.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Signatures of a Tidally Induced Spiral Arm at the Anticenter of the Milky Way and a Kinematically Extended Anticenter Stream Using DESI Data Release 2
The Astronomical Journal · 2026
- The PAU Survey: Uncovering the connection between intrinsic and observed galaxy properties using symbolic regression
Monthly Notices of the Royal Astronomical Society · 2026
- Disentangling the Distant Stellar Halo Using K Giants in DESI Year 3 Data
The Astrophysical Journal · 2026
- The DESI Y1 RR Lyrae catalog II: The metallicity dependency of pulsational properties, the shape of the RR Lyrae instability strip, and metal rich RR Lyrae
arXiv (Cornell University) · 2025
- Dimensional reduction for sampled priors and application to photometric redshift distributions
DIGITAL.CSIC (Spanish National Research Council (CSIC)) · 2025
- The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation
Monthly Notices of the Royal Astronomical Society · 2024
- Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensing
Journal of Cosmology and Astroparticle Physics · 2024
- The PAU Survey: The quasar Ly<i>α</i> and UV luminosity functions at 2.7 < <i>z</i> < 5.3
Astronomy and Astrophysics · 2024
- The PAU survey: photometric calibration of narrow band images
Monthly Notices of the Royal Astronomical Society · 2024
- DESI Emission-line Galaxies: Unveiling the Diversity of [O ii] Profiles and Its Links to Star Formation and Morphology
The Astrophysical Journal · 2024
- The imprint of cosmic voids from the DESI Legacy Survey DR9 LRGs in the Planck 2018 lensing map through spectroscopically calibrated mocks
arXiv (Cornell University) · 2024
- The PAU Survey: galaxy stellar population properties estimates with narrowband data
arXiv (Cornell University) · 2024
- The PAU Survey: The quasar UV and Ly$α$ luminosity functions at $2.7
arXiv (Cornell University) · 2024
- ANNZ+: an enhanced photometric redshift estimation algorithm with applications on the PAU Survey
arXiv (Cornell University) · 2024
- The Physics of the Accelerating Universe Survey: narrow-band image photometry
Monthly Notices of the Royal Astronomical Society · 2023
- Monthly Notices of the Royal Astronomical Society×236
- arXiv (Cornell University)×137
- The Astrophysical Journal×63
- Physical review. D/Physical review. D.×40
- Journal of Cosmology and Astroparticle Physics×36
- K. Honscheid
Physics and Astronomy · The Ohio State University
- M. Lima
Physics and Astronomy · The Ohio State University
- Kyoung-Soo Lee
Physics and Astronomy · Purdue University West Lafayette
- K. Honscheid
Physics and Astronomy · The Ohio State University
- Paul Martini
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.
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