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RC100: Rotation Curves of 100 Massive Star-forming Galaxies at z = 0.6-2.5 Reveal Little Dark Matter on Galactic Scales
A. Nestor Shachar, S. H. Price, N. M. Förster Schreiber, R. Genzel, T. T. Shimizu, L. J. Tacconi, H. Übler, A. Burkert, R. I. Davies, A. Dekel, R. Herrera-Camus, L. L. Lee, D. Liu, D. Lutz, T. Naab, R. Neri, A. Renzini, R. Saglia, K. F. Schuster, A. Sternberg
- Tel Aviv University
- Max Planck Institut für Extraterrestrische Physik
- University of Pittsburgh
- University of California
- University of Cambridge
- Ludwig Maximilian University of Munich
- The Hebrew University of Jerusalem
- Universidad de Concepción
- Max Planck Institute for Astrophysics
- Institut de Radioastronomie Millimétrique
- INAF - Osservatorio Astronomico di Padova
- Flatiron Institute
- The Australian National University
- ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)
Research output: Contribution to journal › Article › peer-review
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