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Review Cycle Records

Nature Astronomy

Springer SCIE Non-OA
2026 Emerging Zone 12025 CAS Zone 1 TOP2025 JCR Q1
276.1Average days
238.5Median days
121Fastest days
477Longest days
2932025 publications

Paper Review Records

All Paper Review Records

10 valid samples · Newest publication first
Review days = acceptance date − received date. PDF, DOI, and publisher-page sources are retained.

465 days

The CosmoCube lunar mission for probing the dark ages and cosmic dawn via 21-cm cosmology

AuthorsEloy de lera Acedo; David Bacon; Will Grainger; Dominic Anstey; Harry Bevins; Lucinda King; Kaan Artuc; Mohammed Al-Badri; Chris Pearson; Suresh Balaji; Richard Holdaway; Judd Bowman; Daniel Jacobs; Theodora Varelidi-Strati; Steve Eckersley; Abigail Harvey; Andrea Turconi; Ana-Maria Dorobat; Andri M. Gretarsson; Yabin Liao; Xan Morice-Atkinson; Olugbenga Olumodimu

Affiliations1. Cavendish Laboratory, University of Cambridge, Cambridge, UK; 2. Kavli Institute for Cosmology in Cambridge, University of Cambridge, Cambridge, UK; 3. Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, UK; 4. RAL Space, STFC, Rutherford Appleton Laboratory, Didcot, UK; 5. In-Space Missions, BAE Systems, Alton, UK; 6. Cambridge Space Associates, c/o Opus, Newbury, UK; 7. School of Earth and Space Exploration, Arizona State University, Tempe, USA; 8. Surrey Satellite Technology Limited, Guildford, UK; 9. Physics and Astronomy Department, Embry-Riddle Aeronautical University, Prescott, USA; 10. Aerospace Engineering Department, Embry-Riddle Aeronautical University, Prescott, USA

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360 days

Measuring the high-energy neutrino sky using the deep-valley neutrino observatory TAMBO

AuthorsTAMBO collaboration

Affiliations1. Laboratory for Particle Physics and Cosmology, Department of Physics, Harvard University, Cambridge, MA, USA; 2. Sección Física, Departamento de Ciencias, Pontificia Universidad Católica del Perú, Lima, Perú; 3. Electrical and Mechatronic Department, Universidad de Ingeniería y Tecnología, Barranco, Perú; 4. Niels Bohr International Academy, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark; 5. Universidad del Pacífico, Lima, Perú; 6. Instituto de Radioastronomía, Pontificia Universidad Católica del Perú, San Miguel, Perú; 7. Program in Science, Technology, and Society, and Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA; 8. Department of History and Philosophy of Science, and Institute of Astronomy, University of Cambridge, Cambridge, UK; 9. Luleå University of Technology, Luleå, Sweden; 10. Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Padova, Padova, Italy; 11. Institute of Physics, Academia Sinica, Taipei City, Taiwan; 12. Donostia International Physics Center (DIPC), San Sebastián/Donostia, Spain; 13. Instituto de Física Corpuscular (IFIC), CSIC and Universitat de València, Paterna, Spain; 14. Los Alamos National Laboratory, Los Alamos, NM, USA; 15. Department of Physics and Astronomy, University of Nevada, Las Vegas, NV, USA; 16. Nevada Center for Astrophysics, University of Nevada, Las Vegas, NV, USA; 17. Centre for Cosmology, Particle Physics and Phenomenology -- CP3, Université catholique de Louvain, Louvain-la-Neuve, Belgium; 18. Department of Physics and Astronomy, University of Hawaiʻi at Mānoa, Honolulu, HI, USA; 19. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA; 20. Department of Physics, Columbia University, New York, NY, USA; 21. Departamento de Física & ICTEA, Universidad de Oviedo, Oviedo, Spain; 22. Department of Physics, Enigneering Physics and Astronomy, Queen’s University, Kingston, Ontario, Canada; 23. Arthur B. McDonald Canadian Astroparticle Physics Research, Kingston, Ontario, Canada; 24. Perimeter Institute for Theoretical Physics, Waterloo, Ontario, Canada; 25. Universidad Continental, Arequipa, Perú

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145 days

The multimessenger Universe as a training ground for frontier AI

AuthorsAbigail Petulante; Chayan Chatterjee; Karan Jani; Jesse Spencer-Smith; Stephen R. Taylor; Adam A. Miller; Keivan G. Stassun; Gioia Rau; Simon Peter Worden; Jeff Shen; Digvijay Wadekar; Javier Roulet; Deep Chatterjee; Nima Laal; Ignacio Magana Hernandez; Daniel Moyer; Matthew Johnson-Roberson; Michele Vallisneri; Suyash Deshmukh; Ryan Nowicki

Affiliations1. Data Science Institute, Vanderbilt University, Nashville, USA; 2. Department of Physics and Astronomy, Vanderbilt University, Nashville, USA; 3. Department of Physics and Astronomy, Northwestern University, Evanston, USA; 4. Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University, Evanston, USA; 5. NSF-Simons AI Institute for the SKy (SKAI), Chicago, USA; 6. Schmidt Sciences, New York, USA; 7. Breakthrough Prize Foundation, Menlo Park, USA; 8. Department of Astrophysical Sciences, Princeton University, Princeton, USA; 9. Department of Physics and Astronomy, Johns Hopkins University, Baltimore, USA; 10. Department of Astronomy, The University of Texas at Austin, Austin, USA; 11. Kavli Institute for Cosmological Physics, The University of Chicago, Chicago, USA; 12. School of Natural Sciences, Institute for Advanced Study, Princeton, USA; 13. MIT Kavli Institute, Massachusetts Institute of Technology, Cambridge, USA; 14. McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburg, USA; 15. Department of Computer Science, Vanderbilt University, Nashville, USA; 16. College of Connected Computing, Vanderbilt University, Nashville, USA; 17. Department of Physics, ETH Zurich, Zurich, Switzerland

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342 days

Ram-pressure stripping caught in action in a young cluster at z = 2.51

AuthorsKe Xu; Tao Wang; Emanuele Daddi; David Elbaz; Hanwen Sun; Longyue Chen; Qiaoyang Hao; Raphael Gobat; Anita Zanella; Daizhong Liu; Mengyuan Xiao; Renyue Cen; Tadayuki Kodama; Kotaro Kohno; Tiancheng Yang; Can Xu; Zhi-Yu Zhang; Luwenjia Zhou; Francesco Valentino

Affiliations1. School of Astronomy and Space Science, Nanjing University, Nanjing, China; 2. Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing, China; 3. Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France; 4. Instituto de Física, Pontificia Universidad Católica de Valparaíso, Valparaíso, Chile; 5. Istituto Nazionale di Astrofisica (INAF), Padua, Italy; 6. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China; 7. State Key Laboratory of Radio Astronomy and Technology, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China; 8. Department of Astronomy, University of Geneva, Versoix, Switzerland; 9. Centre for Cosmology and Computational Astrophysics, Institute for Advanced Study in Physics and Institute of Astronomy, School of Physics, Zhejiang University, Hangzhou, China; 10. Astronomical Institute, Tohoku University, Sendai, Japan; 11. Institute of Astronomy, School of Science, The University of Tokyo, Tokyo, Japan; 12. Research Centre for the Early Universe, School of Science, The University of Tokyo, Tokyo, Japan; 13. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Chiba, Japan; 14. Cosmic Dawn Center (DAWN), Copenhagen, Denmark; 15. DTU Space, Technical University of Denmark, Kongens Lyngby, Denmark

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121 days

Compact dusty starbursts at cosmic noon linked to high-energy neutrinos

AuthorsYuji Urata; Kuiyun Huang; Bunyo Hatsukade; Mansi Kasliwal; Shigeo S. Kimura; Yuichi Matsuda; Yusuke Miyamoto; Hiroshi Nagai; Kouichiro Nakanishi; Robert Stein

Affiliations1. MITOS Science Co. LTD, New Taipei, Taiwan; 2. Institute of Astronomy, National Central University, Chung-Li, Taiwan; 3. Center for General Education, Chung Yuan Christian University, Taoyuan, Taiwan; 4. National Astronomical Observatory of Japan, Tokyo, Japan; 5. The Graduate University for Advanced Studies, SOKENDAI, Tokyo, Japan; 6. Department of Astronomy, Graduate School of Science, The University of Tokyo, Tokyo, Japan; 7. Cahill Center for Astrophysics, California Institute of Technology, Pasadena, USA; 8. Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai, Japan; 9. Astronomical Institute, Tohoku University, Sendai, Japan; 10. Ministry of Education, Culture, Sports, Science and Technology, Tokyo, Japan; 11. Department of Electrical, Electronic and Computer Engineering, Fukui University of Technology, Fukui, Japan; 12. Department of Astronomy, University of Maryland, College Park, USA; 13. Joint Space-Science Institute, University of Maryland, College Park, USA; 14. Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, USA

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226 days

The timing of the last r-process event near Earth from interstellar 60 Fe, 244 Pu and 247 Cm deposition on Earth

AuthorsDominik Koll; Sebastian Fichter; Michael A. C. Hotchkis; Stephen T. Battisson; Sabrina Beutner; L. Keith Fifield; Michaela B. Froehlich; Johannes Lachner; Stefan Pavetich; Georg Rugel; Zuzana Slavkovská; Stephen G. Tims; Anton Wallner

Affiliations1. Accelerator Mass Spectrometry and Isotope Research, Helmholtz-Zentrum Dresden-Rossendorf, Dresden, Germany; 2. Department of Nuclear Physics and Accelerator Applications, The Australian National University, Canberra, Australia; 3. Institute of Nuclear and Particle Physics, TUD Dresden University of Technology, Dresden, Germany; 4. Centre for Accelerator Science, Australian Nuclear Science and Technology Organisation, Sydney, Australia; 5. Institute of Resource Ecology, Helmholtz-Zentrum Dresden-Rossendorf, Dresden, Germany

Source PDF DOI Publisher page
477 days

On the tidal response of Titan inferred from Cassini data

AuthorsDaniele Durante; Luciano Iess; Valery Lainey

Affiliations1. Sapienza University of Rome, Rome, Italy; 2. LTE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Université, Université de Lille, Lille, France

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198 days

Magnetic field strengths of hot giant exoplanets consistent with Solar System values

AuthorsJulia V. Seidel; Vivien Parmentier; Bibiana Prinoth; Thea Hood; Nishil Mehta; Valentin De Lia; Konstantin Batygin; Tristan Guillot; Ragnar Van den Broeck; Hayley Beltz; Brian Thorsbro; Florian Debras; Daniel D. B. Koll; Thaddeus D. Komacek; Emily Rauscher; Lorenzo Pino; Matteo Brogi; Joost P. Wardenier; Jacob L. Bean; Björn Benneke; Jean-Michel L. B. Désert; Pablo Drake; Siddharth Gandhi; Mark Hammond; David Kasper; Michael R. Line; Elspeth K. H. Lee; Stefan Pelletier; Andreas Seifahrt; Adrien Simonnin; Peter C. B. Smith; Kevin B. Stevenson

Affiliations1. Laboratoire Lagrange, Observatoire de la Côte d’Azur, CNRS, Université Côte d’Azur, Nice, France; 2. European Southern Observatory, Vitacura, Chile; 3. Lund Observatory, Department of Physics, Lund University, Lund, Sweden; 4. European Southern Observatory, Garching, Germany; 5. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, USA; 6. Department of Astronomy, University of Maryland, College Park, USA; 7. Department of Physics and Astronomy, University of Kansas, Lawrence, USA; 8. IRAP, Université de Toulouse, CNRS UMR 5277, Toulouse, France; 9. School of Physics, Peking University, Beijing, People’s Republic of China; 10. Department of Physics, University of Oxford, Oxford, UK; 11. Department of Astronomy and Astrophysics, University of Michigan, Ann Arbor, USA; 12. INAF Osservatorio Astrofisico di Arcetri, Florence, Italy; 13. Dipartimento di Fisica, Università degli Studi di Torino, Torino, Italy; 14. INAF Osservatorio Astrofisico di Torino, Pino Torinese, Italy; 15. Institut Trottier de recherche sur les exoplanètes, Université de Montréal, Montreal, Canada; 16. Weltraumforschung und Planetologie, Physikalisches Institut, University of Bern, Bern, Switzerland; 17. Department of Astronomy and Astrophysics, University of Chicago, Chicago, USA; 18. Department of Earth Planetary and Space Sciences, University of California Los Angeles, Los Angeles, USA; 19. Leibniz Institut für Astrophysik Potsdam, Potsdam, Germany; 20. Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, The Netherlands; 21. DESY, Zeuthen, Germany; 22. Department of Physics, University of Warwick, Coventry, UK; 23. Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK; 24. School of Earth and Space Exploration, Arizona State University, Tempe, USA; 25. Center for Space and Habitability, University of Bern, Bern, Switzerland; 26. Observatoire astronomique de l’Université de Genève, Versoix, Switzerland; 27. International Gemini Observatory NSF NOIRLab, Tucson, USA; 28. JHU Applied Physics Laboratory, Laurel, USA

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176 days

Periodic radio and X-ray emission from an accreting white dwarf binary

AuthorsKovi Rose; Joshua Pritchard; Tara Murphy; L. N. Driessen; D. L. Kaplan; M. Caleb; Ziteng Wang; A. Zic; I. Andreoni; J. Carney; B. N. Barlow; D. Dobie; M. Gu; G. Heald; D. Huber; E. Lenc; J. K. Leung; W. Lu; R. Momose; M. G. Pedersen; Y. Qu; N. Rea; I. de Ruiter; K. Shaji; G. R. Sivakoff; A. J. M. Thomson; Y. L. Wang; G. J. Yang; F. Zahedy

Affiliations1. Sydney Institute for Astronomy, School of Physics, The University of Sydney, Sydney, Australia; 2. Australia Telescope National Facility, CSIRO, Space & Astronomy, Epping, Australia; 3. ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), Hawthorn, Australia; 4. Center for Gravitation, Cosmology, and Astrophysics, Department of Physics and Astronomy, University of Wisconsin-Milwaukee, Milwaukee, USA; 5. International Centre for Radio Astronomy Research, Curtin University, Bentley, Australia; 6. Department of Physics and Astronomy, University of North Carolina, Chapel Hill, USA; 7. Department of Astronomy, Tsinghua University, Beijing, China; 8. The Hong Kong Institute for Astronomy and Astrophysics, The University of Hong Kong, Hong Kong, China; 9. SKA Observatory, SKA-Low Science Operations Centre, Kensington, Australia; 10. Australia Telescope National Facility, CSIRO, Space & Astronomy, Kensington, Australia; 11. Institute for Astronomy, University of Hawai’i, Honolulu, USA; 12. David A. Dunlap Department of Astronomy and Astrophysics, University of Toronto, Toronto, Canada; 13. Dunlap Institute for Astronomy and Astrophysics, University of Toronto, Toronto, Canada; 14. Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, Israel; 15. Department of Astronomy and Theoretical Astrophysics Center, University of California at Berkeley, Berkeley, USA; 16. Carnegie Science Observatories, Pasadena, USA; 17. Department of Astronomy, School of Science, The University of Tokyo, Bunkyo-ku, Japan; 18. Nevada Center for Astrophysics, University of Nevada, Las Vegas, USA; 19. Department of Physics and Astronomy, University of Nevada Las Vegas, Las Vegas, USA; 20. Institute of Space Sciences, ICE-CSIC, Barcelona, Spain; 21. Institut d’Estudis Espacials de Catalunya, Castelldefels, Spain; 22. Department of Physics, University of Alberta, Edmonton, Canada; 23. National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China; 24. School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, China; 25. Department of Physics, University of North Texas, Denton, USA

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251 days

A modern dynamo at Triton as a consequence of its capture by Neptune

AuthorsLana J. Tilke; Kevin T. Trinh; Joseph G. O’Rourke

Affiliations1. School of Earth and Space Exploration, Arizona State University, Tempe, USA; 2. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, USA

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Machine Learning and Life-Cycle Assessment for Predicting and Optimizing Carbon Emissions in Urban Wastewater Treatment

SampleLatest 5 valid paper samples from 2026

Average review96.4 days

Median77 days

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