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291.7Average days
226Median days
121Fastest days
677Longest days
2932025 publications

Paper Review Records

All Paper Review Records

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

360 days

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

Authors
TAMBO collaborationShow moreShow less
Affiliations
1. 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, PerúShow moreShow less
Source PDF DOI Publisher page
145 days

The multimessenger Universe as a training ground for frontier AI

Authors
Abigail 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 NowickiShow moreShow less
Affiliations
1. 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, SwitzerlandShow moreShow less
Source PDF DOI Publisher page
342 days

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

Authors
Ke 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 ValentinoShow moreShow less
Affiliations
1. 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, DenmarkShow moreShow less
Source PDF DOI Publisher page
121 days

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

Authors
Yuji Urata; Kuiyun Huang; Bunyo Hatsukade; Mansi Kasliwal; Shigeo S. Kimura; Yuichi Matsuda; Yusuke Miyamoto; Hiroshi Nagai; Kouichiro Nakanishi; Robert SteinShow moreShow less
Affiliations
1. 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, USAShow moreShow less
Source PDF DOI Publisher page
226 days

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

Authors
Dominik 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 WallnerShow moreShow less
Affiliations
1. 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, GermanyShow moreShow less
Source PDF DOI Publisher page
477 days

On the tidal response of Titan inferred from Cassini data

Authors
Daniele Durante; Luciano Iess; Valery LaineyShow moreShow less
Affiliations
1. Sapienza University of Rome, Rome, Italy; 2. LTE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Université, Université de Lille, Lille, FranceShow moreShow less
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Machine Learning and Life-Cycle Assessment for Predicting and Optimizing Carbon Emissions in Urban Wastewater Treatment

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Median65 days

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