The Distributed Peer Review Experiment
- Author(s)
- F. Patat, W. Kerzendorf, D. Bordelon, G. Van de Ven, T. Pritchard
- Abstract
All large, ground- and space-based astronomical facilities serving wide communities face a similar problem: in many cases the number of applications they receive in response to each call exceeds 1000. This poses a serious challenge to running an effective selection process under the classic peer-review paradigm, in which the proposals are assigned to pre-allocated panels with fixed compositions. Although, in principle, one could increase the size of the time allocation committee, this creates logistic and financial problems which place a practical limit on its maximum size, making this solution unviable beyond a certain volume of applications. For this reason, alternative solutions must be sought. One of these is the so-called Distributed Peer Review (DPR) in which, by submitting a proposal, the Principal Investigators (PIs) agree both to act as reviewers and to have their proposal reviewed by their peers. In this article we report the results of a DPR experiment run by ESO in Period 103, in parallel with the regular review by the Observing Programmes Committee (OPC).
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Michigan State University, European Southern Observatory (Germany), New York University
- Journal
- The Messenger
- Volume
- 177
- Pages
- 3-13
- ISSN
- 0722-6691
- DOI
- https://doi.org/10.18727/0722-6691/5147
- Publication date
- 09-2019
- Austrian Fields of Science 2012
- 103003 Astronomy, 103004 Astrophysics
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/718cfedd-75ac-458e-98ef-0114de0cff51