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An Open Letter from the Optical/Infrared Panel...(1Mar94) of the Committee on Astronomy and Astrophysics (from the Director's Office, NOAO Newsletter No. 37, 1 March 1994) The Optical/Infrared Review Panel of the Committee on Astronomy and Astrophysics of the National Academy of Sciences has requested that the National Optical Astronomy Observatories circulate the following letter to our user community. The review underway by the OIR Panel may well have profound effect on the way astronomy is done well into the next century, and we urge all users of national astronomy facilities to respond to the Panel's request for input. Caty Pilachowski Most of you have probably heard that the Committee on Astronomy and Astrophysics (CAA) has formed a panel (the "OIR Panel") to recommend a strategy for optical and infrared astronomy in the US. The charge to the panel, in response to a request by Hugh Van Horn and subject to approval by the National Research Council, is as follows: 1) Assess the context in which optical and infrared astronomy will be pursued in the coming decade, including existing and planned instruments worldwide, NASA missions, and likely technological developments. This examination must consider the appropriate mission for the National Optical Astronomy Observatories (NOAO); the most effective use of NSF funds for support of facilities, instrument development, and research; and how best to structure our efforts to meet the challenges of the next decade. 2) Within this context, evaluate the mission of the NOAO and define its optimal role (including both nighttime and solar activities) relative to that of other government facilities and optical/infrared university observatories and research departments. This evaluation will take into account both the research and educational roles of the organizations. 3) Suggest and evaluate alternative strategies designed to optimize progress in the field, taking into account the funding available from various federal and nonfederal sources and projections for the future. Give advice for strategies and priorities within optical/infrared astronomy in the light of the expectation that the NSF resources available for these programs will be severely constrained in the coming decade. The OIR panel members are: Richard McCray (Chairman), Bruce Carney, Jay Gallagher, John Huchra, Ken Kellermann, Tony Tyson, Judith Pipher, and Robert Rosner. In addition, Marc Davis and Jeremiah Ostriker are liaison members from the CAA, and Jill Knapp is a liaison member from the NRC Board on Physics and Astronomy. We are expected to deliver a final report to the NSF Astronomy Division by the end of 1994; that will require us to finish a draft report by September. Our report will actually be a report of the CAA, which will have the final say on its content. Of course, a report such as this gives astronomers an opportunity to reaffirm and, we hope, strengthen the case for increased support of optical/infrared astronomy. We certainly intend to do that. However, we would not be responsive to our charge if our recommended strategy simply required such an increase. In carrying out our work, the OIR Panel will be guided by two principles. First, our recommended strategy must conform to the primary recommendation of the Bahcall Report (p. 12): "The highest priority for ground-based astronomy is the strengthening of the infrastructure for research, that is, increased support for individual research grants and for the maintenance and refurbishment of existing frontier equipment at national observatories." Second, our recommended strategy must be resilient: it must work in a pessimistic scenario for future NSF funding of optical/infrared astronomy as well as an optimistic scenario. The reference in item (2) of our charge to solar activities at NOAO has led to some uncertainty which we hope to clear up here. If our panel should recommend changes in the way that NOAO serves the astronomical community, those recommendations might have implications for the future operations of the National Solar Observatories. Therefore, we must be cognizant of the potential impact of our recommendations on solar astronomy. We do not, however, intend to address scientific priorities for solar astronomy. If our recommendations raise questions regarding scientific strategy for solar astronomy, those questions will have to be addressed elsewhere. The OIR Panel will hold its first meeting in Tucson on 24-26 February. At that meeting we will plan our work in more detail and we will open a dialogue with astronomers from NOAO and other observatories located in Arizona. We have also scheduled a meeting in Washington, DC, on 26-27 April, at which we will discuss the issues with the NSF astronomy division, and a meeting in Minneapolis, concurrent with the summer AAS meeting, at which we hope to hold a discussion with the community at large. We will hold one or two more meetings, at times and locations to be determined. We plan to consult with directors of both public and private observatories to understand better the factors driving the operating costs and the possible opportunities for achieving higher productivity through sharing facilities. We believe that we can do our work most effectively through an open process that involves maximum participation by the community. Accordingly, a substantial part of every meeting of the panel will be conducted in open session, and we will invite members of the community to present a variety of perspectives to the panel. We will also use the Internet as a tool to include all interested members of the astronomy community in the dialogue. Accordingly, we have established the following account: oirpanel@jila.colorado.edu. Please, if at all possible, use e-mail to the above address rather than hardcopy for all communication with the panel. Be sure to indicate whether your correspondence is intended as: (1) open to all interested astronomers; (2) confidential to the panel members; (3) confidential to the panel chairman. We hope that you will use option (1) unless there is a compelling reason not to. All interested astronomers will be able to read the open correspondence and dispatches from the panel through anonymous ftp: ftp jila.colorado.edu. Username: anonymous. The password "oirpanel" will automatically transfer you to the right directory. Further instructions can be found there in the file read.me. With the proliferation of large telescopes and major advances in instrumentation, optical/infrared astronomy is entering a golden age. The trick is to develop an evolutionary strategy in which all US observatories, both public and private, can be used to their maximum advantage. Perhaps new advances in technology, such as the information highway, will enable astronomers to use a greater variety of telescopes and instruments at lower cost than today. Although the charge to the panel mentions the need for a strategy to deal with the possibility of a severely constrained NSF budget, we would be missing a big opportunity if we focused exclusively on the near-term issues. The most creative thinking will probably result from asking the question: what kind of infrastructure might be possible and optimal for optical/infrared astronomy on timescales of 10, 20, 30 years from now? We hope that our colleagues won't hesitate to offer their suggestions, even if such suggestions may invite criticism. A certain level of such "creative discomfort" may yield a better result in the task before us. Richard McCray
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