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Hard Times for These Times (1Dec92) (from the Director's Office, NOAO Newsletter No. 32, 1 December 1992) NOAO users and management have gained a growing awareness in recent weeks that there appears to be a fundamental change in the way that Congress approaches funding for basic research and that NSF is preparing to respond to that change. In October, Kent Wilson (Acting Director of the Astronomy Division of the NSF) visited Tucson and addressed a joint meeting of the CTIO and KPNO Users' Committees. The following week, a group from NOAO attended the Advisory Committee of the Astronomy Division (ACAST) meeting in Washington, during which we heard from Walter Massey (Director of the NSF) and Bill Harris (Associate Director for the Math and Physical Sciences Division). The deep issue is that the rationale for supporting basic research is undergoing careful scrutiny and fundamental revision. That support was originally sold to Congress on the basis of strengthening defense, increasing economic competitiveness, and improving health care. The Cold War is over, the status of the US economy is a subject of considerable debate, and the control of health care costs is now a major issue. There is a growing sentiment in Congress that they wish to see more accountability in terms of direct return on their research investment. Consequences include an increased emphasis on research with direct application, an increased involvement of the "end users" (i.e., in industry and education) in the evaluation of the effectiveness of funded programs, and a generally closer coupling of supported research to defined societal goals. The NSF is receiving advice from a commission of the National Science Board on how to increase its involvement as an interface between university and national laboratory research and industrial application. That commission received over 600 letters from the research community in reaction to this contemplated new direction. The exact structure of such a new interface is yet to be decided, but two trends seem very clear. One is that the current intention of NSF is to move in the direction of supporting technology transfer and research of interest to industry and of value to economic competitiveness. The second is that fields of research with easily identifiable application, such as materials science, will have a demonstrably stronger claim to funding priority. The development of this year's funding situation provides a portent for the near-term direction of astronomy support. Despite a strong request in the President's budget, the House-Senate conference committee finally committed to a total allocation for Research and Related Activities (our grants and centers) that is about 1% less than last year's total. However, this year's bill contained an unprecedented level of direction for the NSF, both in terms of fields of emphasis and individually earmarked projects. To show allocations responsive to Congressional guidelines in targeted science areas, the NSF has to reduce the other areas of the program, given the flat funding profile. As a result, at the time of this writing, the budget for the Astronomy Division was starting out at a level down by about 10% from last year's. The NSF then must wrestle with accommodating the three projects earmarked for Math and Physical Sciences: LIGO, Gemini and the High Magnetic Fields Lab. The consequence for NOAO must inevitably be reduced support for the current fiscal year. Many university departments have suffered similar difficulties recently, but there is an important difference. In many cases, the universities had been enjoying a period of substantial growth prior to the current downturn. NOAO has incurred a loss of support of over 20% in real terms in the last ten years. There is little to no flexibility left to respond to a sharp reduction in funding by imposing across the board cuts. Each division within the observatories is now struggling to define new modes of operation. The goal is to preserve as much access as possible to the telescope data stream (even if not directly to the telescopes) and to maintain the core of excellence in instrument development that makes forefront science possible and leads to a defining role for NOAO in the era of Gemini and new solar physics projects. In this context, I would like your input on two very general questions. What are the aspects of NOAO that are most important to you and should receive the highest priority for sustained support? For example, there are several models of nighttime operation that could be considered. Resources could be concentrated on the largest aperture telescopes, with the smaller instruments closed or given over to consortia. Limited direct access could be given to the broader range of telescopes, with a substantial increase in queue scheduling for the programs with fewer requirements for real-time decision making. Significant shares of telescope time could be "sold" to user groups in exchange for operations or instrumentation development support. Do you view the availability of reliable, cutting-edge instrumentation as critical to your programs? Does NOAO's active development of data reduction or instrument interface software strongly benefit your research productivity? The other question is: How can we successfully promote ground-based optical astronomy, both solar and night-time, in an era of emphasis on applied research and measurable return on research investment? We as a community must develop that case and be prepared to offer it high visibility to justify continuing support in an increasingly competitive environment. The notion of research funding as an entitlement based solely on excellence is coming under sharp attack. Should we emphasize our impact on the general public, on attracting young people to scientific careers, and on training researchers of high caliber to enhance the relevance of our field? Should we attempt to define a set of priorities for operations, infrastructure, and grants in the same spirit as project prioritization in the decade surveys, in order to offer a more united voice to our funding agencies? NOAO takes pride in the unique combination of facilities and instrumentation that it offers to its users and in the level of support it provides in maintaining the quality of the data obtained here. We anticipate a strong future through the vitality of our current facilities and in our role as the focus for the US participation in the Gemini Project and in new solar physics initiatives. We ask your advice on our choice of new, reduced operating modes so that we can be positioned for maximum effectiveness to achieve our shared goal of US leadership in astronomical science. Please send your responses to me, rgreen@noao.edu. Richard F. Green
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