LEADER 03359nam 2200661Ia 450 001 9910956063803321 005 20251116165702.0 010 $a9786610262786 010 $a9780309182058 010 $a0309182050 010 $a9781280262784 010 $a1280262788 010 $a9780309551755 010 $a0309551757 035 $a(CKB)1000000000245214 035 $a(EBL)3378010 035 $a(SSID)ssj0000277086 035 $a(PQKBManifestationID)11221985 035 $a(PQKBTitleCode)TC0000277086 035 $a(PQKBWorkID)10232859 035 $a(PQKB)10921966 035 $a(MiAaPQ)EBC3378010 035 $a(Au-PeEL)EBL3378010 035 $a(CaPaEBR)ebr10091312 035 $a(CaONFJC)MIL26278 035 $a(OCoLC)61672311 035 $a(Perlego)4737869 035 $a(BIP)12806889 035 $a(EXLCZ)991000000000245214 100 $a20051104d2005 uy 0 101 0 $aeng 135 $aurcn||||||||| 181 $ctxt 182 $cc 183 $acr 200 04$aThe atacama large millimeter array (ALMA) $eimplications of a potential descope /$fCommittee to Review the Science Requirements for the Atacama Large Millimeter Array 205 $a1st ed. 210 $aWashington, D.C. $cNational Academies Press$dc2005 215 $a1 online resource (48 p.) 300 $aDescription based upon print version of record. 311 08$a9780309096942 311 08$a0309096944 327 $a""Front Matter""; ""Preface""; ""Acknowledgment of Reviewers""; ""Contents""; ""Summary""; ""1 Introduction""; ""2 Technical Performance Specifications""; ""3 Performance Degradation""; ""4 The Threshold for Transformational Science""; ""5 Minimum Number of Antennas""; ""Appendixes""; ""Appendix A Letter of Request""; ""Appendix B ALMA Level-1 Science Requirements"" 330 $aThe 1991 NRC decadal survey for astronomy and astrophysics included a project called the Millimeter Array (MMA). This instrument would be an array of millimeter-wavelength telescopes intended to capture images of star-forming regions and distant star-burst galaxies. With the addition of contributions form Europe, the MMA evolved into the Atacama Large Millimeter Array (ALMA), a proposed array of 64, 12-meter antennas. The project is now part of the NSF Major Research Equipment and Facilities budget request. Increased costs, however, have forced the NSF to reconsider the number of antennas. To help with that review, NSF asked the NRC to assess the scientific consequences of reducing the number of active antennas from 60 to either 50 or 40. This report presents an assessment of the effect of downsizing on technical performance specifications, performance degradation, and the ability to perform transformational science, and of the minimum number of antennas needed. 606 $aRadar 606 $aDetectors 615 0$aRadar. 615 0$aDetectors. 676 $a522.682 712 02$aNational Research Council (U.S.).$bCommittee to Review the Science Requirements for the Atacama Large Millimeter Array. 712 02$aNational Research Council (U.S.).$bCommittee on Astronomy and Astrophysics. 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910956063803321 996 $aThe atacama large millimeter array (ALMA)$94365955 997 $aUNINA