Z. Ahmed, D. Alonso, M. Amin, R. Ansari, Evan J. Arena, K. Bandura, A. Beardsley, P. Bull, E. Castorina, Tzu-Ching Chang, R. Dav'e, J. Dillon, A. V. Engelen, A. Ewall-Wice, S. Ferraro, S. Foreman, J. Frisch, D. Green, G. Holder, D. Jacobs, Dionysios Karagiannis, A. Kaurov, L. Knox, E. Kuhn, Adrian Liu, Yin-Zhe Ma, K. Masui, T. McClintock, K. Moodley, M. Munchmeyer, L. Newburgh, A. Nomerotski, P. O'Connor, A. Obuljen, H. Padmanabhan, D. Parkinson, O. Perdereau, D. Rapetti, B. Saliwanchik, N. Sehgal, J. Shaw, C. Sheehy, E. Sheldon, R. Shirley, E. Silverstein, T. Slatyer, A. Slosar, P. Stankus, A. Stebbins, P. Timbie, G. Tucker, W. Tyndall, F. Villaescusa-Navarro, D. Wulf
{"title":"Research and Development for HI Intensity Mapping","authors":"Z. Ahmed, D. Alonso, M. Amin, R. Ansari, Evan J. Arena, K. Bandura, A. Beardsley, P. Bull, E. Castorina, Tzu-Ching Chang, R. Dav'e, J. Dillon, A. V. Engelen, A. Ewall-Wice, S. Ferraro, S. Foreman, J. Frisch, D. Green, G. Holder, D. Jacobs, Dionysios Karagiannis, A. Kaurov, L. Knox, E. Kuhn, Adrian Liu, Yin-Zhe Ma, K. Masui, T. McClintock, K. Moodley, M. Munchmeyer, L. Newburgh, A. Nomerotski, P. O'Connor, A. Obuljen, H. Padmanabhan, D. Parkinson, O. Perdereau, D. Rapetti, B. Saliwanchik, N. Sehgal, J. Shaw, C. Sheehy, E. Sheldon, R. Shirley, E. Silverstein, T. Slatyer, A. Slosar, P. Stankus, A. Stebbins, P. Timbie, G. Tucker, W. Tyndall, F. Villaescusa-Navarro, D. Wulf","doi":"10.2172/1558438","DOIUrl":null,"url":null,"abstract":"Development of the hardware, data analysis, and simulation techniques for large compact radio arrays dedicated to mapping the 21 cm line of neutral hydrogen gas has proven to be more difficult than imagined twenty years ago when such telescopes were first proposed. Despite tremendous technical and methodological advances, there are several outstanding questions on how to optimally calibrate and analyze such data. On the positive side, it has become clear that the outstanding issues are purely technical in nature and can be solved with sufficient development activity. Such activity will enable science across redshifts, from early galaxy evolution in the pre-reionization era to dark energy evolution at low redshift.","PeriodicalId":8459,"journal":{"name":"arXiv: Instrumentation and Methods for Astrophysics","volume":"18 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2019-07-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: Instrumentation and Methods for Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.2172/1558438","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 4
Abstract
Development of the hardware, data analysis, and simulation techniques for large compact radio arrays dedicated to mapping the 21 cm line of neutral hydrogen gas has proven to be more difficult than imagined twenty years ago when such telescopes were first proposed. Despite tremendous technical and methodological advances, there are several outstanding questions on how to optimally calibrate and analyze such data. On the positive side, it has become clear that the outstanding issues are purely technical in nature and can be solved with sufficient development activity. Such activity will enable science across redshifts, from early galaxy evolution in the pre-reionization era to dark energy evolution at low redshift.
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