LEADER 04590nam 2200745 450 001 9910796108603321 005 20200520144314.0 010 $a0-8122-9189-1 024 7 $a10.9783/9780812291896 035 $a(CKB)3790000000033271 035 $a(EBL)4321853 035 $a(SSID)ssj0001545543 035 $a(PQKBManifestationID)16135531 035 $a(PQKBTitleCode)TC0001545543 035 $a(PQKBWorkID)12994637 035 $a(PQKB)11459064 035 $a(OCoLC)921007970 035 $a(MdBmJHUP)muse46663 035 $a(DE-B1597)452780 035 $a(OCoLC)952799454 035 $a(DE-B1597)9780812291896 035 $a(Au-PeEL)EBL4321853 035 $a(CaPaEBR)ebr11149341 035 $a(CaONFJC)MIL829224 035 $a(OCoLC)935259514 035 $a(MiAaPQ)EBC4321853 035 $a(EXLCZ)993790000000033271 100 $a20160210h20162016 uy 0 101 0 $aeng 135 $aur|||||||nn|n 181 $ctxt 182 $cc 183 $acr 200 14$aThe 4-H harvest $esexuality and the state in rural America /$fGabriel N. Rosenberg 210 1$aPhiladelphia, Pennsylvania :$cUniversity of Pennsylvania Press,$d2016. 210 4$dİ2016 215 $a1 online resource (301 p.) 225 1 $aPolitics and Culture in Modern America 300 $aIncludes index. 311 $a0-8122-4753-1 320 $aIncludes bibliographical references and index. 327 $tFront matter --$tContents --$tList of Abbreviations --$tIntroduction. Signs of the State --$tChapter 1. Agrarian Futurism, Rural Degeneracy, and the Origins of 4-H --$tChapter 2. Financial Intimacy and Rural Manhood --$tChapter 3. 4-H Body Politics in the 1920's --$tChapter 4. Conserving Farm and Family in New Deal 4-H --$tChapter 5. Citizenship and Difference in Wartime 4-H --$tChapter 6. International 4-H in the Cold War --$tEpilogue. Future Farmers of Afghanistan: Agrarian Futurism at the Twilight of Empire --$tNotes --$tIndex --$tAcknowledgments 330 $a4-H, the iconic rural youth program run by the U.S. Department of Agriculture, has enrolled more than 70 million Americans over the last century. As the first comprehensive history of the organization, The 4-H Harvest tracks 4-H from its origins in turn-of-the-century agricultural modernization efforts, through its role in the administration of federal programs during the New Deal and World War II, to its status as an instrument of international development in Cold War battlegrounds like Vietnam and Latin America. In domestic and global settings, 4-H's advocates dreamed of transforming rural economies, communities, and families. Organizers believed the clubs would bypass backward patriarchs reluctant to embrace modern farming techniques. In their place, 4-H would cultivate efficient, capital-intensive farms and convince rural people to trust federal expertise. The modern 4-H farm also featured gender-appropriate divisions of labor and produced healthy, robust children. To retain the economic potential of the "best" youth, clubs insinuated state agents at the heart of rural family life. By midcentury, the vision of healthy 4-H'ers on family farms advertised the attractiveness of the emerging agribusiness economy. With rigorous archival research, Gabriel N. Rosenberg provocatively argues that public acceptance of the political economy of agribusiness hinged on federal efforts to establish a modern rural society through effective farming technology and techniques as well as through carefully managed gender roles, procreation, and sexuality. The 4-H Harvest shows how 4-H, like the countryside it often symbolizes, is the product of the modernist ambition to efficiently govern rural economies, landscapes, and populations. 410 0$aPolitics and culture in modern America. 606 $a4-H clubs$zUnited States$xHistory 606 $aSociology, Rural$y20th century$xHistory$y20th century 606 $aAgriculture$zUnited States$xSocial aspects$xHistory$y20th century 607 $aUnited States$xRural conditions 610 $aAgriculture. 610 $aAmerican History. 610 $aAmerican Studies. 610 $aGender Studies. 610 $aWomen's Studies. 615 0$a4-H clubs$xHistory. 615 0$aSociology, Rural$xHistory 615 0$aAgriculture$xSocial aspects$xHistory 676 $a630.6073 700 $aRosenberg$b Gabriel N.$01565256 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910796108603321 996 $aThe 4-H harvest$93834751 997 $aUNINA LEADER 09673nam 22006013 450 001 9910346694803321 005 20230527060419.0 010 $a9789813270107 010 $a9813270101 010 $a9789813270091 010 $a9813270098 035 $a(CKB)4100000007992398 035 $a(oapen)https://directory.doabooks.org/handle/20.500.12854/58998 035 $a(MiAaPQ)EBC6204152 035 $a(Au-PeEL)EBL6204152 035 $a(OCoLC)1164493310 035 $a(Perlego)978989 035 $a(oapen)doab58998 035 $a(EXLCZ)994100000007992398 100 $a20230527d2018 uy 0 101 0 $aeng 135 $aurmn|---annan 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aScience With The Cherenkov Telescope Array 210 $cWorld Scientific Publishing Co$d2019 210 1$aSingapore :$cWorld Scientific Publishing Company,$d2018. 210 4$dİ2019. 215 $a1 electronic resource (364 p.) 311 08$a9789813270084 311 08$a981327008X 327 $aIntro -- Contents -- Executive Summary -- Authors -- Acknowledgements -- Chapters and Corresponding Authors -- Chapter 1. Introduction to CTA Science -- 1.1 Key Characteristics and Capabilities -- 1.1.1 Surveying Capabilities -- 1.1.2 Short Timescale Capabilities -- 1.1.3 Capabilities Beyond Gamma Rays -- 1.2 Overview of CTA Science Themes -- 1.2.1 Understanding the Origin and Role of Relativistic Cosmic Particles -- 1.2.1.1 Cosmic accelerators -- 1.2.1.2 Propagation and influence of accelerated particles -- 1.2.2 Probing Extreme Environments -- 1.2.2.1 Black holes and jets -- 1.2.2.2 Neutron stars and relativistic outflows -- 1.2.2.3 Cosmic voids -- 1.2.3 Exploring Frontiers in Physics -- 1.2.3.1 Dark matter -- 1.2.3.2 Quantum gravity and axion-like particle search -- 1.3 Community Input to the Science Case -- Chapter 2. Synergies -- 2.1 Radio to (Sub)Millimetre -- 2.2 Infrared/Optical through Ultraviolet and Transient Factories -- 2.3 X-ray -- 2.4 Sub-VHE Gamma-ray Energies -- 2.5 Complementary VHE Gamma-ray Instruments -- 2.6 VHE and UHE Neutrinos -- 2.7 Gravitational Waves -- Chapter 3. Core Programme Overview -- Chapter 4. Dark Matter Programme -- 4.1 Science Targeted -- 4.1.1 Existence of Dark Matter -- 4.1.2 Distribution of Dark Matter -- 4.1.3 The Nature of Dark Matter -- 4.1.4 Search Methods for Dark Matter -- 4.1.5 Annihilation of Dark Matter Particles -- 4.1.6 Parameters Expected for WIMP Dark Matter -- 4.1.7 Rate of Gamma Rays in Detector -- 4.2 Strategy -- 4.2.1 Milky Way -- 4.2.1.1 Description -- 4.2.1.2 Evolution of knowledge -- 4.2.1.3 Observational strategy -- 4.2.1.4 Performance -- 4.2.2 Dwarf Spheroidal Galaxies and Dark Clumps -- 4.2.2.1 Description -- 4.2.2.2 Evolution of knowledge -- 4.2.2.3 Observational strategy -- 4.2.2.4 Performance -- 4.2.3 Large Magellanic Cloud -- 4.2.3.1 Description -- 4.2.3.2 Evolution of knowledge. 327 $a4.2.3.3 Observational strategy -- 4.2.3.4 Performance -- 4.2.4 Clusters of Galaxies -- 4.2.5 Summary of Targets -- 4.3 Data Products -- Chapter 5. KSP: Galactic Centre -- 5.1 Science Targeted -- 5.1.1 Scientific Objectives -- 5.1.1.1 Revealing the nature of the central gamma-ray source -- 5.1.1.2 Diffuse VHE emission: Particle acceleration in the vicinity of the Galactic Centre -- 5.1.1.3 Exploring large-scale outflows -- 5.1.1.4 Supernova remnants, pulsar-wind nebulae, and molecular clouds -- 5.1.2 Context/Advance beyond State of the Art -- 5.1.2.1 Central engine -- 5.1.2.2 Advances in the study of diffuse emission -- 5.2 Strategy -- 5.2.1 Timeline and Sub-array Choice -- 5.2.2 Relation to other KSPs -- 5.2.3 Analysis Strategy -- 5.3 Data Products -- 5.4 Expected Performance/Return -- 5.4.1 Determination of the Nature of the Central Source -- 5.4.2 A Detailed View of the Diffuse VHE Emission -- 5.4.3 Resolving New, Previously Undetectable Sources -- 5.4.4 Search for Variability in the VHE Source Near Sgr A* -- 5.4.5 Studying the Interaction of the Central Source with Neighbouring Clouds -- 5.4.6 Science Impact -- Chapter 6. KSP: Galactic Plane Survey -- 6.1 Science Targeted -- 6.1.1 Scientific Objectives -- 6.1.2 Context/Advance beyond State of the Art -- 6.1.3 Multi-wavelength/Multi-messenger Context -- 6.1.3.1 Synergy with HAWC -- 6.1.3.2 Synergies with other instruments -- 6.2 Strategy -- 6.2.1 Observation Requirements -- 6.2.2 Targets, Observation Strategy, and Follow-ups -- 6.2.3 Relation/Importance to other KSPs -- 6.3 Data Products -- 6.4 Expected Performance/Return -- 6.4.1 Performance of the CTA GPS -- 6.4.2 Source Confusion -- 6.4.3 Summary -- Chapter 7. KSP: Large Magellanic Cloud Survey -- 7.1 Science Targeted -- 7.1.1 Scientific Objectives -- 7.1.2 Context/Advance beyond State of the Art -- 7.2 Strategy -- 7.3 Data Products. 327 $a7.4 Expected Performance/Return -- Chapter 8. KSP: Extragalactic Survey -- 8.1 Science Targeted -- 8.1.1 Scientific Objectives -- 8.1.2 Context/advance beyond state of the art -- 8.2 Strategy -- 8.2.1 Possibility of Several Pointings for a given Field of View -- 8.2.2 Shallow survey versus deep survey -- 8.2.3 Targets -- 8.3 Data Products -- 8.4 Expected Performance/Return -- 8.4.1 Method -- 8.4.2 Serendipitous Discoveries during the Construction Phase -- 8.4.3 Results after the Completion of the Survey -- 8.4.4 Participation of LSTs -- 8.4.5 Prospects for Divergent Pointing -- Chapter 9. KSP: Transients -- 9.1 Science Targeted -- 9.1.1 Scientific Objectives -- 9.1.2 Context/Advance beyond State of the Art -- 9.2 Strategy -- 9.3 Data Products -- 9.4 Expected Performance/Return -- Chapter 10. KSP: Cosmic Ray PeVatrons -- 10.1 Science Targeted -- 10.1.1 Scientific Objectives -- 10.1.2 Context/Advance beyond State of the Art -- 10.1.2.1 Hadronic mechanisms and the connection with cosmic-ray origin -- 10.2 Strategy -- 10.2.1 Targets -- 10.3 Data Products -- 10.4 Expected Performance/Return -- Chapter 11. KSP: Star Forming Systems -- 11.1 Science Targeted -- 11.1.1 Scientific Objectives -- 11.1.2 Context/Advance beyond State of the Art -- 11.1.2.1 Star-forming regions -- 11.1.2.2 Star-forming galaxies -- 11.1.2.3 Starburst galaxies -- 11.1.2.4 ULIRGs -- 11.2 Strategy -- 11.3 Data Products -- 11.4 Expected Performance/Return -- 11.4.1 Star-forming Regions -- 11.4.2 Star-forming Galaxies -- 11.4.3 Starburst Galaxies -- 11.4.4 ULIRGs -- Chapter 12. KSP: Active Galactic Nuclei -- 12.1 Science Targeted -- 12.1.1 Relativistic Jets from Supermassive Black Holes -- 12.1.1.1 What are the relevant particle acceleration and emission processes in VHE blazars? How are different blazar types related?. 327 $a12.1.1.2 What causes the observed variability in AGN from time scales of a few years down to a few minutes? -- 12.1.1.3 From where does the VHE emission of radio galaxies originate? -- 12.1.1.4 Do other classes of AGN emit VHE gamma rays? -- 12.1.2 Blazars as Probes of the Universe -- 12.1.2.1 What is the spectrum of the EBL at redshift z ? 0 and how does it evolve at higher redshifts? -- 12.1.2.2 What is the strength of the IGMF? -- 12.1.3 UHECRs and Fundamental Physics -- 12.1.3.1 AGN as potential sources of UHECRs -- 12.1.3.2 Can we find signatures for the existence of axion-like particles? -- 12.1.3.3 Can we rule out Lorentz Invariance Violation? -- 12.1.4 Advance beyond State of the Art -- 12.2 Strategy -- 12.2.1 Target Selection -- 12.2.1.1 Long-term monitoring -- 12.2.1.2 AGN flare programme -- 12.2.1.3 High-quality spectra -- 12.2.1.4 Time distribution model for the AGN KSP -- 12.2.2 Multi-wavelength and Multi-messenger Coverage -- 12.3 Data Products -- 12.4 Expected Performance/Return -- 12.4.1 Guaranteed Science Return -- 12.4.2 Discovery Potential -- Chapter 13. KSP: Clusters of Galaxies -- 13.1 Science Targeted -- 13.1.1 Scientific Objectives -- 13.1.2 Context/Advance beyond State of the Art -- 13.2 Strategy -- 13.2.1 Targets -- 13.3 Data Products -- 13.4 Expected Performance/Return -- Chapter 14. Capabilities beyond Gamma Rays -- 14.1 Cosmic-Ray Nuclei -- 14.2 Cosmic-Ray Electrons -- 14.3 Optical Measurements with CTA -- Chapter 15. Appendix: Simulating CTA -- References -- Glossary. 330 $aThis book summarizes the science to be carried out by the upcoming Cherenkov Telescope Array, a major ground-based gamma-ray observatory that will be constructed over the next six to eight years. The major scientific themes, as well as core program of key science projects, have been developed by the CTA Consortium, a collaboration of scientists from many institutions worldwide. CTA will be the major facility in high-energy and very high-energy photon astronomy over the next decade and beyond. CTA will have capabilities well beyond past and present observatories. Thus, CTA's science program is expected to be rich and broad and will complement other major multiwavelength and multimessenger facilities. This book is intended to be the primary resource for the science case for CTA and it thus will be of great interest to the broader physics and astronomy communities. The electronic version (e-book) is available in open access. 606 $aGamma ray astronomy 606 $aAstronomy 615 0$aGamma ray astronomy. 615 0$aAstronomy. 676 $a522/.6862 700 $aThe Cta Consortium$01315250 701 $aOng$b Rene A$01357728 701 $aThe Cta Consortium$01315250 712 02$aCTA Consortium (Organization) 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910346694803321 996 $aScience With The Cherenkov Telescope Array$93364341 997 $aUNINA