THE IMPACT OF FEDERALISM ON EDUCATION FINANCE: A COMPARATIVE ANALYSIS *

Drawing on the implications suggested by several recent studies in comparative public policy, this article examines the impact of the structure of intergovernmental relations on the patterns of distribution of educational funds. The fundamental hypothesis underlying this analysis is that differences in this structure, and in particular the distinction between federal and unitary systems of government, are systematically related to differences in distribution across and within nations. The variations in total educational allocations among eighteen nations in Europe and North America are considered in order to discover whether the aggregate funding of education, relative to a nation's wealth, is related to the structure of intergovernmental relations. Then, in a more intensive analysis, the intranational patterns of distribution are compared in four federal and four unitary systems. This analysis suggests that there is a significant difference between the two types of system in the degree to which educational policy outputs equalize the territorial disparities in wealth and effect a redistribution of funds within the nation.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/74630/1/j.1475-6765.1974.tb00752.x.pd

An overview of the mid-infrared spectro-interferometer MATISSE: science, concept, and current status

MATISSE is the second-generation mid-infrared spectrograph and imager for the Very Large Telescope Interferometer (VLTI) at Paranal. This new interferometric instrument will allow significant advances by opening new avenues in various fundamental research fields: studying the planet-forming region of disks around young stellar objects, understanding the surface structures and mass loss phenomena affecting evolved stars, and probing the environments of black holes in active galactic nuclei. As a first breakthrough, MATISSE will enlarge the spectral domain of current optical interferometers by offering the L and M bands in addition to the N band. This will open a wide wavelength domain, ranging from 2.8 to 13 um, exploring angular scales as small as 3 mas (L band) / 10 mas (N band). As a second breakthrough, MATISSE will allow mid-infrared imaging - closure-phase aperture-synthesis imaging - with up to four Unit Telescopes (UT) or Auxiliary Telescopes (AT) of the VLTI. Moreover, MATISSE will offer a spectral resolution range from R ~ 30 to R ~ 5000. Here, we present one of the main science objectives, the study of protoplanetary disks, that has driven the instrument design and motivated several VLTI upgrades (GRA4MAT and NAOMI). We introduce the physical concept of MATISSE including a description of the signal on the detectors and an evaluation of the expected performances. We also discuss the current status of the MATISSE instrument, which is entering its testing phase, and the foreseen schedule for the next two years that will lead to the first light at Paranal.Comment: SPIE Astronomical Telescopes and Instrumentation conference, June 2016, 11 pages, 6 Figure

The mid-infrared instrument for the James Webb space telescope, II: design and build

Instrumentatio

The Impact of federalism on educational spending: Patterns within and across nations

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