97 research outputs found
Thinking about "The tale of Maturanomiya" Princess Kayo
Get PDFapplication/pdfThis thesis especially discusses the Princess Kayo about “The tale of Maturanomiya” The influence of story preceding and a variety of is seen in “The tale of Maturanomiya”. A forming of princess Kayo also is influenced from preceding story. The purpose of this thesis is to clear what influences forming princess Kayo and to clear what does the story try by handling her. In this thesis, the influence of Naka no kimi at “Yoru no nezame” and Murasaki no ue at “The Tale of Genji’” pointed out first. These women was shouldering suffering. Because they have to do count on a man who has other women. The same thing can be said also to princess Kayo. Therefore, I pointed out it that she is is a successor of these women. Though she was a successor in the one side that is certainly, the problem, that is, their “Suffer of the woman” is not made a focus. This reason is that the problem, “Suffer of the woman” changes in quality at this story. This problem do not focus in women’s mind but focuses a man who becomes dilemma among women. This story depicts a man assuming that it is cool. The very important fact is Princess Kayo having been influenced another person is not only two people but also princess Shikishi. She was a woman of author（Fuziwara no Sadaie）’s yearning. The author had him accomplish the desire that ended in the yearning in the story in the reality. This story made situation fall in love by such a woman, and careless in woman’s feelings. In a word, this story of the man, by the man, for the man. In the near future,I am going to think about the problem of two heroines of the remainder. I want to continue thinking about this story, to a total.departmental bulletin pape
Archival Resources Reimagined: a Feminist Examination of the "Latin American Twentieth-century Pamphlets"
No full textIn this practicum report, I use the insights afforded by feminist scholarship and theory to analyze my experience examining the Latin American Twentieth-Century Pamphlets collection at Special Collections & University Archives, Rutgers University Libraries, a collection assembled by Robert Jackson Alexander, 1918-2010. I focus in Brazil and Guyana collections and identify political beliefs and perspectives that uncover different actors and forces in these two countries, acknowledging discriminatory structures or alternative accounts of history. I also examine the issue of organization and access tools in the management of archives and their usefulness to organize this type of collection. Finally, I present the insights on uncovered resources, along with my readings on the transnational dimensions of politics and ideologies in both collections as an area for a valuable intervention for archivists and librarians to undertake.This practicum report was submitted to fulfill the requirements for the M.A. degree in Women's and Gender Studies (2010). The Practicum Committee: Nancy Hewitt (chair), Carlos Decena, and Yana van der Meulen Rodgers
Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
No full textProperties of host haloes of Lyman-break galaxies and Lyman α emitters from their number densities and angular clustering
No full textInternational audienceWe explore empirical relations between three different populations of high-redshift galaxies and their hosting dark haloes employing the halo model approach. Specifically we consider Lyman-break galaxies (LBGs) at z~ 4 and at z~ 5, and Lyman α emitters (LAEs) at z~= 4.86, all from the Subaru Deep Field survey extending over an area of about 600 arcmin2. We adopt a halo occupation function (HOF) prescription to parametrize the properties of their hosting haloes and the efficiency of halo-dependent star formation. We find that the two LBG samples are well described by the halo model with an appropriate HOF. Comparing the model predictions with the observed number densities and the angular correlation functions for those galaxies, we obtain constraints on properties of their hosting haloes. A typical mass of hosting haloes for LBGs is 5 × 1011h-1 Msolar and the expected number of LBGs per halo is ~0.5 therefore there is an approximate one-to-one correspondence between haloes and LBGs. We also find an indication that the minimum mass of LBG hosting haloes decreases with time, although its statistical significance is not strong. We discuss the implications of these findings on the star formation history of LBGs. On the other hand, for LAEs, our simple HOF prescription fails to reproduce simultaneously the observed angular correlation function and the number density. In particular, a very high amplitude of the correlation function on scales larger than 120 arcsec cannot be easily reconciled by the HOF model; a set of parameters that account for this high correlation amplitude on large scales predict either excessive clustering on small scales or a much smaller number density than observed. While this difficulty might imply either that the distribution of LAEs within hosting haloes differs from that of dark matter, or that the strong large-scale correlation is due to the existence of an unusual, large overdense region, and so the survey region is not a representative of the z~ 5 Universe, the definite answer should wait for a much wider survey of LAEs at high redshifts
Bispectrum and nonlinear biasing of galaxies: perturbation analysis, numerical simulation and SDSS galaxy clustering
No full textWe consider nonlinear biasing models of galaxies with particular attention to a correlation between the linear and quadratic biasing coefficients, b(1) and b(2). We first derive perturbative expressions for b(1) and b(2) in halo and peak biasing models. We then discuss our computations of the power spectra and bispectra of dark matter particles and halos using N-body simulation data and of volume-limited subsamples of Sloan Digital Sky Survey (SDSS) galaxies, and determine their b(1) and b(2). We find that the values of those coefficients at linear regimes (k < 0.2 h Mpc(-1)) are fairly insensitive to the redshift-space distortion and the survey volume shape. The resulting normalized amplitudes of the bispectra, Q, for equilateral triangles are insensitive to the values of b(1), implying that b(2) indeed correlates with b(1). The present results explain the previous finding of Kayo et al. (2004, PASJ, 56, 415) for the hierarchical relation of three-point correlation functions of SDSS galaxies. While the relations between b(1) and b(2) are quantitatively different for specific biasing models, their approximately similar correlations indicate a fairly generic outcome of the biasing due to the gravity in primordial Gaussian density fields
Chasing unbiased spectra of the Universe
No full textInternational audienceThe cosmological power spectrum of the coherent matter flow is measured exploiting an improved prescription for the apparent anisotropic clustering pattern in redshift space. New statistical analysis is presented to provide an optimal observational platform to link the improved redshift distortion theoretical model to future real data sets. The statistical power as well as robustness of our method are tested against 60 realizations of 8h-3Gpc3 dark matter simulation maps mocking the precision level of upcoming wide-deep surveys. We showed that we can accurately extract the velocity power spectrum up to quasilinear scales of k∼0.1hMpc-1 at z=0.35 and up to k∼0.15hMpc-1 at higher redshifts within a couple of percentage precision levels. Our understanding of redshift space distortion is proved to be appropriate for precision cosmology, and our statistical method will guide us to a righteous path to meet the real world
Public Health Approach to Etiology of Cerebrovasular Accidents
Get PDFThough there are many studies of cerebrovascular accidents from etiological point of view, few have been reported concerning impacts of daily life to cerebrovascular accidents from the view point of public health. The author examined the interactions between human factors and his environment in the cases of cerebrovascular accidents in two areas and one group of workers. The 227 objects were selected to discuss from the patients and the dead in two rural areas by examining answeres to questionnaires, medical records by doctors, and dath certificates. The results are as follows. 1) There was a difference of incidence of cerebrovascular accidents between those two areas it was 4.35 per 1,000 adults over 40 years in Kayo, whereas 6.20 in Yao. 2) Cerebrovascular accidents often occurred at either dinning and bath room in the evening or toilet in the midnight. 3) The impacts of climate was not clear in Yao where the climate is calm, on the conrary there were observed two peaks of incidence in summer and winter in Kayo where the climate is sever. 4) There were found more frequently cerebral hemorrahge than cerebral thrombosis among male farmers in those two areas. 5) The author pointed out that not only natural impacts but also soci-economical and cultural background to cerebrovascular accidents must be discussed, such as organization of labour and so forth. 6) There were observed the evidence that chronic CS(2) exposure resulted in high incidence of hypetention and cerebrovascular accidents
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