We present a measurement of the energy spectrum of ultra-high-energy cosmic rays performed by the Telescope Array experiment using monocular observations from its two new FADC-based fluorescence ...detectors. After a short description of the experiment, we describe the data analysis and event reconstruction procedures. Since the aperture of the experiment must be calculated by Monte Carlo simulation, we describe this calculation and the comparisons of simulated and real data used to verify the validity of the aperture calculation. Finally, we present the energy spectrum calculated from the merged monocular data sets of the two FADC-based detectors, and also the combination of this merged spectrum with an independent, previously published monocular spectrum measurement performed by Telescope Array's third fluorescence detector (Abu-Zayyad {\it et al.}, {Astropart. Phys.} 39 (2012), 109). This combined spectrum corroborates the recently published Telescope Array surface detector spectrum (Abu-Zayyad {\it et al.}, {Astrophys. Journ.} 768 (2013), L1) with independent systematic uncertainties.
The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic rays with primary energies above 1.6 x 10^(18) eV. This measurement is based upon four years of ...observation by the surface detector component of TA. The spectrum shows a dip at an energy of 4.6 x 10^(18) eV and a steepening at 5.4 x 10^(19) eV which is consistent with the expectation from the GZK cutoff. We present the results of a technique, new to the analysis of ultra-high energy cosmic ray surface detector data, that involves generating a complete simulation of ultra-high energy cosmic rays striking the TA surface detector. The procedure starts with shower simulations using the CORSIKA Monte Carlo program where we have solved the problems caused by use of the "thinning" approximation. This simulation method allows us to make an accurate calculation of the acceptance of the detector for the energies concerned.
We study the anisotropy of Ultra-High Energy Cosmic Ray (UHECR) events collected by the Telescope Array (TA) detector in the first 40 months of operation. Following earlier studies, we examine event ...sets with energy thresholds of 10 EeV, 40 EeV, and 57 EeV. We find that the distributions of the events in right ascension and declination are compatible with an isotropic distribution in all three sets. We then compare with previously reported clustering of the UHECR events at small angular scales. No significant clustering is found in the TA data. We then check the events with E>57 EeV for correlations with nearby active galactic nuclei. No significant correlation is found. Finally, we examine all three sets for correlations with the large-scale structure of the Universe. We find that the two higher-energy sets are compatible with both an isotropic distribution and the hypothesis that UHECR sources follow the matter distribution of the Universe (the LSS hypothesis), while the event set with E>10 EeV is compatible with isotropy and is not compatible with the LSS hypothesis at 95% CL unless large deflection angles are also assumed. We show that accounting for UHECR deflections in a realistic model of the Galactic magnetic field can make this set compatible with the LSS hypothesis.
The Telescope Array (TA) experiment, located in the western desert of Utah,USA, is designed for observation of extensive air showers from extremely high energy cosmic rays. The experiment has a ...surface detector array surrounded by three fluorescence detectors to enable simultaneous detection of shower particles at ground level and fluorescence photons along the shower track. The TA surface detectors and fluorescence detectors started full hybrid observation in March, 2008. In this article we describe the design and technical features of the TA surface detector.
The Telescope Array's Middle Drum fluorescence detector was instrumented with telescopes refurbished from the High Resolution Fly's Eye's HiRes-1 site. The data observed by Middle Drum in monocular ...mode was analyzed via the HiRes-1 profile-constrained geometry reconstruction technique and utilized the same calibration techniques enabling a direct comparison of the energy spectra and energy scales between the two experiments. The spectrum measured using the Middle Drum telescopes is based on a three-year exposure collected between December 16, 2007 and December 16, 2010. The calculated difference between the spectrum of the Middle Drum observations and the published spectrum obtained by the data collected by the HiRes-1 site allows the HiRes-1 energy scale to be transferred to Middle Drum. The HiRes energy scale is applied to the entire Telescope Array by making a comparison between Middle Drum monocular events and hybrid events that triggered both Middle Drum and the Telescope Array's scintillator Ground Array.
Since 2007, the Telescope Array (TA) experiment, based in Utah, USA, has been observing ultra high energy cosmic rays to understand their origins. The experiment involves a surface detector (SD) ...array and three fluorescence detector (FD) stations. FD stations, installed surrounding the SD array, measure the air fluorescence light emitted from extensive air showers (EASs) for precise determination of their energies and species. The detectors employed at one of the three FD stations were relocated from the High Resolution Fly's Eye experiment. At the other two stations, newly designed detectors were constructed for the TA experiment. An FD consists of a primary mirror and a camera equipped with photomultiplier tubes. To obtain the EAS parameters with high accuracies, understanding the FD optical characteristics is important. In this paper, we report the characteristics and installation of new FDs and the performances of the FD components. The results of the monitored mirror reflectance during the observation time are also described in this report.
This study was conducted to investigate the effects of sex hormones upon the nature of soluble immune response suppressor (SIRS) produced by concanavalin A-stimulated Lyt-2+ T cells. Conventional ...SIRS affected IgM PFC only. However, SIRS made with progesterone (20-400 ng/ml or Prog-SIRS) suppressed IgM PFC, one-way MLR, and generation CTL; and SIRS made with estrogen (0.2-50 ng/ml or Est-SIRS) enhanced these responses. The factor(s) (MW 40,000-55,000) to stimulate macrophages to produce the second soluble factor (M phi-SF) was isolated from all preparations by gel filtration. Furthermore, Est-SIRS contained a factor(s) (MW 10,000-30,000) to enhance IgM PFC, MLR, and mitogen-induced blastogenesis of both T and B cells; and Prog-SIRS possessed the suppressive factor(s) to IgM PFC, MLR, and mitogen-induced T-cell proliferation. These activities were not impaired by 2-mercaptoethanol. Moreover, the suppressive activity of Prog-SIRS was completely absorbed by T cells only, but the enhancing activity of Est-SIRS was not completely absorbed by a single-cell population. These data suggest that progesterone can contribute to the suppression of allograft rejection through soluble factors, and estrogen can enhance host responses which may be affected by several soluble factors during pregnancy.
We have encountered 3 patients with a small aortic annulus for whom the conventional posterior enlargement alone was not extensive enough to implant an artificial valve of acceptable size. Therefore, ...we performed two-directional enlargement, which is a combination of posterior and anterior enlargement. First, the posterior enlargement was done, and then an additional aortotomy was made anteriorly and extended to the ventricular septum. The aortic annulus was enlarged by 68% after the two-directional enlargement. At a follow-up of 31 months, the patients’ functional status was New York Heart Association class I.
(Ann Thorac Surg 1997;63:261–3)
The present study was carried out to ascertain whether the active component of Corynebacterium kutscheri (CK-M) could stimulate host cells of mice to produce several cytokines. CK-M stimulated ...thioglycollate-induced peritoneal macrophages to produce interleukin 1 (IL-1) and tumor necrosis factor alpha (TNF-alpha) at concentrations of 1-100 ng/ml, and it also induced IL-2 and interferon-gamma (IFN-gamma) as well as IL-6 production by splenocytes. Maximum production of each cytokine induced by CK-M was obtained at the following doses: IL-1 at 5 ng/ml, TNF-alpha at 50 ng/ml, IL-2 at 1 microgram/ml, IL-6 at 500 ng/ml and IFN-gamma at 750 ng/ml. In contrast, IL-4 was not produced to a significant extent by CK-M-stimulated splenocytes. Furthermore, when mice were intravenously injected with 20 micrograms of CK-M, IL-2 and IFN-gamma production by splenocytes, upon stimulation with either formalin-killed C. kutscheri or mitogens, was significantly higher on day 10 of treatment than on day 2. Additionally, the cytotoxicity to L929 cells of this serum from CK-M-treated mice increased with time, and the activity in the serum of day 10 was not abrogated by the antibody to TNF-alpha. Data obtained here indicate that CK-M may preferentially stimulate type-1 helper T cells to produce IL-2 and IFN-gamma, and that the enhanced cytokine production could contribute to the nonspecific resistance induced by C. kutscheri.
