55 research outputs found
Low temperature formation of low resistivity W contact with ultra thin mixed layer on molecular layer epitaxially-grown GaAs
Proceedings of the IEEE 24th international symposium on compound semiconductors, San diego, California, 8-11 Semptember 199
Obliquity of an Earth-like planet from frequency modulation of its direct imaged lightcurve: mock analysis from general circulation model simulation
Direct-imaging techniques of exoplanets have made significant progress
recently, and will eventually enable to monitor photometric and spectroscopic
signals of earth-like habitable planets in the future. The presence of clouds,
however, would remain as one of the most uncertain components in deciphering
such direct-imaged signals of planets. We attempt to examine how the planetary
obliquity produce different cloud patterns by performing a series of GCM
(General Circulation Model) simulation runs using a set of parameters relevant
for our Earth. Then we use the simulated photometric lightcurves to compute
their frequency modulation due to the planetary spin-orbit coupling over an
entire orbital period, and attempt to see to what extent one can estimate the
obliquity of an Earth-twin. We find that it is possible to estimate the
obliquity of an Earth-twin within the uncertainty of several degrees with a
dedicated 4 m space telescope at 10 pc away from the system if the stellar flux
is completely blocked. While our conclusion is based on several idealized
assumptions, a frequency modulation of a directly-imaged earth-like planet
offers a unique methodology to determine its obliquity.Comment: 29 pages, 18 figures, accepted for publication in Ap
Current Performance and On-Going Improvements of the 8.2 m Subaru Telescope
An overview of the current status of the 8.2 m Subaru Telescope constructed
and operated at Mauna Kea, Hawaii, by the National Astronomical Observatory of
Japan is presented. The basic design concept and the verified performance of
the telescope system are described. Also given are the status of the instrument
package offered to the astronomical community, the status of operation, and
some of the future plans. The status of the telescope reported in a number of
SPIE papers as of the summer of 2002 are incorporated with some updates
included as of 2004 February. However, readers are encouraged to check the most
updated status of the telescope through the home page,
http://subarutelescope.org/index.html, and/or the direct contact with the
observatory staff.Comment: 18 pages (17 pages in published version), 29 figures (GIF format),
This is the version before the galley proo
First Data Release of the Hyper Suprime-Cam Subaru Strategic Program
The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered
imaging survey aimed at addressing some of the most outstanding questions in
astronomy today, including the nature of dark matter and dark energy. The
survey has been awarded 300 nights of observing time at the Subaru Telescope
and it started in March 2014. This paper presents the first public data release
of HSC-SSP. This release includes data taken in the first 1.7 years of
observations (61.5 nights) and each of the Wide, Deep, and UltraDeep layers
covers about 108, 26, and 4 square degrees down to depths of i~26.4, ~26.5, and
~27.0 mag, respectively (5sigma for point sources). All the layers are observed
in five broad bands (grizy), and the Deep and UltraDeep layers are observed in
narrow bands as well. We achieve an impressive image quality of 0.6 arcsec in
the i-band in the Wide layer. We show that we achieve 1-2 per cent PSF
photometry (rms) both internally and externally (against Pan-STARRS1), and ~10
mas and 40 mas internal and external astrometric accuracy, respectively. Both
the calibrated images and catalogs are made available to the community through
dedicated user interfaces and database servers. In addition to the pipeline
products, we also provide value-added products such as photometric redshifts
and a collection of public spectroscopic redshifts. Detailed descriptions of
all the data can be found online. The data release website is
https://hsc-release.mtk.nao.ac.jp/.Comment: 34 pages, 20 figures, 7 tables, moderate revision, accepted for
publication in PAS
病床機能報告を用いた医療提供体制における地域性の検討
京都府立医科大学大学院生命基礎数理学京都府立医科大学大学院地域保健医療福祉行政システム学奈良県立医科大学地域医療学講座和歌山大学観光学部京都府立大学大学院生命環境科学研究科京都先端科学大学健康医療学部地域医療構想は、医療計画の一部として持続可能な社会保障制度の確立に重要な役割を担っている。現在、超高齢社会にも耐えうる医療提供体制の構築に向けて、地域の実情に合わせた病床機能分化の定量的な基準が検討されている。本報告は、病床機能報告データを用いて、全国の各都道府県および2 次医療圏の病床機能区分割合を算出し、空間パターン解析を実施した。その結果、都道府県別は、高度急性期と急性期の病床割合が、東日本において高い値の集積(ホットスポット)、西日本において低い値の集積(コールドスポット)が広範囲で統計的有意に認められた。一方で、2次医療圏別では広域なスポットの特徴はみられなかった。本結果は、病床機能区分割合の地域性があることを示し、地域医療提供体制の構築に有用な情報である
High resolution imaging polarimetry of HL Tau and magnetic field structure
We present high quality near infrared imaging polarimetry of HL Tau at 0.4 to
0.6 arcsec resolution, obtained with Subaru/CIAO and UKIRT/IRCAM. 3-D Monte
Carlo modelling with aligned oblate grains is used to probe the structure of
the circumstellar envelope and the magnetic field, as well as the dust
properties. At J band the source shows a centrosymmetric pattern dominated by
scattered light. In the H and K bands the central source becomes visible and
its polarisation appears to be dominated by dichroic extinction, with a
position angle inclined by ~40 degrees to the disc axis. The polarisation
pattern of the environs on scales up to 200 AU is consistent with the same
dichroic extinction signature superimposed on the centrosymmetric scattering
pattern. These data can be modelled with a magnetic field which is twisted on
scales from tens to hundreds of AU, or alternatively by a field which is
globally misaligned with the disc axis. A unique solution to the field
structure will require spatially resolved circular polarisation data. The best
fit Monte Carlo model indicates a shallow near infrared extinction law. When
combined with the observed high polarisation and non-negligible albedo these
constraints can be fitted with a grain model involving dirty water ice mantles
in which the largest particles have radii slightly in excess of 1 um. The best
fit model has an envelope structure which is slightly flattened on scales up to
several hundred AU. Both lobes of the bipolar outflow cavity contain a
substantial optical depth of dust (not just within the cavity walls). Curved,
approximately parabolic, cavity walls fit the data better than a conical
cavity. The small inner accretion disc observed at millimetre wavelengths is
not seen at this spatial resolution.Comment: Accepted by MNRAS, 21 pages, 10 figure
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