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Shipman, Jean P. 한국의학도서관협의회 1998 한국의학도서관협의회지 Vol.25 No.2
워싱턴대학 도서관에서 실시한 이용자조사에서 전자전문문헌에 대한 Desktop access는 가장 바람직한 서비스중의 하나로 평가받았다. University of Washington의 Health Sciences Libraries(UW HSL)는 1996년 8월부터 1997년 5월까지 10개월 동안 pilot test를 실시했는데, 이테스트는 원격지 교수들에게 인터넷을 토해서 전자잡지논문의 발송 가능성 여부를 결정하기 위해서 실행되었다. 논문은 Adobe Acrobot (AA) PDF 파일형식로 받아 표준 e-mail 기능을 갖춘 MIME(Multipurpose Internet Mail Extentions)와 Web을 통해서 이용자들에게 발송되었다. 참가자들은 스캐닝된 논문을 검색하고 AA Reader 소프트웨어를 사용하여 파일을 보거나 출력했다. 이 pilot test에서는 이용자 통지와 파일삭제 과정을 자동화하기 위하여 특별한 프로그래밍 기법이 요구되었다. 페스트 참가자들은 다소 기술적인 문제점이 있음에도 불구하고 pilot test에 만족했다. 현재 UW HSL에서는 보편적인 문헌 발송방법으로 Desktop delivery를 제공하고 있다.
Data processing pipeline for <i>Herschel </i>HIFI
Shipman, R. F.,Beaulieu, S. F.,Teyssier, D.,Morris, P.,Rengel, M.,McCoey, C.,Edwards, K.,Kester, D.,Lorenzani, A.,Coeur-Joly, O.,Melchior, M.,Xie, J.,Sanchez, E.,Zaal, P.,Avruch, I.,Borys, C.,Braine, Springer-Verlag 2017 Astronomy and astrophysics Vol.608 No.-
Social Innovation: Thinking about Changing the System
Jay J. Caughron,Amanda S. Shipman,Cheryl K. Beeler 대한사고개발학회 2009 The International Journal of Creativity & Problem Vol.19 No.1
Complex social systems are increasingly faced with dynamic, emergent changes in the environments in which they exist. Some social systems appear to implement changes that allow them to adapt to their environment while others seem to struggle. There is reason to suspect that the application of mental models by multiple individuals across a given social system may influence the detection of change events as well as the nature of a social system’s response (or lack thereof) to changing conditions. It is argued that the analysis of causal variables, the avail-ability of relevant case-based knowledge, and the motivation to pursue social change will influence an individual’s ability to design and promote a social change effort as well as others’ responses to it. Implications for complex social systems, such as organizations, are discussed.
2006 WHOLE EARTH TELESCOPE OBSERVATIONS OF GD358: A NEW LOOK AT THE PROTOTYPE DBV
Provencal, J. L.,Montgomery, M. H.,Kanaan, A.,Shipman, H. L.,Childers, D.,Baran, A.,Kepler, S. O.,Reed, M.,Zhou, A.,Eggen, J.,Watson, T. K.,Winget, D. E.,Thompson, S. E.,Riaz, B.,Nitta, A.,Kleinman, S IOP Publishing 2009 The Astrophysical journal Vol.693 No.1
Provencal, J. L.,Montgomery, M. H.,Kanaan, A.,Thompson, S. E.,Dalessio, J.,Shipman, H. L.,Childers, D.,Clemens, J. C.,Rosen, R.,Henrique, P.,Bischoff-Kim, A.,Strickland, W.,Chandler, D.,Walter, B.,Wat IOP Publishing 2012 The Astrophysical journal Vol.751 No.2
<P>We report on an analysis of 308.3 hr of high-speed photometry targeting the pulsating DA white dwarf EC14012-1446. The data were acquired with the Whole Earth Telescope during the 2008 international observing run XCOV26. The Fourier transform of the light curve contains 19 independent frequencies and numerous combination frequencies. The dominant peaks are 1633.907, 1887.404, and 2504.897 mu Hz. Our analysis of the combination amplitudes reveals that the parent frequencies are consistent with modes of spherical degree l = 1. The combination amplitudes also provide m identifications for the largest amplitude parent frequencies. Our seismology analysis, which includes 2004-2007 archival data, confirms these identifications, provides constraints on additional frequencies, and finds an average period spacing of 41 s. Building on this foundation, we present nonlinear fits to high signal-to-noise light curves from the SOAR 4.1 m, McDonald 2.1 m, and KPNO 2 m telescopes. The fits indicate a time-averaged convective response timescale of tau(0) = 99.4 +/- 17 s, a temperature exponent N = 85 +/- 6.2, and an inclination angle of theta(i) = 32 degrees.9 +/- 3 degrees.2. We present our current empirical map of the convective response timescale across the DA instability strip.</P>
Redaelli, M.,Kepler, S. O.,Costa, J. E. S.,Winget, D. E.,Handler, G.,Castanheira, B. G.,Kanaan, A.,Fraga, L.,Henrique, P.,Giovannini, O.,Provencal, J. L.,Shipman, H. L.,Dalessio, J.,Thompson, S. E.,Mu Blackwell Publishing Ltd 2011 Monthly notices of the Royal Astronomical Society Vol.415 No.2
<P><B>ABSTRACT</B></P><P>PG 1351+489 is one of the 20 DBVs – pulsating helium‐atmosphere white dwarf stars – known and has the simplest power spectrum for this class of star, making it a good candidate to study cooling rates. We report accurate period determinations for the main peak at 489.334 48 s and two other normal modes using data from the Whole Earth Telescope (WET) observations of 1995 and 2009. In 2009, we detected a new pulsation mode and the main pulsation mode exhibited substantial change in its amplitude compared to all previous observations. We were able to estimate the star's rotation period, of 8.9 h, and discuss a possible determination of the rate of period change of (2.0 ± 0.9) × 10<SUP>−13</SUP> s s <SUP>−1</SUP>, the first such estimate for a DBV.</P>