http://chineseinput.net/에서 pinyin(병음)방식으로 중국어를 변환할 수 있습니다.
변환된 중국어를 복사하여 사용하시면 됩니다.
- 中文 을 입력하시려면 zhongwen을 입력하시고 space를누르시면됩니다.
- 北京 을 입력하시려면 beijing을 입력하시고 space를 누르시면 됩니다.
RISS 인기검색어
- 검색키워드
- 저자 : Pforr, J. (검색결과 2 건)
- 무료
- 기관 내 무료
- 유료
-
Aji Cahya Nusantara,Michael Volgger,Christof Pforr 한국마케팅과학회 2021 마케팅과학연구 Vol.31 No.4
This paper discusses a recent political transition which led to changes in tourism development of the Indonesian city of Surakarta, and shifted the focus from preserving cultural uniqueness to boosting mainstream tourism infrastructure. The paper investigates impacts of such a fundamental change in tourism development policy and explores how its actions- and results-related impacts are evaluated by stakeholders. In this context, the paper adopts a relativistic stakeholder approach to impact evaluation. Findings reveal that the stark policy shift generated relatively balanced outcome assessments by interviewed stakeholders, although they criticised a lack of involvement in the decision-making process. Overall, this research contributes to impact assessment research by lending support to a relativistic and activity/process-based view. Stakeholder involvement into decision-making not only supports a continuous and critical evaluation due to the presence of a multitude of voices, but seemingly provides a counter-balance to sudden ruptures which characterize political dynamics.
-
STELLAR MASSES FROM THE CANDELS SURVEY: THE GOODS-SOUTH AND UDS FIELDS
Santini, P.,Ferguson, H. C.,Fontana, A.,Mobasher, B.,Barro, G.,Castellano, M.,Finkelstein, S. L.,Grazian, A.,Hsu, L. T.,Lee, B.,Lee, S.-K.,Pforr, J.,Salvato, M.,Wiklind, T.,Wuyts, S.,Almaini, O.,Coope IOP Publishing 2015 The Astrophysical journal Vol.801 No.2
<P>We present the public release of the stellar mass catalogs for the GOODS-S and UDS fields obtained using some of the deepest near-IR images available, achieved as part of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey project. We combine the effort from 10 different teams, who computed the stellar masses using the same photometry and the same redshifts. Each team adopted their preferred fitting code, assumptions, priors, and parameter grid. The combination of results using the same underlying stellar isochrones reduces the systematics associated with the fitting code and other choices. Thanks to the availability of different estimates, we can test the effect of some specific parameters and assumptions on the stellar mass estimate. The choice of the stellar isochrone library turns out to have the largest effect on the galaxy stellar mass estimates, resulting in the largest distributions around the median value (with a semi interquartile range larger than 0.1 dex). On the other hand, for most galaxies, the stellar mass estimates are relatively insensitive to the different parameterizations of the star formation history. The inclusion of nebular emission in the model spectra does not have a significant impact for the majority of galaxies (less than a factor of 2 for similar to 80% of the sample). Nevertheless, the stellar mass for the subsample of young galaxies (age <100 Myr), especially in particular redshift ranges (e.g., 2.2 < z < 2.4, 3.2 < z < 3.6, and 5.5 < z < 6.5), can be seriously overestimated (by up to a factor of 10 for <20 Myr sources) if nebular contribution is ignored.</P>
연관 검색어 추천
이 검색어로 많이 본 자료
활용도 높은 자료
