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Institution

Earlham College

EducationRichmond, Indiana, United States
About: Earlham College is a education organization based out in Richmond, Indiana, United States. It is known for research contribution in the topics: Population & Turtle (robot). The organization has 388 authors who have published 556 publications receiving 14286 citations. The organization is also known as: Earlham.


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Journal ArticleDOI
Monika Böhm1, Ben Collen1, Jonathan E. M. Baillie1, Philip Bowles2  +240 moreInstitutions (95)
TL;DR: The results provide the first analysis of the global conservation status and distribution patterns of reptiles and the threats affecting them, highlighting conservation priorities and knowledge gaps which need to be addressed urgently to ensure the continued survival of the world’s reptiles.

720 citations

Journal ArticleDOI
A-Li Luo1, Yong-Heng Zhao1, Gang Zhao1, Licai Deng1, Xiaowei Liu2, Yipeng Jing1, Gang Wang1, Haotong Zhang1, Jianrong Shi1, Xiangqun Cui1, Yaoquan Chu3, Guoping Li1, Zhong-Rui Bai1, Yue Wu1, Yan Cai1, Shu-Yun Cao1, Zihuang Cao1, Jeffrey L. Carlin4, Jeffrey L. Carlin5, Hai-Yuan Chen1, Jian-Jun Chen1, Kunxin Chen1, Li Chen1, Xuelei Chen1, Xiao-Yan Chen1, Ying Chen1, Norbert Christlieb6, Jia-Ru Chu3, Chenzhou Cui1, Yi-Qiao Dong1, Bing Du1, Dongwei Fan1, Lei Feng1, Jian-Ning Fu7, Peng Gao1, Xuefei Gong1, Bozhong Gu1, Yan-Xin Guo1, Zhanwen Han1, Boliang He1, Jinliang Hou1, Yong-Hui Hou1, Wen Hou1, Hong-Zhuan Hu3, Ning-Sheng Hu1, Zhongwen Hu1, Zhi-Ying Huo1, Lei Jia1, Fang-Hua Jiang1, Xiang Jiang1, Zhibo Jiang1, Ge Jin3, Xiao Kong1, Xu Kong3, Ya-Juan Lei1, Aihua Li1, Changhua Li1, Guang-Wei Li1, Haining Li1, Jian Li1, Qi Li1, Shuang Li1, Sha-Sha Li1, Li Xinnan1, Yan Li1, Yin-Bi Li1, Ye-Ping Li1, Yuan Liang1, Chien-Cheng Lin1, Chao Liu1, Genrong Liu1, Guan-Qun Liu1, Zhi-Gang Liu3, Wen-Zhi Lu1, Yu Luo1, Yin-Dun Mao1, Heidi Jo Newberg5, Ji-Jun Ni1, Zhaoxiang Qi1, Yong-Jun Qi1, Shiyin Shen1, Huo-Ming Shi1, J. Song1, Yi-Han Song1, Ding-qiang Su1, Hongjun Su1, Zheng-Hong Tang1, Qing-Sheng Tao1, Yuan Tian1, Dan Wang1, D. Wang1, Fengfei Wang1, Guo-Min Wang1, Hai Wang1, Hongchi Wang1, Jian Wang3, Jia-Ning Wang1, Jianling Wang1, Jian-Ping Wang3, Junxian Wang3, Lei Wang1, Meng-Xin Wang1, Shou-Guan Wang1, Shu-Qing Wang1, Xia Wang1, Ya-nan Wang1, You Wang1, Yue-Fei Wang1, Y. Wang1, Peng Wei1, Ming-Zhi Wei1, Hong Wu1, Ke-Fei Wu1, Xue-Bing Wu2, Y. Wu1, Xiao-Zheng Xing3, Lingzhe Xu1, Xin-Qi Xu1, Yan Xu1, Tai-Sheng Yan1, Dehua Yang1, Haifeng Yang1, Hui-Qin Yang1, Ming Yang1, Zheng-Qiu Yao1, Yong Yu1, H.-L. Yuan1, Haibo Yuan2, Hailong Yuan1, Wei-Min Yuan1, Chao Zhai3, En-Peng Zhang1, Huawei Zhang2, Jian-Nan Zhang1, Li-Pin Zhang1, Wei Zhang1, Yong Zhang1, Yanxia Zhang1, Zheng-Chao Zhang1, Ming Zhao1, Fang Zhou1, Xu Zhou1, Jie Zhu1, Yongtian Zhu1, Si-Cheng Zou1, Fang Zuo1 
TL;DR: The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs as discussed by the authors.
Abstract: The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in the LAMOST DR1. The pilot survey started in October 2011 and ended in June 2012, and the data have been released to the public as the LAMOST Pilot Data Release in August 2012. The regular survey started in September 2012, and completed its first year of operation in June 2013. The LAMOST DR1 includes a total of 1202 plates containing 2 955 336 spectra, of which 1 790 879 spectra have observed signal-to-noise ratio (SNR)>= 1 0. All data with SNR >= 2 are formally released as LAMOST DR1 under the LAMOST data policy. This data release contains a total of 2 204 696 spectra, of which 1 944 329 are stellar spectra, 12 082 are galaxy spectra and 5017 are quasars. The DR1 not only includes spectra, but also three stellar catalogs with measured parameters: late A, FGK-type stars with high quality spectra (1 061 918 entries), A-type stars (100 073 entries), and M-type stars (121 522 entries). This paper introduces the survey design, the observational and instrumental limitations, data reduction and analysis, and some caveats. A description of the FITS structure of spectral files and parameter catalogs is also provided.

513 citations

Journal ArticleDOI
TL;DR: The water-soluble compounds of Hg that exist in flue gases (termed reactive gaseo... as mentioned in this paper ) are critical to understanding its fate once released from point sources.
Abstract: Knowledge of atmospheric mercury speciation is critical to understanding its fate once released from point sources. The water-soluble compounds of Hg that exist in flue gases (termed reactive gaseo...

477 citations

Journal ArticleDOI
Leor Barack1, Vitor Cardoso2, Vitor Cardoso3, Samaya Nissanke4  +228 moreInstitutions (101)
TL;DR: A comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress can be found in this article, which is an initiative taken within the framework of the European Action on 'Black holes, Gravitational waves and Fundamental Physics'.
Abstract: The grand challenges of contemporary fundamental physics-dark matter, dark energy, vacuum energy, inflation and early universe cosmology, singularities and the hierarchy problem-all involve gravity as a key component. And of all gravitational phenomena, black holes stand out in their elegant simplicity, while harbouring some of the most remarkable predictions of General Relativity: event horizons, singularities and ergoregions. The hitherto invisible landscape of the gravitational Universe is being unveiled before our eyes: the historical direct detection of gravitational waves by the LIGO-Virgo collaboration marks the dawn of a new era of scientific exploration. Gravitational-wave astronomy will allow us to test models of black hole formation, growth and evolution, as well as models of gravitational-wave generation and propagation. It will provide evidence for event horizons and ergoregions, test the theory of General Relativity itself, and may reveal the existence of new fundamental fields. The synthesis of these results has the potential to radically reshape our understanding of the cosmos and of the laws of Nature. The purpose of this work is to present a concise, yet comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress. This write-up is an initiative taken within the framework of the European Action on 'Black holes, Gravitational waves and Fundamental Physics'. © 2019 IOP Publishing Ltd.

314 citations

Journal ArticleDOI
30 Oct 2008-Nature
TL;DR: Jankaew et al. as mentioned in this paper used sedimentary records of earlier tsunamis preserved in the dark soils of marshy swales at Phra Thong, a barrier island in western Thailand.
Abstract: Nothing known from written history gave reason to expect the Indian Ocean tsunami that took nearly a quarter million lives on 26 December 2004. That tsunami entered geological history by laying down centimetres of sand on the coastal plains that it overran. Jankaew et al. have now found such sedimentary records of earlier tsunamis preserved in the dark soils of marshy swales at Phra Thong, a barrier island in western Thailand. The cover shows an example from a pit dug there in 2007: the topmost light-coloured layer represents the 2004 tsunami, while a similar layer below records a tsunami in the fourteenth or fifteenth century AD. The ruler divisions are 10 cm long. In a separate study in Aceh, Indonesia, Monecke et al. found the 2004 sand sheet preceded by the deposits of three tsunamis from the past 1,200 years. One of these earlier deposits may match the medieval one found in Thailand. The combined findings suggest that the 2004 tsunami is neither the first nor the last of its kind. The Indian Ocean tsunami of 26 December 2004 reached maximum wave heights of 35 m in Aceh, the northernmost province of Sumatra1,2. Both the tsunami and the associated Sumatra–Andaman earthquake were unprecedented in Acehnese history3,4. Here we use sand sheets to extend tsunami history 1,000 years into Aceh’s past. The 2004 tsunami deposited a sand sheet up to 1.8 km inland on a marshy beach ridge plain. Sediment cores from these coastal marshes revealed two older extensive sand sheets with similar sediment characteristics. These sheets, deposited soon after ad 1290–1400 and ad 780–990, probably resulted from earlier tsunamis. An additional sand sheet of limited extent might correlate with a documented smaller tsunami of ad 1907. These findings, a first step towards a palaeotsunami record for northern Sumatra, suggest that damage-causing tsunamis in Aceh recur infrequently enough for entire human lifetimes to typically elapse between them. Such recurrence adds to the challenge of preparing communities along the northern Indian Ocean shorelines for future tsunamis.

284 citations


Authors

Showing all 390 results

NameH-indexPapersCitations
James R. Miller5930215118
Richard S. Surwit5314816263
John B. Iverson451726995
Jeffrey L. Carlin391557962
Chris Smith381225259
Peter F. MacNeilage381206658
Omar S. Harb31586684
Eric B. Nelson28483026
Harvey M. Sussman26711921
Peter Suber241342252
Geoffrey R. Smith241622035
Sarah Schaack23553726
Stephen R. Humphrey22321618
Steven T. Kosak20322589
Carena J. van Riper20611454
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20227
202125
202034
201930
201827
201722