Change in lithic technological organization strategies during the Middle and Later Stone Ages in east Africa

This dissertation reports on archaeological research carried out in Kenya’s central Rift Valley. The primary research objective was to investigate differences in lithic technological organization strategies among archaeological sites dating to the Middle (MSA) and Later (LSA) Stone Ages. The motivation for the project was to better understand how the development of cooperative social networks by modern humans during the late MSA enabled more effective planning of tool use during the LSA. To accomplish the research objective I analyzed six flaked stone artifact assemblages from three different archaeological sites located in the Lake Naivasha basin. Three MSA assemblages from Marmonet Drift are dated >110 ka, 110-94 ka, and 40 to 36 ka; and one LSA assemblage from Ol Tepesi dates to 19 ka. Assemblages were analyzed in four ways: 1) typological composition; 2) artifact morphometrics; 3) tool production techniques; and 4) artifact curation strategies, including use-wear analysis and retouch patterns. These assemblages provided an exceptional opportunity to examine long-term changes in human technological organization with great control over raw material quality and availability. Results of my analysis show dramatic change in lithic technological organization strategies between the MSA and LSA in terms of artifact size, shape, morphological standardization, production techniques, use, and curation. Large and heavily retouched stone artifacts, including unifacial points, scrapers, and knives, dominate MSA assemblages. Most of these tools accumulated high frequencies of use-wear traces and, along with large numbers of soft hammer retouch flakes in assemblages, indicate long artifact use-lives. These data suggest a technological organization strategy of curating large, transformable, morphologically flexible, and functionally versatile tools that had the potential to perform a wide range of unplanned tool-using activities. Conversely, smaller, thinner backed microliths with low frequencies of use-wear traces dominate LSA assemblages. End scrapers made on blades and their associated steep-edged retouch flakes represent the only major curated tool class. These data suggest that LSA technological organization strategies were geared toward the production of disposable, replaceable, and morphologically standardized tools organized in anticipation of more planned tool-using activities. The results of this research project are significant for our understanding of the evolution of human technological planning. It appears that MSA humans reacted to foraging opportunities they encountered in their environments by relying on flexible and transformable toolkits while LSA humans appear to have anticipated and strategically planned for tool-using activities with specialized toolkits. The development of cooperative social networks during the late MSA likely enhanced the ability of modern humans to plan resource acquisition strategies using mechanically efficient and standardized tool designs

Guidance for management of free-roaming community cats: a bioeconomic analysis

Objectives This study used computer simulation modeling to estimate and compare costs of different free-roaming cat (FRC) management options (lethal and non-lethal removal, trap–neuter–return, combinations of these options and no action) and their ability to reduce FRC population abundance in open demographic settings. The findings provide a resource for selecting management approaches that are well matched for specific communities, goals and timelines, and they represent use of best available science to address FRC issues. Methods Multiple FRC management approaches were simulated at varying intensities using a stochastic individual- based model in the software package Vortex. Itemized costs were obtained from published literature and expert feedback. Metrics generated to evaluate and compare management scenarios included final population size, total cost and a cost efficiency index, which was the ratio between total cost and population size reduction. Results Simulations suggested that cost-effective reduction of FRC numbers required sufficient management intensity, regardless of management approach, and greatly improved when cat abandonment was minimized. Removal yielded the fastest initial reduction in cat abundance, but trap–neuter–return was a viable and potentially more cost-effective approach if performed at higher intensities over a sufficient duration. Of five management scenarios that reduced the final population size by approximately 45%, the three scenarios that relied exclusively on removal were considerably more expensive than the two scenarios that relied exclusively or primarily on sterilization. Conclusions and relevance FRCs present a challenge in many municipalities, and stakeholders representing different perspectives may promote varying and sometimes incompatible population management policies and strategies. Although scientific research is often used to identify FRC impacts, its use to identify viable, cost-effective management solutions has been inadequate. The data provided by simulating different interventions, combined with community- specific goals, priorities and ethics, provide a framework for better-informed FRC policy and management outcomes

LSST: from Science Drivers to Reference Design and Anticipated Data Products

(Abridged) We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). A vast array of science will be enabled by a single wide-deep-fast sky survey, and LSST will have unique survey capability in the faint time domain. The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the Solar System, exploring the transient optical sky, and mapping the Milky Way. LSST will be a wide-field ground-based system sited at Cerro Pach\'{o}n in northern Chile. The telescope will have an 8.4 m (6.5 m effective) primary mirror, a 9.6 deg$^2$ field of view, and a 3.2 Gigapixel camera. The standard observing sequence will consist of pairs of 15-second exposures in a given field, with two such visits in each pointing in a given night. With these repeats, the LSST system is capable of imaging about 10,000 square degrees of sky in a single filter in three nights. The typical 5$\sigma$ point-source depth in a single visit in $r$ will be $\sim 24.5$ (AB). The project is in the construction phase and will begin regular survey operations by 2022. The survey area will be contained within 30,000 deg$^2$ with $\delta<+34.5^\circ$, and will be imaged multiple times in six bands, $ugrizy$, covering the wavelength range 320--1050 nm. About 90\% of the observing time will be devoted to a deep-wide-fast survey mode which will uniformly observe a 18,000 deg$^2$ region about 800 times (summed over all six bands) during the anticipated 10 years of operations, and yield a coadded map to $r\sim27.5$. The remaining 10\% of the observing time will be allocated to projects such as a Very Deep and Fast time domain survey. The goal is to make LSST data products, including a relational database of about 32 trillion observations of 40 billion objects, available to the public and scientists around the world.Comment: 57 pages, 32 color figures, version with high-resolution figures available from https://www.lsst.org/overvie

Search for dark matter produced in association with bottom or top quarks in √s = 13 TeV pp collisions with the ATLAS detector

A search for weakly interacting massive particle dark matter produced in association with bottom or top quarks is presented. Final states containing third-generation quarks and miss- ing transverse momentum are considered. The analysis uses 36.1 fb−1 of proton–proton collision data recorded by the ATLAS experiment at √s = 13 TeV in 2015 and 2016. No significant excess of events above the estimated backgrounds is observed. The results are in- terpreted in the framework of simplified models of spin-0 dark-matter mediators. For colour- neutral spin-0 mediators produced in association with top quarks and decaying into a pair of dark-matter particles, mediator masses below 50 GeV are excluded assuming a dark-matter candidate mass of 1 GeV and unitary couplings. For scalar and pseudoscalar mediators produced in association with bottom quarks, the search sets limits on the production cross- section of 300 times the predicted rate for mediators with masses between 10 and 50 GeV and assuming a dark-matter mass of 1 GeV and unitary coupling. Constraints on colour- charged scalar simplified models are also presented. Assuming a dark-matter particle mass of 35 GeV, mediator particles with mass below 1.1 TeV are excluded for couplings yielding a dark-matter relic density consistent with measurements

Finishing the euchromatic sequence of the human genome

The sequence of the human genome encodes the genetic instructions for human physiology, as well as rich information about human evolution. In 2001, the International Human Genome Sequencing Consortium reported a draft sequence of the euchromatic portion of the human genome. Since then, the international collaboration has worked to convert this draft into a genome sequence with high accuracy and nearly complete coverage. Here, we report the result of this finishing process. The current genome sequence (Build 35) contains 2.85 billion nucleotides interrupted by only 341 gaps. It covers ∼99% of the euchromatic genome and is accurate to an error rate of ∼1 event per 100,000 bases. Many of the remaining euchromatic gaps are associated with segmental duplications and will require focused work with new methods. The near-complete sequence, the first for a vertebrate, greatly improves the precision of biological analyses of the human genome including studies of gene number, birth and death. Notably, the human enome seems to encode only 20,000-25,000 protein-coding genes. The genome sequence reported here should serve as a firm foundation for biomedical research in the decades ahead