News, intelligence and 'little lies' : rumours between the Cherokees and the British 1740-1785

Rumour and information are one of the most fundamental ways in which people engage with one another. Rumours can change the way that individuals and groups see each other and the actions that they take. Sociologists and anthropologists have long used rumour as a way to explore the experiences of their subjects. Historians of early America have, in recent years, begun to make use of rumour as a way of examining the, often hidden, world of interactions between American Indians and white Europeans. This thesis will expand upon this work by exploring the changing role of rumour within an intercultural relationship over several decades. This thesis will focus on rumour in the relationship between the Cherokee Nation and the colonists of the British Empire. It will explore the ways that rumour influenced these interactions and the impact of the rapidly changing backcountry environment of the latter eighteenth century, both on rumour and on the wider Cherokee- British relationship. This thesis will argue that rumour shifted in the course of the eighteenth century from being a diplomatic tool which could be used- either to create further panic and confusion or to calm and smooth over problems- to an uncontrollable force which would deepen and exacerbate the divisions between Cherokees and the British. Rumour played an important role in politics and society in the eighteenth century backcountry and its changing function offers a way to better understand the shifting currents of life in early America

The eROSITA X-ray telescope on SRG

eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the primary instrument on the Spectrum-Roentgen-Gamma (SRG) mission, which was successfully launched on July 13, 2019, from the Baikonour cosmodrome. After the commissioning of the instrument and a subsequent calibration and performance verification phase, eROSITA started a survey of the entire sky on December 13, 2019. By the end of 2023, eight complete scans of the celestial sphere will have been performed, each lasting six months. At the end of this program, the eROSITA all-sky survey in the soft X-ray band (0.2-2.3 keV) will be about 25 times more sensitive than the ROSAT All-Sky Survey, while in the hard band (2.3-8 keV) it will provide the first ever true imaging survey of the sky. The eROSITA design driving science is the detection of large samples of galaxy clusters up to redshifts z > 1 in order to study the large-scale structure of the universe and test cosmological models including Dark Energy. In addition, eROSITA is expected to yield a sample of a few million AGNs, including obscured objects, revolutionizing our view of the evolution of supermassive black holes. The survey will also provide new insights into a wide range of astrophysical phenomena, including X-ray binaries, active stars, and diffuse emission within the Galaxy. Results from early observations, some of which are presented here, confirm that the performance of the instrument is able to fulfil its scientific promise. With this paper, we aim to give a concise description of the instrument, its performance as measured on ground, its operation in space, and also the first results from in-orbit measurements