Archives from Houses of Cistercian Nuns and Their Evidence for Powerful Thirteenth-Century Secular Women

This essay examines documents from abbeys of Cistercian nuns in northern France. The documents reveal the presence of numerous women of power and authority as founders and patrons of those women\u27s houses. Where some women were acting as widows or regents, others had access to sufficient funds for acts of patronage and foundation because they were heiresses. Here those named Matilda from the ecclesiastical province of Sens in northern France are underlined, showing the diversity of female wealth and power

Women and Monasticism in Medieval Europe: Sisters and Patrons of the Cistercian Reform

A selection of documents, translated primarily from medieval Latin but occasionally from Old French, that shows how religious women and their patrons managed resources to make monastic communities - particularly a variety of Cistercian communities - work. The records help us reconstruct how nuns and abbesses of Cistercian communities in the thirteenth century organized and kept records, managed their properties, responded to attempts at usurpation, and balanced their lives between devotional practices, which were part of their cloistered world, and family and social responsibilities beyond the convent walls.https://scholarworks.wmich.edu/mip_teamsdp/1003/thumbnail.jp

The Seventh Data Release of the Sloan Digital Sky Survey

This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDSS-II. It includes 11663 deg^2 of imaging data, with most of the roughly 2000 deg^2 increment over the previous data release lying in regions of low Galactic latitude. The catalog contains five-band photometry for 357 million distinct objects. The survey also includes repeat photometry over 250 deg^2 along the Celestial Equator in the Southern Galactic Cap. A coaddition of these data goes roughly two magnitudes fainter than the main survey. The spectroscopy is now complete over a contiguous area of 7500 deg^2 in the Northern Galactic Cap, closing the gap that was present in previous data releases. There are over 1.6 million spectra in total, including 930,000 galaxies, 120,000 quasars, and 460,000 stars. The data release includes improved stellar photometry at low Galactic latitude. The astrometry has all been recalibrated with the second version of the USNO CCD Astrograph Catalog (UCAC-2), reducing the rms statistical errors at the bright end to 45 milli-arcseconds per coordinate. A systematic error in bright galaxy photometr is less severe than previously reported for the majority of galaxies. Finally, we describe a series of improvements to the spectroscopic reductions, including better flat-fielding and improved wavelength calibration at the blue end, better processing of objects with extremely strong narrow emission lines, and an improved determination of stellar metallicities. (Abridged)Comment: 20 pages, 10 embedded figures. Accepted to ApJS after minor correction