At Risk: The Bay Area Greenbelt

In 2006, Greenbelt Alliance, the Bay Area's land conservation and urban planning organization, published the newest edition of its landmark study on the state of the region's landscapes. The report found that if current development patterns continue, roughly one out of every 10 acres in the entire Bay Area could be paved over in the next thirty years. Today, there are 401,500 acres of greenbelt lands at risk of sprawl development. That includes 125,200 acres at risk within the next 10 years, classified as high-risk land, and 276,200 acres at risk within the next 10 to 30 years, classified as medium-risk land. Around the region, the places at highest risk -- the sprawl hot spots -- include the I-80 corridor in Solano County, the eastern cities in Contra Costa County, Coyote Valley in southern Santa Clara County, the Tri-Valley area of Alameda and Contra Costa Counties, and areas along Highway 101 through Sonoma County

Divine Art / Infernal Machine: Western Views of Printing Surveyed

The University of Pennsylvania Libraries A.S.W. Rosenbach Lectures in Bibliography for 2010: Monday, March 22, 2010: First Impressions Welcome: David McKnight (00:01-06:00); Introduction: Peter Stallybrass (06:00-13:02); Lecture: Elizabeth L. Eisenstein (13:02-59:57); Question and Answer: (59:57-01:12:33)Tuesday, March 23, 2010: Eighteenth-Century Attitudes Introduction: David McKnight, Libby Kislak (00:01-07:02); Lecture: Elizabeth L. Eisenstein (07:02-52:57); Question and Answer: (52:57-01:07:31)Thursday, March 25, 2010: From Steam Press to Cyberspace Welcome: David McKnight (00:01-04:32); Introduction: Roger Chartier (04:32-11:33); Lecture: Elizabeth L. Eisenstein (11:33-59:05); Question and Answer: (59:20-01:09:22) The 2010 Rosenbach Fellow, Elizabeth L. Eisenstein, is a graduate of Vassar College and Harvard University and is Professor Emerita of History at the University of Michigan. Her classic work The Printing Press as an Agent of Change: Communications and Cultural Transformations in Early Modern Europe (1979) is available in many formats and languages, and her other works include Grub Street Abroad: Aspects of the French Cosmopolitan Press from the Age of Louis XIV to the French Revolution (1992). Professor Eisenstein received the Scholarly Distinction award from the American Historical Association in 2002. An expanded version of these lectures has been published as Divine Art, Infernal Machine: The Reception of Printing in the West from First Impressions to the Sense of an Ending (University of Pennsylvania Press, 2011).To download a podcast of each lecture, choose one of the additional files below. To view the event announcement, select the Download button at upper right

Quantitative Molecular Endoscope for Real-­‐Time Optical Imaging of Colorectal Cancer

http://deepblue.lib.umich.edu/bitstream/2027.42/96180/1/me450f12project3_report.pd

Dialect-robust Evaluation of Generated Text

Evaluation metrics that are not robust to dialect variation make it impossible to tell how well systems perform for many groups of users, and can even penalize systems for producing text in lower-resource dialects. However, currently, there exists no way to quantify how metrics respond to change in the dialect of a generated utterance. We thus formalize dialect robustness and dialect awareness as goals for NLG evaluation metrics. We introduce a suite of methods and corresponding statistical tests one can use to assess metrics in light of the two goals. Applying the suite to current state-of-the-art metrics, we demonstrate that they are not dialect-robust and that semantic perturbations frequently lead to smaller decreases in a metric than the introduction of dialect features. As a first step to overcome this limitation, we propose a training schema, NANO, which introduces regional and language information to the pretraining process of a metric. We demonstrate that NANO provides a size-efficient way for models to improve the dialect robustness while simultaneously improving their performance on the standard metric benchmark

The Sloan Bright Arcs Survey : Six Strongly Lensed Galaxies at z=0.4-1.4

We present new results of our program to systematically search for strongly lensed galaxies in the Sloan Digital Sky Survey (SDSS) imaging data. In this study six strong lens systems are presented which we have confirmed with follow-up spectroscopy and imaging using the 3.5m telescope at the Apache Point Observatory. Preliminary mass models indicate that the lenses are group-scale systems with velocity dispersions ranging from 466-878 km s^{-1} at z=0.17-0.45 which are strongly lensing source galaxies at z=0.4-1.4. Galaxy groups are a relatively new mass scale just beginning to be probed with strong lensing. Our sample of lenses roughly doubles the confirmed number of group-scale lenses in the SDSS and complements ongoing strong lens searches in other imaging surveys such as the CFHTLS (Cabanac et al 2007). As our arcs were discovered in the SDSS imaging data they are all bright ($r\lesssim22$), making them ideally suited for detailed follow-up studies.Comment: 13 pages, 3 figures, submitted to ApJL, the Sloan Bright Arcs page is located here: http://home.fnal.gov/~kubo/brightarcs.htm

The Sloan Bright Arcs Survey: Four Strongly Lensed Galaxies with Redshift >2

We report the discovery of four very bright, strongly-lensed galaxies found via systematic searches for arcs in Sloan Digital Sky Survey Data Release 5 and 6. These were followed-up with spectroscopy and imaging data from the Astrophysical Research Consortium 3.5m telescope at Apache Point Observatory and found to have redshift $z>2.0$. With isophotal magnitudes $r = 19.2 - 20.4$ and 3\arcsec-diameter magnitudes $r = 20.0 - 20.6$, these systems are some of the brightest and highest surface brightness lensed galaxies known in this redshift range. In addition to the magnitudes and redshifts, we present estimates of the Einstein radii, which range from 5.0 \arcsec to 12.7 \arcsec, and use those to derive the enclosed masses of the lensing galaxies

Observations and properties of candidate high frequency GPS radio sources in the AT20G survey

We used the Australia Telescope Compact Array (ATCA) to obtain 40 GHz and 95 GHz observations of a number of sources that were selected from the Australia Telescope Compact Array 20 GHz (AT20G) survey . The aim of the observations was to improve the spectral coverage for sources with spectral peaks near 20 GHz or inverted (rising) radio spectra between 8.6 GHz and 20 GHz. We present the radio observations of a sample of 21 such sources along with optical spectra taken from the ANU Siding Spring Observatory 2.3m telescope and the ESO-New Technology Telescope (NTT). We find that as a group the sources show the same level of variability as typical GPS sources, and that of the 21 candidate GPS sources roughly 60% appear to be genuinely young radio galaxies. Three of the 21 sources studied show evidence of being restarted radio galaxies. If these numbers are indicative of the larger population of AT20G radio sources then as many as 400 genuine GPS sources could be contained within the AT20G with up to 25% of them being restarted radio galaxies.Comment: 21 pages, 24 figures, Table 1 truncated at 11 column

The NICMOS Ultra Deep Field: Observations, Data Reduction, and Galaxy Photometry

This paper describes the observations and data reduction techniques for the version 2.0 images and catalog of the NICMOS Ultra Deep Field Treasury program. All sources discussed in this paper are based on detections in the combined NICMOS F110W and F160W bands only. The NICMOS images are drizzled to 0.09 arc second pixels and aligned to the ACS UDF F850LP image which was rebinned to the same pixel scale. These form the NICMOS version 2.0 UDF images. The catalog sources are chosen with a conservative detection limit to avoid the inclusion of numerous spurious sources. The catalog contains 1293 objects in the 144 x 144 arc sececonds NICMOS subfield of the UDF. The 5 sigma signal to noise level is an average 0.6 arc second diameter aperture AB magnitude of ~27.7 at 1.1 and 1.6 microns. The catalog sources, listed in order of right ascension, satisfy a minimum signal to noise criterion of 1.4 sigma in at least 7 contiguous pixels of the combined F110W and F160W imageComment: Accepted for publication in the Astronomical Journal. 33 Pages, 6 Figure

Inflation and Dark Energy from spectroscopy at z > 2

The expansion of the Universe is understood to have accelerated during two epochs: in its very first moments during a period of Inflation and much more recently, at z < 1, when Dark Energy is hypothesized to drive cosmic acceleration. The undiscovered mechanisms behind these two epochs represent some of the most important open problems in fundamental physics. The large cosmological volume at 2 < z < 5, together with the ability to efficiently target high-$z$ galaxies with known techniques, enables large gains in the study of Inflation and Dark Energy. A future spectroscopic survey can test the Gaussianity of the initial conditions up to a factor of ~50 better than our current bounds, crossing the crucial theoretical threshold of $\sigma(f_{NL}^{\rm local})$ of order unity that separates single field and multi-field models. Simultaneously, it can measure the fraction of Dark Energy at the percent level up to $z = 5$, thus serving as an unprecedented test of the standard model and opening up a tremendous discovery space