New York University

About: New York University is a education organization based out in New York, New York, United States. It is known for research contribution in the topics: Population & Poison control. The organization has 72380 authors who have published 165545 publications receiving 8334030 citations. The organization is also known as: NYU & University of the City of New York.

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Abstract: We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg^2 and volume of 18.7 Gpc^3, divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance and Hubble parameter H from the baryon acoustic oscillation (BAO) method, in combination with a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product D_MH from the Alcock–Paczynski (AP) effect and the growth of structure, quantified by fσ_8(z), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between D_M and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvature Ω_K = 0.0003 ± 0.0026 and a dark energy equation-of-state parameter w = −1.01 ± 0.06, in strong affirmation of the spatially flat cold dark matter (CDM) model with a cosmological constant (ΛCDM). Our RSD measurements of fσ_8, at 6 per cent precision, are similarly consistent with this model. When combined with supernova Ia data, we find H_0 = 67.3 ± 1.0 km s^−1 Mpc^−1 even for our most general dark energy model, in tension with some direct measurements. Adding extra relativistic species as a degree of freedom loosens the constraint only slightly, to H_0 = 67.8 ± 1.2 km s^−1 Mpc^−1. Assuming flat ΛCDM, we find Ω_m = 0.310 ± 0.005 and H_0 = 67.6 ± 0.5 km s^−1 Mpc^−1, and we find a 95 per cent upper limit of 0.16 eV c^−2 on the neutrino mass sum.

Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey

Abstract: We develop a new method to constrain the star formation histories, dust attenuation and stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-A break strength and the Balmer absorption-line index Hδ A . Together, these indices allow us to constrain the mean stellar ages of galaxies and the fractional stellar mass formed in bursts over the past few Gyr. A comparison with broad-band photometry then yields estimates of dust attenuation and of stellar mass. We generate a large library of Monte Carlo realizations of different star formation histories, including starbursts of varying strength and a range of metallicities. We use this library to generate median likelihood estimates of burst mass fractions, dust attenuation strengths, stellar masses and stellar mass-to-light ratios for a sample of 122 808 galaxies drawn from the Sloan Digital Sky Survey. The typical 95 per cent confidence range in our estimated stellar masses is ′40 per cent. We study how the stellar mass-to-light ratios of galaxies vary as a function of absolute magnitude, concentration index and photometric passband and how dust attenuation varies as a function of absolute magnitude and 4000-A break strength. We also calculate how the total stellar mass of the present Universe is distributed over galaxies as a function of their mass, size, concentration, colour, burst mass fraction and surface mass density. We find that most of the stellar mass in the local Universe resides in galaxies that have, to within a factor of approximately 2, stellar masses ∼5 x 10 1 0 M O ., half-light radii ∼3 kpc and half-light surface mass densities ∼10 9 M O .kpc - 2 . The distribution of D n (4000) is strongly bimodal, showing a clear division between galaxies dominated by old stellar populations and galaxies with more recent star formation.

Democracy and the Market: Political and Economic Reforms in Eastern Europe and Latin America

Abstract: The quest for freedom from hunger and repression has triggered in recent years a dramatic, worldwide reform of political and economic systems. Never have so many people enjoyed, or at least experimented with democratic institutions. However, many strategies for economic development in Eastern Europe and Latin America have failed with the result that entire economic systems on both continents are being transformed. This major book analyzes recent transitions to democracy and market-oriented economic reforms in Eastern Europe and Latin America. Drawing in a quite distinctive way on models derived from political philosophy, economics, and game theory, Professor Przeworski also considers specific data on individual countries. Among the questions raised by the book are: What should we expect from these experiments in democracy and market economy? What new economic systems will emerge? Will these transitions result in new democracies or old dictatorships?

The Adoption of Radical and Incremental Innovations: An Empirical Analysis

Abstract: This paper proposes and empirically tests whether different models are needed to predict the adoption of technical process innovations that contain a high degree of new knowledge radical innovations and a low degree of new knowledge incremental innovations. Results from a sample of 40 footwear manufacturers suggest that extensive knowledge depth measured by the number of technical specialists is important for the adoption of both innovation types. Larger firms are likely to have both more technical specialists and to adopt radical innovations. The study did not find associations between the adoption of either innovation type and decentralized decision making, managerial attitudes toward change, and exposure to external information. By implication, managers trying to encourage technical process innovation adoption need not be as concerned about modifying centralization of decision making, managerial attitudes and exposure to external information as would managers trying to encourage other types of innovation adoption, e.g., innovations in social services where these factors have been found to be important. Instead, investment in human capital in the form of technical specialists appears to be a major facilitator of technical process innovation adoption.

Management of Immune-Related Adverse Events in Patients Treated With Immune Checkpoint Inhibitor Therapy: American Society of Clinical Oncology Clinical Practice Guideline

Abstract: PurposeTo increase awareness, outline strategies, and offer guidance on the recommended management of immune-related adverse events in patients treated with immune checkpoint inhibitor (ICPi) therapyMethodsA multidisciplinary, multi-organizational panel of experts in medical oncology, dermatology, gastroenterology, rheumatology, pulmonology, endocrinology, urology, neurology, hematology, emergency medicine, nursing, trialist, and advocacy was convened to develop the clinical practice guideline Guideline development involved a systematic review of the literature and an informal consensus process The systematic review focused on guidelines, systematic reviews and meta-analyses, randomized controlled trials, and case series published from 2000 through 2017ResultsThe systematic review identified 204 eligible publications Much of the evidence consisted of systematic reviews of observational data, consensus guidelines, case series, and case reports Due to the paucity of high-quality evidence on management