The American Bar Association: Its Organization, History and Achievements

The American Bar Association holds its fifty-first annual meeting in Seattle, Washington, July 25, 26, 27, 1928. This is the Semi-Centennial meeting of the Association and special preparations are being made to make the occasion notable, and it is therefore appropriate that the whole bar of Washington who have so courteously invited the National Association to Seattle this year, should know something about the organization, history and achievements of the largest and one of the oldest organizations of lawyers in the world. A considerable portion of the bar of Washington are already members of the National Association, and to them many of the things hereinafter stated are well known, but it is hoped that all reputable lawyers of the great state of Washington will be sufficiently interested in the affairs of the National Association, to join its ranks, and thereby assist in the important work which the future has in store for the advancement of the profession and the welfare of the Nation

Forecasting pulsar timing array sensitivity to anisotropy in the stochastic gravitational wave background

Statistical anisotropy in the nanohertz-frequency gravitational-wave background (GWB) is expected to be detected by pulsar timing arrays (PTAs) in the near future. By developing a frequentist statistical framework that intrinsically restricts the GWB power to be positive, we establish scaling relations for multipole-dependent anisotropy decision thresholds that are a function of the noise properties, timing baselines, and cadences of the pulsars in a PTA. We verify that $(i)$ a larger number of pulsars, and $(ii)$ factors that lead to lower uncertainty on the cross-correlation measurements between pulsars, lead to a higher overall GWB signal-to-noise ratio, and lower anisotropy decision thresholds with which to reject the null hypothesis of isotropy. Using conservative simulations of realistic NANOGrav datasets, we predict that an anisotropic GWB with angular power $C_{l=1} > 0.3\,C_{l=0}$ may be sufficient to produce tension with isotropy at the $p = 3\times10^{-3}$ ($\sim3\sigma$) level in near-future NANOGrav data with a $20$~yr baseline. We present ready-to-use scaling relationships that can map these thresholds to any number of pulsars, configuration of pulsar noise properties, and sky coverage. We discuss how PTAs can improve the detection prospects for anisotropy, as well as how our methods can be adapted for more versatile searches.Comment: Submitted to ApJ. Comments welcom

America is not losing its religion – population trends mean thatit is simply becoming more religiously diverse.

A recent Pew study found that there has been an increase in the number of Americans who claim to have ‘no-religion’. Does this mean that religion in the U.S. is on the way out? In new research which examines data from three national surveys, R. Khari Brown, Robert Joseph Taylor, and Linda M. Chatters find that African Americans and African Caribbean Americans are less likely than Non-Hispanic Whites, Hispanic Americans, and Asian Americans to identify as non-religious, with the latter group the most likely to identify as non-religious. They write that the recent shifts in religious affiliation may have less to do with Americans abandoning religion to America shifting towards increasing religious diversity

Supermassive Black-hole Demographics & Environments With Pulsar Timing Arrays

Precision timing of large arrays (>50) of millisecond pulsars will detect the nanohertz gravitational-wave emission from supermassive binary black holes within the next ~3-7 years. We review the scientific opportunities of these detections, the requirements for success, and the synergies with electromagnetic instruments operating in the 2020s.Comment: Submitted to the Astro2020 Decadal Survey. One of 5 core white-papers authored by members of the NANOGrav Collaboration. 9 pages, 2 figure