Technology Changes Everything: Inclusive Tech and Jobs for a Diverse Workforce: Pierce Memorial Foundation Report

This document serves as the final report to the Pierce Foundation for funding to support the design and implementation of a 1.5-day Forum entitled “Technology Changes Everything: A Forum on Inclusive Tech and Jobs for a Diverse Workforce” conducted in NYC on October 26-27, 2017 at Baruch College. The conference idea was conceived to address the need to raise awareness across a number of distinct areas where technology is currently impacting employment outcomes for people with disabilities. The topics ranged from one as straightforward as the critical need for attention on equitably integrating individuals with disabilities into the rapidly exploding tech sector workforce, to the much more nuanced and complex application of algorithmic screening and job-matching tools increasingly used in online job applications and selection processes. Other topics focused on were equitable access to entrepreneurship opportunities, inclusive design in technology-based products and services, and the growing targeted focus of technology sector and tech-intensive industries in affirmative recruitment and hiring of individuals with Autism

Local Government Policy and Planning for Unmanned Aerial Systems

This research identifies key state and local government stakeholders in California for drone policy creation and implementation, and describes their perceptions and understanding of drone policy. The investigation assessed stakeholders’ positions, interests, and influence on issues, with the goal of providing potential policy input to achieve successful drone integration in urban environments and within the national airspace of the United States. The research examined regulatory priorities through the use of a two-tiered Stakeholder Analysis Process. The first tier consisted of a detailed survey sent out to over 450 local agencies and jurisdictions in California. The second tier consisted of an in-person focus group to discuss survey results as well as to gain deeper insights into local policymakers’ current concerns. Results from the two tiers of analysis, as well as recommendations, are provided here

TESS unveils the phase curve of WASP-33b. Characterization of the planetary atmosphere and the pulsations from the star

We present the detection and characterization of the full-orbit phase curve and secondary eclipse of the ultra-hot Jupiter WASP-33b at optical wavelengths, along with the pulsation spectrum of the host star. We analyzed data collected by the Transiting Exoplanet Survey Satellite (TESS) in sector 18. WASP-33b belongs to a very short list of highly irradiated exoplanets that were discovered from the ground and were later visited by TESS. The host star of WASP-33b is of delta Scuti-type and shows nonradial pulsations in the millimagnitude regime, with periods comparable to the period of the primary transit. These completely deform the photometric light curve, which hinders our interpretations. By carrying out a detailed determination of the pulsation spectrum of the host star, we find 29 pulsation frequencies with a signal-to-noise ratio higher than 4. After cleaning the light curve from the stellar pulsations, we confidently report a secondary eclipse depth of 305.8 +/- 35.5 parts-per-million (ppm), along with an amplitude of the phase curve of 100.4 +/- 13.1 ppm and a corresponding westward offset between the region of maximum brightness and the substellar point of 28.7 +/- 7.1 degrees, making WASP-33b one of the few planets with such an offset found so far. Our derived Bond albedo, A_B = 0.369 +/- 0.050, and heat recirculation efficiency, epsilon = 0.189 +/- 0.014, confirm again that he behavior of WASP-33b is similar to that of other hot Jupiters, despite the high irradiation received from its host star. By connecting the amplitude of the phase curve to the primary transit and depths of the secondary eclipse, we determine that the day- and nightside brightness temperatures of WASP-33b are 3014 +/- 60 K and 1605 +/- 45 K, respectively. From the detection of photometric variations due to gravitational interactions, we estimate a planet mass of M_P = 2.81 +/- 0.53 M$_J.Comment: 19 pages, 15 figure