LMDA Newsletter, July 1, 2016

Contents include: Letter from the Editor; A Message from our LMDA President; Canadian Fellows: Vicki Stroich & Bob White in Conversation; Freelancing Across America: On the Road with Heather Helinsky; From Producing to Freelancing: Artistic Leaders Jayne Wenger & Mead Hunter; Freelancing in Canada: David Geary Talks Shop & Indigenous Dramaturgy; Early Career Projects: Anna Woodruff Collaborates with Melis Aker; Benches We Have Shared: Elizabeth Bennett & Liz Engelman Talk Life after Institutional Dramaturgy; Upcoming Events.https://soundideas.pugetsound.edu/lmdanewsletter/1008/thumbnail.jp

Paper Session II-B - The Advanced Camera for the Hubble Space Telescope

The Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) will have a high throughput, wide field, optical and I-band camera (WFC), a critically sampled high resolution camera (HRC), and a high throughput, moderate field of view far ultraviolet, solar-blind camera (SBC). The key characteristics of the ACS are listed in Table 1. The throughputs include the geometrical, scattering, and reflectivity losses from the HST optical telescope assembly (Burrows, HST OTA Handbook). Two figures are listed for the ACS efficiencies. The first is the efficiency using the quantum efficiency (QE) of the Scientific Imaging Technologies (SITe) 2K x 4K WFC CCDs and the SITe HRC 1K ´ 1K CCDs selected for the first build of the flight cameras. The second and higher efficiencies are those achieved with SITe CCDs processed and anti-reflection coated at Steward Observatory by Dr. Michael Lesser. We plan to use these better CCDs for the second build of the flight cameras

Web-based horizon scanning: Concepts and practice

PurposeIn this review, the aim is first to define horizon scanning and then outline the general approach currently employed by many organisations using web‐based resources. It then aims to discuss the benefits and drivers of horizon scanning, to identify some organisations currently undertaking activities in the field, and explain in detail how the web‐based horizon scanning approach is implemented. The aim is then to conclude with a discussion of good practice and areas for further research.Design/methodology/approachThe basis for this review is a symposium held at the UK Defence Science and Technology Laboratory in March 2010, where groups undertaking horizon scanning activities shared practices and reviewed the state of the art. Practitioners from both public sector and private organisations attending this symposium, as well as others, were invited to contribute to the manuscript, developing this as an iterative exercise over the last year.FindingsStructured processes of web‐based horizon scanning, underpinned by strong technical understanding and principles of good practice described in the review, can add significant value to organisational decision making.Originality/valueWhile a growing number of private and public sector organisations have already embarked on the use of the web as a key information resource, no detailed explanation of the web‐based horizon scanning approach has been published. The review therefore makes an original contribution to this field, with collaborations by horizon scanning practitioners, discussing what constitutes good practice and highlighting areas where future research is needed.</jats:sec

"Are you sad, Cozmo?" How humans make sense of a home robot's emotion displays

This paper explores how humans interpret displays of emotion pro- duced by a social robot in real world situated interaction. Taking a multimodal conversation analytic approach, we analyze video data of families interacting with a Cozmo robot in their homes. Focusing on one happy and one sad robot animation, we study, on a turn-by-turn basis, how participants respond to audible and visible robot behavior designed to display emotion. We show how emotion animations are consequential for interactional progres- sivity: While displays of happiness typically move the interaction forward, displays of sadness regularly lead to a reconsideration of previous actions by humans. Furthermore, in making sense of the robot animations people may move beyond the designer’s re- ported intentions, actually broadening the opportunities for their subsequent engagement. We discuss how sadness functions as an interactional "rewind button" and how the inherent vagueness of emotion displays can be deployed in design.Funding agencies:  Swedish Research CouncilSwedish Research Council [2016-00827]</p

PolStar - An Explorer-Class FUV Spectropolarimetry Mission to Map the Environments of Massive Stars

International audiencePolStar is an Explorer-class far ultraviolet (FUV) spectropolarimetry mission designed to target massive stars and their environments. PolStar will take advantage of resonance lines only available in the FUV to measure for the first time the magnetic and wind environment around massive stars to constrain models of rotation and mass loss

The Probe-class mission concept, Cosmic Evolution Through UV Surveys (CETUS)

International audienceCETUS is a 1.5-m, wide-field UV observatory that will be a worthy successor to Hubble. Its distinguishing characteristics include multi-object slit spectroscopy, long-slit spectroscopy, spectroscopy in the Lyman-UV, prompt-response observations, and detection of low-surface brightness objects. These new capabilities ensure future discoveries