Measuring the Nexus: The Relationship Between Minority Ownership and Broadcast Diversity After Metro Broadcasting

In Metro Broadcasting, Inc. v. FCC, the Court found a nexus between minority ownership and diversity of viewpoint. The recent Lutheran Church-Missouri Synod v. FCC decision dismissed the government’s arguments that a nexus exists between minority employment in broadcast stations and greater diversity in broadcast programming, and that the government has an interest in fostering such diversity. Given the challenge of the Lutheran Church opinion and potentially significant changes in the regulation and operation of the broadcast market, sole reliance on Metro Broadcasting’s holdings may be ill advised and a new study documenting the continued existence of the nexus may be warranted. Forum: New Approaches to Minority Media Ownership, Columbia Institute for Tele-Information, Columbia University

FCC Comment: In the Matter of Connect America Fund

The Broadband Institute of California (BBIC) and the Broadband Regulatory Clinic of Santa Clara Law (BRC) petition the Commission to expressly consider the needs of rural tribal lands in promulgating regulations regarding spectrum allocated for the development of 5G technologies, and encourages the Commission to work with prospective auction participants, broadband service providers and tribal communities to develop 5G use cases targeting rural and tribal needs. Presently, barriers to broadband deployment across tribal lands include geographical isolation, low population densities, difficult terrain, and political fragmentation arising from tribal governance issues. The first portion of this Comment explains these particularly crippling barriers. Enabling tribes with access to broadband connectivity can assist in combating social problems that arise as a result of these barriers. With regards to geographic isolation, access to healthcare and employment opportunities would improve, without the need for commuting long distances, as consumer markets expand

Regulating Broadband Communication Networks

Professor Allen Hammond argues that the impending development of broadband communication networks has the potential to expand and equalize speech rights by endowing the public with more numerous and more powerful opportunities for speech. To realize these benefits, however, Congress must design a novel regulatory scheme that will maximize the speech rights of both the owners and the users of broadband communication networks. Current regulatory schemes governing print, broadcast and cable provide media owners and editors with extensive speech rights, but fail to provide sufficient public access. In contrast, the regulatory scheme governing telephone service providers assures public speech rights only by depriving media owners of all opportunities for speech

Deliberative democracy and inequality: Two cheers for enclave deliberation among the disempowered

Deliberative democracy grounds its legitimacy largely in the ability of speakers to participate on equal terms. Yet theorists and practitioners have struggled with how to establish deliberative equality in the face of stark differences of power in liberal democracies. Designers of innovative civic forums for deliberation often aim to neutralize inequities among participants through proportional inclusion of disempowered speakers and discourses. In contrast, others argue that democratic equality is best achieved when disempowered groups deliberate in their own enclaves (interest groups, parties, and movements) before entering the broader public sphere. Borrowing from each perspective, the authors argue that there are strong reasons to incorporate enclave deliberation among the disempowered within civic forums. They support this claim by presenting case study evidence showing that participants in such forums can gain some of the same benefits of deliberation found in more heterogeneous groups (e.g., political knowledge, efficacy and trust), can consider a diversity of viewpoints rather than falling into groupthink and polarization, and can persuade external stakeholders of the legitimacy of the group’s deliberations

Opportunities to Learn Mathematics Pedagogy and Connect Classroom Learning to Practice: A Study of Future Teachers in the United States and Singapore

In this study, we conducted secondary analyses using the TEDS-M database to explore future mathematics specialists teachers’ opportunities to learn (OTL) how to teach mathematics. We applied latent class analysis techniques to differentiate among groups of prospective mathematics specialists with potentially different OTL mathematics pedagogy within the United States and Singapore. Within the United States, three subgroups were identified: (a) Comprehensive OTL, (b) Limited OTL, and (c) OTL Mathematics Pedagogy. Within Singapore, four subgroups were identified: (a) Comprehensive OTL, (b) Limited Opportunities to Connect Classroom Learning with Practice, (c) OTL Mathematics Pedagogy, and (d) Basic OTL. Understanding the opportunities different prospective teachers had to learn from and their experiences with different components of instructional practice in university and practicum settings has implications for teacher preparation programs

A search of the Orion spur for continuous gravitational waves using a "loosely coherent" algorithm on data from LIGO interferometers

We report results of a wideband search for periodic gravitational waves from isolated neutron stars within the Orion spur towards both the inner and outer regions of our Galaxy. As gravitational waves interact very weakly with matter, the search is unimpeded by dust and concentrations of stars. One search disk (A) is $6.87^\circ$ in diameter and centered on $20^\textrm{h}10^\textrm{m}54.71^\textrm{s}+33^\circ33'25.29"$, and the other (B) is $7.45^\circ$ in diameter and centered on $8^\textrm{h}35^\textrm{m}20.61^\textrm{s}-46^\circ49'25.151"$. We explored the frequency range of 50-1500 Hz and frequency derivative from $0$ to $-5\times 10^{-9}$ Hz/s. A multi-stage, loosely coherent search program allowed probing more deeply than before in these two regions, while increasing coherence length with every stage. Rigorous followup parameters have winnowed initial coincidence set to only 70 candidates, to be examined manually. None of those 70 candidates proved to be consistent with an isolated gravitational wave emitter, and 95% confidence level upper limits were placed on continuous-wave strain amplitudes. Near $169$ Hz we achieve our lowest 95% CL upper limit on worst-case linearly polarized strain amplitude $h_0$ of $6.3\times 10^{-25}$, while at the high end of our frequency range we achieve a worst-case upper limit of $3.4\times 10^{-24}$ for all polarizations and sky locations.Comment: Fixed minor typo - duplicate name in the author lis

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta