The Impact of Pretrial Release Programming on Rearrest: Results from an Eastern Pennsylvania County Sample

Corrections ◽  
2021 ◽  
pp. 1-15
Author(s):  
Michelle A. Bolger ◽  
Michael J. Phillips
2019 ◽  
Vol 31 (6) ◽  
pp. 833-856
Author(s):  
Alissa Pollitz Worden ◽  
Reveka V. Shteynberg ◽  
Kirstin A. Morgan ◽  
Andrew L. B. Davies

This article examines the impact of early provision of counsel on judges’ pretrial release and bail decisions in two rural counties in upstate New York, in cases involving felony charges. This study builds upon previously reported research on misdemeanor cases. We note that although the stakes are higher in felony cases, few studies have investigated the dynamics of first appearance decisions at either level. We investigate the hypotheses that when defendants are represented by attorneys at their first appearances in court, (a) judges are more inclined to release on recognizance or under supervision, (b) judges impose less restrictive bail amounts, and (c) as a consequence, defendants spend less time detained prior to disposition. We find mixed support for these hypotheses, although some evidence that counsel at first appearance (CAFA) produces the expected outcomes. We conclude that the implementation of programs intended to ensure CAFA may be tempered by courthouse cultures, and that future research on court reform should include the study of rural jurisdictions.


2004 ◽  
Vol 51 (2) ◽  
pp. 222-242 ◽  
Author(s):  
STEPHEN DEMUTH ◽  
DARRELL STEFFENSMEIER

2018 ◽  
Vol 29 (6-7) ◽  
pp. 710-735 ◽  
Author(s):  
Alissa Pollitz Worden ◽  
Kirstin A. Morgan ◽  
Reveka V. Shteynberg ◽  
Andrew L. B. Davies

Recent court decisions and state legislation have highlighted the significance of ensuring that criminal defendants are represented by counsel at their first appearances in court, where judges make critical decisions on pretrial release, bail, and detention. Yet many jurisdictions do not routinely provide counsel to indigent defendants at this stage. We hypothesize that when defendants are represented by counsel at first appearance (CAFA), they are more likely to be released on recognizance, are less likely to have high bail set, and are consequently less likely to be jailed pending disposition. We explore the impact of lawyers’ presence by comparing pretrial decisions and bail outcomes across samples of misdemeanor cases in three rural counties in upstate New York: cases with and without CAFA. We find that these counties saw shifts in decisions or outcomes. We consider the implications of these findings for future research, court practices, and public policy.


Author(s):  
Mary Foltz ◽  
Adrian Shanker ◽  
Liz Bradbury ◽  
Kristen Leipert

With the emergence of COVID-19 in the U.S., many LGBTQ people found ourselves reflecting upon the early years of HIV/AIDS and how our communities responded to the lack of robust federal and state response to this preceding public health crisis. As the leaders of the Bradbury-Sullivan LGBT Community Center (BSC) in eastern Pennsylvania became a central resource for our community sharing up-to-date information about COVID-19 and organizing vaccine clinics, they also recognized the historic nature of this moment as many elders in our community consistently tried to make sense of the current crisis by contemplating their past AIDS activism and organizing. In March of 2020, BSC staff and archivists received grant funding to conduct an oral history project called "40 Years of Public Health in the LGBTQ Community: Collecting and Curating Local LGBTQ Health Experiences From HIV/AIDS to COVID-19," which recorded both timely commentary on the impact of COVID-19 on LGBTQ people and memories of HIV/AIDS organizing that seemed urgent and relevant to our contemporary moment. Offering excerpts from oral histories collected in 2020, this piece explores how COVID-19 spurred LGBTQ people in the Lehigh Valley to share stories about communal grief, health inequity, political responses to pandemics, and organizing to support the health of minoritized communities.


1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.


1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.


1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.


1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.


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