The Promise of Place-Based Investment in College Access and Success: Investigating the Impact of the Pittsburgh Promise

Author(s):  
Lindsay C. Page ◽  
Jennifer Iriti ◽  
Danielle Lowry ◽  
Aaron M. Anthony
Keyword(s):  
2018 ◽  
Vol 40 (3) ◽  
pp. 399-419 ◽  
Author(s):  
Nicholas A. Bowman ◽  
Sanga Kim ◽  
Laura Ingleby ◽  
David C. Ford ◽  
Christina Sibaouih

GEAR UP (Gaining Early Awareness and Readiness for Undergraduate Programs) is a federal program designed to promote college access and success for students from low-income backgrounds. Although some literature has examined K–12 outcomes, little research has explored the extent to which GEAR UP achieves its intended postsecondary objectives. The present study used a difference-in-differences design with a sample of 17,605 students to explore the impact of GEAR UP Iowa on college enrollment and persistence. The findings indicate that GEAR UP Iowa promotes the college enrollment of high school graduates by 3 to 4 percentage points, whereas it appears to have no effect on college persistence. Results are similar regardless of students’ socioeconomic status, race/ethnicity, sex, and K–12 special education status.


2005 ◽  
Vol 27 (4) ◽  
pp. 291-307 ◽  
Author(s):  
Sara Goldrick-Rab ◽  
Kathleen M. Shaw

The college participation rates of African Americans and Latinos continue to lag behind those of other racial and ethnic groups in the United States, despite the efforts of financial aid and affirmative action policies. Two recent federal policies that are “work-first” in nature threaten to further exacerbate racial and ethnic disparities in college access. This article examines the complex ways in which the 1996 welfare reform and the 1998 Workforce Investment Act differentially affect opportunities for college enrollment among disadvantaged adults. Utilizing national and state-level data, the authors argue that both policies restrict access to postsecondary education through the implementation of their guiding philosophy, “work-first,” which emphasizes rapid job placement as the strategy of choice in achieving stable employment and moving out of poverty. These policies have reduced the size of the clientele receiving welfare and restricted access to education and training for those who remain on the rolls. Moreover, this reduction in access is particularly acute among African Americans and Latinos. Thus, the findings indicate that these work-first federal policies serve to limit higher education opportunities available to these already disadvantaged populations.


2017 ◽  
Vol 11 (6) ◽  
pp. e12480 ◽  
Author(s):  
Amanda R. Baker ◽  
Benjamin D. Andrews ◽  
Anne McDaniel

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.


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