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Institution

University of Arizona

EducationTucson, Arizona, United States
About: University of Arizona is a education organization based out in Tucson, Arizona, United States. It is known for research contribution in the topics: Population & Galaxy. The organization has 63805 authors who have published 155998 publications receiving 6854915 citations. The organization is also known as: UA & U of A.
Topics: Population, Galaxy, Star formation, Redshift, Planet


Papers
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Journal ArticleDOI
TL;DR: The authors have developed the Arizona Sexual Experiences Scale (ASEX), a five-item rating scale that quantifies sex drive, arousal, vaginal lubrication/penile erection, ability to reach orgasm, and satisfaction from orgasm.
Abstract: Although sexual dysfunction is common in psychiatric patients, quantification of sexual dysfunction is limited by the paucity of validated, user-friendly scales. In order to address this problem, the authors have developed the Arizona Sexual Experiences Scale (ASEX), a five-item rating scale that quantifies sex drive, arousal, vaginal lubrication/penile erection, ability to reach orgasm, and satisfaction from orgasm. Possible total scores range from 5 to 30, with the higher scores indicating more sexual dysfunction. This study assesses the internal consistency, test-retest reliability, and convergent and discriminant validity of the ASEX.

893 citations

Journal ArticleDOI
18 Feb 1998-JAMA
TL;DR: Alcohol consumption is associated with a linear increase in breast cancer incidence in women over the range of consumption reported by most women, and reducing alcohol consumption is a potential means to reduce breast cancer risk.
Abstract: Objective. - To assess the risk of invasive breast cancer associated with total and beverage-specific alcohol consumption and to evaluate whether dietary and nondietary factors modify the association. Data Sources. - We included in these analyses 6 prospective studies that had at least 200 incident breast cancer cases, assessed long-term intake of food and nutrients, and used a validated diet assessment instrument. The studies were conducted in Canada, the Netherlands, Sweden, and the United States. Alcohol intake was estimated by food frequency questionnaires in each study. The studies included a total of 322 647 women evaluated for up to 11 years, including 4335 participants with a diagnosis of incident invasive breast cancer. Data Extraction. - Pooled analysis of primary data using analyses consistent with each study's original design and the random-effects model for the overall pooled analyses. Data Synthesis. - For alcohol intakes less than 60 g/d (reported by >99% of participants), risk increased linearly with increasing intake; the pooled multivariate relative risk for an increment of 10 g/d of alcohol (about 0.75-1 drink) was 1.09 (95% confidence interval [CI], 1.04-1.13; P for heterogeneity among studies, .71). The multivariate- adjusted relative risk for total alcohol intakes of 30 to less than 60 g/d (about 2-5 drinks) vs nondrinkers was 1.41 (95% CI, 1.18-1.69). Limited data suggested that alcohol intakes of at least 60 g/d were not associated with further increased risk. The specific type of alcoholic beverage did not strongly influence risk estimates. The association between alcohol intake and breast cancer was not modified by other factors. Conclusions. - Alcohol consumption is associated with a linear increase in breast cancer incidence in women over the range of consumption reported by most women. Among women who consume alcohol regularly, reducing alcohol consumption is a potential means to reduce breast cancer risk.

892 citations

Journal ArticleDOI
TL;DR: The content of main theorems is presented in a tutorial form aimed at a broad audience of engineers and applied mathematicians interested in control, estimation and optimization of dynamic systems.

892 citations

Journal ArticleDOI
TL;DR: In this article, the authors examine the role of borrower accounting quality in debt contracting and find that poorer borrowers prefer private debt (bank loans) compared to public debt (government bonds).
Abstract: We study the role of borrower accounting quality in debt contracting. Specifically, we examine how accounting quality affects the borrower's choice of private versus public debt market and how the design of debt contracts vary with accounting quality in the two markets. We find that accounting quality affects the choice of the market, with poorer accounting quality borrowers preferring private debt (bank loans). This is consistent with banks possessing superior information access and processing abilities which reduce adverse selection costs for borrowers. We also find that accounting quality has an economically significant but differential impact on contract design in the two markets consistent with differences in recontracting flexibility across the two markets. For private debt (which has greater recontracting flexibility), both the price (interest) and non-price (maturity and collateral) terms are significantly more stringent for poorer accounting quality borrowers, unlike public debt where only the price terms are more stringent. The impact of accounting quality on interest spreads of public debt is 2.5 times that of the private debt, since the price terms alone reflect the variation in accounting quality. Overall, the results are consistent with greater recontracting flexibility of banks enabling them to write more customized contracts relative to dispersed bondholders.

890 citations

Journal ArticleDOI
TL;DR: In this article, the authors compare new maps of the hot gas, dark matter, and galaxies for 1E 0657-56, a cluster with a rare high-velocity merger occurring nearly in the plane of the sky.
Abstract: We compare new maps of the hot gas, dark matter, and galaxies for 1E 0657-56, a cluster with a rare high-velocity merger occurring nearly in the plane of the sky. The X-ray observations reveal a bullet-like gas subcluster just exiting the collision site. A prominent bow shock gives an estimate of the subcluster velocity, 4500 km s-1, which lies mostly in the plane of the sky. The optical image shows that the gas lags behind the subcluster galaxies. The weak-lensing mass map reveals a dark matter clump lying ahead of the collisional gas bullet but coincident with the effectively collisionless galaxies. From these observations, one can directly estimate the cross section of the dark matter self-interaction. That the dark matter is not fluid-like is seen directly in the X-ray-lensing mass overlay; more quantitative limits can be derived from three simple independent arguments. The most sensitive constraint, ?/m < 1 cm2 g-1, comes from the consistency of the subcluster mass-to-light ratio with the main cluster (and universal) value, which rules out a significant mass loss due to dark matter particle collisions. This limit excludes most of the 0.5-5 cm2 g-1 interval proposed to explain the flat mass profiles in galaxies. Our result is only an order-of-magnitude estimate that involves a number of simplifying, but always conservative, assumptions; stronger constraints may be derived using hydrodynamic simulations of this cluster.

889 citations


Authors

Showing all 64388 results

NameH-indexPapersCitations
Simon D. M. White189795231645
Julie E. Buring186950132967
David H. Weinberg183700171424
Richard Peto183683231434
Xiaohui Fan183878168522
Dennis S. Charney179802122408
Daniel J. Eisenstein179672151720
David Haussler172488224960
Carlos S. Frenk165799140345
Jian-Kang Zhu161550105551
Tobin J. Marks1591621111604
Todd Adams1541866143110
Jane A. Cauley15191499933
Wei Zheng1511929120209
Daniel L. Schacter14959290148
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023205
2022987
20217,005
20207,325
20196,716
20186,375