Standardization work for the calibration of intensities of celestial objects

Observations of celestial phenomena need to be calibrated, to be related, to some measurable quantity. There continues to be a long-term need for accurate photometric standard stars, those with known intensities and colors, so that brightness and color measurements made of various celestial phenomena by different observers can be integrated and compared with one another. Toward this end, the author has been emphasizing data collection in recent years for stars of 'intermediate' brightness, those approximately in the magnitude range 11.5 is less than V is less than 16.0. Photoelectric data were obtained at the Cerro Tololo InterAmerican Observatory's (CTIO) telescopes for stars in certain selected areas near the celestial equator. Stars of extreme color outside the selected areas, but near the equator, also were selected to provide a more broad and complete range in color index. It was proposed to complete the photoelectric phase of the program. The author proposed developing extremely faint sequences of photometric standard stars useful for both large space-based detectors and for land-based detectors. These data were to be collected via charge-coupled devices (CCD's) at telescopes located at CTIO and at the Las Campanas Observatory (LCO), both observatories being located in Chile. It was hoped that accurate data could be collected down to the 21st or 22nd magnitude

Evaluation of the Program Delivery of Every Women\u27s Life in Virginia

Introduction: Among women, breast cancer is the most prevalent cancer and the second leading cause of cancer death. Although technology advances have improved survival rates for breast cancer overall, improvements have not been universally experienced by all socioeconomic and racial groups. Known determinants of breast cancer care disparities include socioeconomic status, race, age, and social support. As a part of the Breast and Cervical Cancer Mortality Prevention Act of 1990 and with the help of CDC funding, the Virginia Breast and Cervical Cancer Early Detection Program (BCCEDP) or Every Woman’s Life (EWL) was created. EWL provides breast cancer screening to female VA residents between the ages of 18 and 64 who lack health insurance and fall at or below 200% of the Federal Poverty Level. Objective: The purpose of this study is to determine if delays in the diagnosis and treatment of breast cancer, within the VDH program EWL, differs based on sociodemographic characteristics and/ or regional location. Methods: From its inception to July 2008, 705 women received a breast cancer diagnosis through the EWL program. For these 705 cases prevalence and crude odds ratios were calculated for both diagnosis and treatment delays for all of the demographic variables along with 95% confidence intervals. Adjusted odds ratios were calculated for sociodemographic variables against screening to diagnosis delays and diagnosis to treatment disparities along with 95% confidence intervals. Results: According to the crude odds ratios more women who fall into the other category of race experienced diagnosis delays (OR=2.28 [1.11, 4.67]), but they were more likely to receive treatment in a timely manner (OR=0.29 [0.11, 0.79]). Women living alone were also more likely to experience diagnosis delays (OR=1.49 [1.10, 3.02]). Hispanic women were more likely to receive treatment in a more timely manner than non-Hispanic women (OR=0.21 [0.05, 0.81]). Also, women being treated in any other region than northern VA were more likely to experience treatment delays. However, according to the adjusted odds ratios, the only significant timing delay was the one experienced more often by women in the other race category. Conclusion: The research indicates known indicators of disparities within cancer care as socioeconomic status, race, ethnicity, age, and social support. The findings of this study indicate that the only significant indicator of disparity within the Every Women’s Life program is race. Although, African-American women were just as likely to receive timely diagnosis and treatment as white women in the program, it was the combined groups of Asian, American Indian, and other women that were more likely to experience diagnosis, but not treatment, delays. The fact that no other significant indicators of disparities were found within EWL indicates a success of the program, as EWL is targeting those women that would have otherwise been missed by the system

Is KR Cygni a Triple Star System?

New multi-color UBVR light curves of the eclipsing binary KR Cyg were obtained in 2005. Photometric solutions were derived using the Wilson- Devinney method. The result shows that KR Cyg is a near-contact binary system with a large effective temperature difference between the components, approximately 5230 K. All the times of minimum light were collected and combined with our observations obtained in 2010 and 2011. Analysing all the times of mid-eclipse, we found for the first time a possible periodic oscillation with an amplitude of 0.001 days and a period of ~76 years. The periodic oscillation could be explained by the light-time effect due to a presumed third component.Comment: 19 pages, 6 figure

The Stink Bugs (Hemiptera: Heteroptera: Pentatomidae) of Washington State

Froeschner (1988) recorded 23 species of stink bugs (Hemiptera: Heteroptera: Pentatomidae) from Washington State. Based on material primarily housed in the M. T. James Entomological Collection at Washington State University, the number of species is increased to 51. Three species recorded by Froeschner (1988) were not found in our collections: Apateticus crocatus (Uhler), Chlorochroa rossiana Buxton and Thomas, and Tepa rugulosa (Say). Species recorded from Washington State for the first time are: Apoecilus bracteatus (Fitch), Perillus bioculatus (Fabricius), Podisus maculiventris (Say), P. pallens (Stål), P. placidus Uhler, P. serieventris Uhler, Zicrona caerulea (Linnaeus), Halyomorpha halys (Stål), Brochymena quadripustulata (Fabricius), B. sulcata Van Duzee, Acrosternum hilare (Say), Aelia americana Dallas, Banasa euchlora Stål, B. tumidifrons Thomas and Yonke, Chlorochroa congrua Uhler, Coenus delius (Say), Cosmopepla uhleri Montandon, Dendrocoris pini Montandon, Euschistus servus (Say), E. tristigmus (Say), E. variolarius (Palisot), Holcostethus limbolarius (Say), Neottiglossa sulcifrons Stål, N. undata (Say), Prionosoma podopioides (Uhler), Tepa yerma (Rolston), Trichopepla grossa (Van Duzee), and Amaurochrous vanduzeei Barber and Sailer

Unordentliche Jugendliche an ordentlichen Orten? Raumkonstruktion im Spannungsfeld städtischer Politik, Raumaneignungen Jugendlicher und Bedürfnissen Anwohnende

This paper focuses on processes of attribution by others to young people as well as processes of self-attribution by the latter. It first examines the attribution by others by looking at Zurich’s youth-policy and its underlying conception of public space. In a second step, it zooms in on an urban square where a conflict of interests has to be solved within the framework of the civic policy, i.e. as a process of negotiation. It thereby examines the relation between the attribution by others to young people and the meaning attributed to the square. The analysis reveals considerable differences regarding the perception of conflicts about the use of the square, the meaning attributed to it, the attributions to young people, as well as differences between scales (city vs. square). It is argued that a concept of a relational space helps to grasp the complexity of conflicts about the use of space, since it allows examining different perspectives simultaneously

Tuning of the Rashba effect in Pb quantum well states via a variable Schottky barrier

Spin-orbit interaction (SOI) in low-dimensional systems results in the fascinating property of spin-momentum locking. In a Rashba system the inversion symmetry normal to the plane of a two-dimensional (2D) electron gas is broken, generating a Fermi surface spin texture reminiscent of spin vortices of different radii. This can be exploited in a spin-based field-effect transistor (spin- FET), where the Rashba system forms a 2D channel between ferromagnetic (FM) source and drain electrodes. The electron spin precesses when propagating through the Rashba channel and spin orientations (anti)parallel to the drain give (low) high conductivity. Crucial is the possibility to tune the momentum splitting, and consequently the precession angle, through an external parameter. Here we show that this can be achieved in Pb quantum well states through the doping dependence of the Schottky barrier, opening up the possibility of a terahertz spin-FET.Comment: 8 pages, 7 figure

The CALSPEC Stars P177D and P330E

Multicolor photometric data are presented for the CALSPEC stars P177D and P330E. Together with previously published photometry for nine other CALSPEC standards, the photometric observations and synthetic photometry from HST/STIS spectrophotometry agree in the B, V, R, and I bands to better than $\sim$1\% (10 mmag).Comment: 15 pages, 6 figure

Trap Response of Michigan Social Wasps (Hymenoptera: Vespidae) to the Feeding Attractants Acetic Acid, Isobutanol, and Heptyl Butyrate.

Nine species of social wasps were captured in traps baited with acetic acid, isobutanol, heptyl butyrate and combinations of acetic acid and either isobutanol or heptyl butyrate. Three yellowjacket species in the Vespula rufa species group were captured in traps (Vespula acadica (Sladen), Vespula consobrina (Saussure), Vespula vidua (Saussure)). They responded similarly, with attraction only to heptyl butyrate. Three yellowjacket species in the Vespula vulgaris species group were also captured in traps (Vespula vulgaris (L.), Vespula flavorpilosa Jacobson, Vespula maculifrons (Buyyson)). They responded similarly, with attraction primarily to the combination of acetic acid and isobutanol. The bald-faced hornet, Dolichovespula maculata (L.), was attracted to acetic acid and was more strongly attracted to the combination of acetic acid and isobutanol. The aerial yellowjacket, Dolichovespula arenaria (Fabr.), was attracted to isobutanol, and was more strongly attracted to the combination of acetic acid and isobutanol. These results add to our understanding of how to target various species of social wasps with chemical lures