Gender Differences in Cisgender Psychologists’ and Trainees’ Attitudes Toward Transgender People

Post print (author accepted) manuscript made available in accordance with publisher copyright policy. 'This article may not exactly replicate the final version published in the APA journal. It is not the copy of record.'Research that has explored the attitudes of cisgender people toward transgender people has identified gender differences, with cisgender men commonly reporting more negative attitudes than cisgender women. However, little research has explored whether such differences exist among mental health professionals. This brief report outlines findings from 3 studies focusing on attitudes toward transgender people among 3 samples of Australian cisgender psychologists or psychology trainees. The first explored attitudes toward transgender people among psychology undergraduates in an Australian university. The second 2 explored attitudes toward transgender people among Australian mental health-care professionals (with the specific focus of this brief report being upon participants in each study who were psychologists). The findings from each study suggest that cisgender men reported more negative attitudes than did cisgender women. This brief report concludes by considering the broader context that potentially shapes cisgender men’s attitudes and advocates for further research that examines the impact of gender ideology upon attitudes and awareness raising so as to improve service outcomes for transgender people

PENGARUH PENDIDIKAN DAN PELATIHAN, DISIPLIN KERJA SERTA MOTIVASI KERJA TERHADAP KINERJA PEGAWAI DI BADAN KEPEGAWAIAN DAERAH KABUPATEN KOTAWARINGIN TIMUR

Tujuan penelitian ini adalah untuk mendeskripsi dan menganalisis pengaruh pendidikan dan pelatihan, disiplin kerja, motivasi kerja baik secara parsial maupun simultan terhadap kinerja pegawai di Badan Kepegawaian Daerah Kabupaten Kotawaringin Timur. Metode penelitian yang digunakan dalam penelitian ini menggunakan metode kuantitatif dengan menggunakan sampel sebanyak 36 orang pegawai yang ada di Badan Kepegawaian Daerah Kabupaten Kotawaringin Timur. Teknik pengambilan sampel yang digunakan dalam penelitian ini menggunakan sampling jenuh, teknik pengumpulan data menggunakan kuesioner / angket dengan cara memberikan seperangkat pertanyaan kepada responden, analisis data menggunakan regresi linear berganda. Hasil uji secara parsial variabel Pendidikan dan Pelatihan (X1) diperoleh nilai signifikansi sebesar 0,771 > 0,05 dan nilai thitung 0,293 < ttabel  2,036, dengan demikian Pendidikan dan Pelatihan tidak berpengaruh signifikan terhadap kinerja pegawai, variabel Disiplin Kerja (X2) diperoleh nilai signifikansi sebesar 0,002 < 0,05 dan nilai thitung 3,457 > ttabel 2,036, dengan demikian disiplin kerja berpengaruh signifikan terhadap kinerja pegawai, variabel Motivasi Kerja (X3) diperoleh nilai signifikansi sebesar 0,122 > 0,05 dan nilai thitung 1,590  < ttabel 2,036,  dengan demikian motivasi kerja tidak berpengaruh signifikan terhadap kinerja pegawai. Hasil uji secara simultan diperoleh nilai signifikansi sebesar 0,000 < 0,05 dan nilai Fhitung 11,999 > Ftabel 2,90, dengan demikian Pendidikan dan Pelatihan, Disiplin Kerja, dan Motivasi Kerja secara simultan (bersama-sama) berpengaruh siginikan terhadap Kinerja Pegawai dengan kontribusi sebesar 52,9% sedangkan sisanya sebear 47,1% dipengaruhi oleh variabel lain di luar variabel yang tidak diteliti

Effect of Vascepa (icosapent ethyl) on progression of coronary atherosclerosis in patients with elevated triglycerides (200-499 mg/dL) on statin therapy: Rationale and design of the EVAPORATE study.

Despite reducing progression and promoting regression of coronary atherosclerosis, statin therapy does not fully address residual cardiovascular (CV) risk. High-purity eicosapentaenoic acid (EPA) added to a statin has been shown to reduce CV events and induce regression of coronary atherosclerosis in imaging studies; however, data are from Japanese populations without high triglyceride (TG) levels and baseline EPA serum levels greater than those in North American populations. Icosapent ethyl is a high-purity prescription EPA ethyl ester approved at 4 g/d as an adjunct to diet to reduce TG levels in adults with TG levels >499 mg/dL. The objective of the randomized, double-blind, placebo-controlled EVAPORATE study is to evaluate the effects of icosapent ethyl 4 g/d on atherosclerotic plaque in a North American population of statin-treated patients with coronary atherosclerosis, TG levels of 200 to 499 mg/dL, and low-density lipoprotein cholesterol levels of 40 to 115 mg/dL. The primary endpoint is change in low-attenuation plaque volume measured by multidetector computed tomography angiography. Secondary endpoints include incident plaque rates; quantitative changes in different plaque types and morphology; changes in markers of inflammation, lipids, and lipoproteins; and the relationship between these changes and plaque burden and/or plaque vulnerability. Approximately 80 patients will be followed for 9 to 18 months. The clinical implications of icosapent ethyl 4 g/d treatment added to statin therapy on CV endpoints are being evaluated in the large CV outcomes study REDUCE-IT. EVAPORATE will provide important imaging-derived data that may add relevance to the clinically derived outcomes from REDUCE-IT

The White Dwarfs within 25 Parsecs of the Sun: Kinematics and Spectroscopic Subtypes

We present the fractional distribution of spectroscopic subtypes, range and distribution of surface temperatures, and kinematical properties of the white dwarfs within 25pc of the sun. There is no convincing evidence of halo white dwarfs in the total 25 pc sample of 224 white dwarfs. There is also little to suggest the presence of genuine thick disk subcomponent members within 25 parsecs. It appears that the entire 25 pc sample likely belong to the thin disk. We also find no significant kinematic differences with respect to spectroscopic subtypes. The total DA to non-DA ratio of the 25 pc sample is 1.8, a manifestation of deepening envelope convection which transforms DA stars with sufficiently thin H surface layers into non-DAs. We compare this ratio with the results of other studies. We find that at least 11% of the white dwarfs within 25 parsecs of the sun (the DAZ and DZ stars) have photospheric metals that likely originate from accretion of circumstellar material (debris disks) around them. If this interpretation is correct, then it suggests the possibility that a similar percentage have planets, asteroid-like bodies or debris disks orbiting them. Our volume-limited sample reveals a pileup of DC white dwarfs at the well-known cutoff in DQ white dwarfs at Tef about 6000K. Mindful of small number statistics, we speculate on its possible evolutionary significance. We find that the incidence of magnetic white dwarfs in the 25 pc sample is at least 8%, in our volume-limited sample, dominated by cool white dwarfs. We derive approximate formation rates of DB and DQ degenerates and present a preliminary test of the evolutionary scenario that all cooling DB stars become DQ white dwarfs via helium convective dredge-up with the diffusion tail of carbon extending upward from their cores.Comment: Accepted for publication in The Astronomical Journa

Dwarf Novae with Newly Determined Parallaxes: Model Analyses of VY Aquari, RU Pegasi, and T Leonis

Using newly determined parallaxes for dwarf novae, we have derived outburst accretion rates for VY Aqr, RU Peg and T Leo and for T Leo during quiescence. The two short-period dwarf novae, VY Aqr and T Leo, show good agreement with optically thick steady-state accretion disks in outburst, whereas RU Peg shows a significant departure from a steady-state disk. We have determined that the white dwarf in T Leo has T$_{eff} = 16,000 \pm 1000$ K, a value consistent with long term compressional heating when gravitational wave emission drives mass transfer. The white dwarf in T Leo has a temperature in the same narrow range as other WZ Sge-like dwarf novae.Comment: The paper will apear in the October, 2004 issue of PAS

Shortest Path Computation with No Information Leakage

Shortest path computation is one of the most common queries in location-based services (LBSs). Although particularly useful, such queries raise serious privacy concerns. Exposing to a (potentially untrusted) LBS the client's position and her destination may reveal personal information, such as social habits, health condition, shopping preferences, lifestyle choices, etc. The only existing method for privacy-preserving shortest path computation follows the obfuscation paradigm; it prevents the LBS from inferring the source and destination of the query with a probability higher than a threshold. This implies, however, that the LBS still deduces some information (albeit not exact) about the client's location and her destination. In this paper we aim at strong privacy, where the adversary learns nothing about the shortest path query. We achieve this via established private information retrieval techniques, which we treat as black-box building blocks. Experiments on real, large-scale road networks assess the practicality of our schemes.Comment: VLDB201

Ultraviolet observations of LMC nova 1988

The IUE obtained ultraviolet spectra of a nova in an external galaxy. The spectral features do not seem unusual for a nova at maximum but it is hoped to be able to follow it for a long enough time to be able to study the high ionization lines that appear when the density drops to lower values (the nebular stage). A high dispersion spectrum was also obtained to assist in the line identification and to study the line of sight to the LMC 1 deg of arc away from SN 1987A

Composite Accretion Disk and White Dwarf Photosphere Analyses of the FUSE and HST Observations of EY Cygni

We explore the origin of FUSE and HST STIS far UV spectra of the dwarf nova, EY Cyg, during its quiescence using \emph{combined} high gravity photosphere and accretion disk models as well as model accretion belts. The best-fitting single temperature white dwarf model to the FUSE plus HST STIS spectrum of EY Cygni has T$_{eff} = 24,000$K, log $g = 9.0$, with an Si abundance of 0.1 x solar and C abundance of 0.2 x solar but the distance is only 301 pc. The best-fitting composite model consists of white dwarf with T$_{eff} = 22,000$K, log $g = 9$, plus an accretion belt with T$_{belt} = 36,000$K covering 27% of the white dwarf surface with V$_{belt} sin i = 2000$ km/s. The accretion belt contributes 63% of the FUV light and the cooler white dwarf latitudes contribute 37%. This fit yields a distance of 351 pc which is within 100 pc of our adopted distance of 450 pc. EY Cyg has very weak C {\sc iv} emission and very strong N {\sc v} emission, which is atypical of the majority of dwarf novae in quiescence. We also conducted a morphological study of the surroundings of EY Cyg using direct imaging in narrow nebular filters from ground-based telescopes. We report the possible detection of nebular material^M associated with EY Cygni. Possible origins of the apparently large N {\scv}/C {\sc iv} emission ratio are discussed in the context of nova explosions, contamination of the secondary star and accretion of nova abundance-enriched matter back to the white dwarf via the accretion disk or as a descendant of a precursor binary that survived thermal timescale mass transfer. The scenario involving pollution of the secondary by past novae may be supported by the possible presence of a nova remnant-like nebula around EY Cyg.Comment: To appear in AJ, Oct. 2004. 5 figures, including 2 color ones (2D pictures

The serendipituous discovery of a short-period eclipsing polar in 2XMMp

We report the serendipituous discovery of the new eclipsing polar 2XMMp J131223.4+173659. Its striking X-ray light curve attracted immediate interest when we were visually inspecting the source products of the 2XMMp catalogue. This light curve revealed its likely nature as a magnetic cataclysmic variable of AM Herculis (or polar) type with an orbital period of ~92 min, which was confirmed by follow-up optical spectroscopy and photometry. 2XMMp J131223.4+173659 probably has a one-pole accretion geometry. It joins the group of now nine objects that show no evidence of a soft component in their X-ray spectra despite being in a high accretion state, thus escaping ROSAT/EUVE detection. We discuss the likely accretion scenario, the system parameters, and the spectral energy distribution.Comment: Accepted for publication in A&