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Chicago, Burlington & Quincy (CBQ) 5127
No full textA photograph print showing Chicago, Burlington & Quincy (CBQ) 5127, 2-8-2, Class O-1-A, Keenesburg, CO
Chicago, Burlington & Quincy (CBQ) 5127
No full textA photograph postcard showing Chicago, Burlington & Quincy (CBQ) 5127, 2-8-2, on westbound freight extra [white flags on locomotive], just west of Keenesburg, CO
Block Card 5127 Burlingame Drive
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | 5127 Burlingame Drive (Toledo, Ohio) | Dwelling | Crestview Subdivision (Toledo, Ohio
Block Card 5127 Ancil Road
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: 5127 Ancil Road (Toledo, Ohio) | Dwelling | Westhaven First Addition (Toledo, Ohio) | Reynolds Corners Area (Toledo, Ohio) | Art Modern
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Going Beyond Counting First Authors in Author Co-citation Analysis
Get PDFThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
Variations on the Author
Get PDF“Variations on the Author” discusses two of Eduardo Coutinho’s recent films (Um Dia na Vida, from 2010, and Últimas Conversas, posthumously released in 2015) and their contribution to the general question of documentary authorship. The director’s filmography is characterized by a consistent yet self-effacing form of authorial self-inscription: Coutinho often features as an interviewer that rather than express opinions propels discourses; an interviewer that is good at listening. This mode of self-inscription characterizes him as an author who is not expressive but who is nonetheless markedly present on the screen. In Um Dia na Vida, however, Coutinho is completely absent form the image, while Últimas Conversas, on the contrary, includes a confessional prologue that moves the director from the margins to the center of his films. This article examines the ways in which these works stand out in the filmography of a director who offers new insights into the notion of cinematic authorship
Appropriate Similarity Measures for Author Cocitation Analysis
Get PDFWe provide a number of new insights into the methodological discussion about author cocitation analysis. We first argue that the use of the Pearson correlation for measuring the similarity between authors’ cocitation profiles is not very satisfactory. We then discuss what kind of similarity measures may be used as an alternative to the Pearson correlation. We consider three similarity measures in particular. One is the well-known cosine. The other two similarity measures have not been used before in the bibliometric literature. Finally, we show by means of an example that our findings have a high practical relevance.information science;Pearson correlation;cosine;similarity measure;author cocitation analysis
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Measurements of anisotropy in the cosmic microwave backgroundradiation at 0 degrees.5 scales near the stars HR 5127 and phiHerculis
No full textWe present measurements of cosmic microwave background (CMB) anisotropy near the stars HR 5127 and phi Herculis from the fifth flight of the Millimeter-wave Anisotropy eXperiment (MAX). We scanned 8 degrees strips of the sky with an approximately Gaussian 0.5 degrees FWHM beam and a 1.4 degrees peak to peak sinusoidal chop. The instrument has four frequency bands centered at 3.5, 6, 9, and 14 cm(-1). The IRAS 100 mu mmap predicts that these two regions have low interstellar dust contrast. The HR 5127 data are consistent with CMB anisotropy. The phi Herculis data, which were measured at lower flight altitudes, show time variability at 9 and 14 cm(-1), which we believe to be due to atmospheric emission. However, the phi Herculis data at 3.5 and 6 cm-l are essentially independent of this atmospheric contribution and are consistent with CMB anisotropy. Confusion from Galactic foregrounds is unlikely based on the spectrum and amplitude of the structure at these frequencies. If the observed HR 5127 structure and the atmosphere-independent phi Herculis structure are attributed to CMB anisotropy, then we find Delta T/T = [I(I + 1)C-1/2 pi](1/2) =1.2(-0.3)(+0.4) x 10(-5) for HR 5127 and 1.9(-0.4)(+0.7) x 10(-5) for phi Herculis in the flat band approximation. The upper and lower limits represent a 68 percent confidence interval added in quadrature with a 10 percent calibration uncertainty
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