1,724,791 research outputs found
Block Card 4643 Clover Lane
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 | 4643 Clover Lane (Toledo, Ohio) | Dwelling | Greenbush Knolls Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)
Block Card 4643 Paisley 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: Dwelling | Reynolds Corners Area (Toledo, Ohio) | 4643 Paisley Road (Toledo, Ohio) | Split-Level Style | attached garage | Countryside Addition (Toledo, Ohio
Block Card 4643 Westway Street
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: Dwelling (Toledo, Ohio) | Bungalow Style | eyebrow dormer | Homeville Subdivision (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | 4643 Westway (Toledo, Ohio
Pärnu muuseum. Amandus Adamson. "Russalka" skits (nr. 4643)
No full textKlaasnegatiiv 9x12 vertikaalneTekst negatiivi ümbrikul: Pärnu muuseum. Adamson:"Russalka" skits /nr 4643/. Foto Tuulse, 1943. Tempel: Instituu
Block Card 4643 Talmadge Green 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: split-level | Dwelling | Talmadge Green Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)) | 4643 Talmadge Green Road (Toledo, Ohio
Linked collectors and determiners for: Blattaria Collection - Instituto Nacional de Pesquisas da Amazônia (INPA).
No full textNatural history specimen data linked to collectors and determiners held within, "Blattaria Collection - Instituto Nacional de Pesquisas da Amazônia (INPA)". Claims or attributions were made on Bionomia by volunteer Scribes, <a href="http://bionomia.net/dataset/c76230d9-61a0-4643-a227-bf8e2f78e7b6">https://bionomia.net/dataset/c76230d9-61a0-4643-a227-bf8e2f78e7b6</a> using specimen data from the dataset aggregated by the Global Biodiversity Information Facility, <a href="https://gbif.org/dataset/c76230d9-61a0-4643-a227-bf8e2f78e7b6">https://gbif.org/dataset/c76230d9-61a0-4643-a227-bf8e2f78e7b6</a>. Formatted as a Frictionless Data package
A Suzaku view of IGR J16393-4643
No full textOpen Access.The pulsar IGR J16393–4643 belongs to a class of highly absorbed supergiant high-mass X-ray binaries (HMXBs), characterized by a very high column density of absorbing matter. We present the results of simultaneous broad-band pulsation and spectrum analysis from a 44-ks Suzaku observation of the source. The orbital intensity profile created with the Swift Burst Alert Telescope (Swift–BAT) light curve shows an indication of IGR J16393–4643 being an eclipsing system with a short eclipse semi-angle θE ∼ 17°. For a supergiant companion star with a 20-R⊙ radius, this implies an inclination of the orbital plane in the range 39°–57°, whereas for a main-sequence B star as the companion with a 10-R⊙ radius, the inclination of the orbital plane is in the range 60°–77°. Pulse profiles created for different energy bands have complex morphology, which shows some energy dependence and increases in pulse fraction with energy. We have also investigated broad-band spectral characteristics, phase-averaged spectra and resolving the pulse phase into peak and trough phases. The phase-averaged spectrum has a very high NH(∼ 3 × 1023 cm−2) and is described by a power law (Γ ∼ 0.9) with a high-energy cut-off above 20 keV. We find a change in the spectral index in the peak and trough phases, implying an underlying change in the source spectrum
Varying discrete Laguerre-Sobolev orthogonal polynomials: Asymptotic behavior and zeros
Get PDFWe consider a varying discrete Sobolev inner product involving the Laguerre weight. Our aim is to study the asymptotic properties of the corresponding orthogonal polynomials and of their zeros. We are interested in Mehler-Heine type formulas because they describe the asymptotic differences between these Sobolev orthogonal polynomials and the classical Laguerre polynomials. Moreover, they give us an approximation of the zeros of the Sobolev polynomials in terms of the zeros of other special functions. We generalize some results appeared very recently in the literature for both the varying and non-varying cases.The author FM is partially supported by Dirección General de Investigación, Ministerio de Economía y Competitividad
Innovación of Spain, Grant MTM2012 36732 C03 01. The author JJMB is partially supported by Dirección General de Inves
tigación, Ministerio de Ciencia e Innovación of Spain and European Regional Development Found, Grant MTM2011 28952
C02 01, and Junta de Andalucía, Research Group FQM 0229 (belonging to Campus of International Excellence CEI MAR), and
projects P09 FQM 4643 and P11 FQM 7276
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
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