1,725,491 research outputs found
Booth, G H, 2743
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/372618Surname: BOOTH
Given Name(s) or Initials: G H
Military Service Number or Last Known Location: 2743
Missing, Wounded and Prisoner of War Enquiry Card Index Number: 194183536
Item: [2016.0049.04943] "Booth, G H, 2743
Ms. 2743
Get PDFManuscrito número 2743 de la Biblioteca Histórica de la USAL252 hojas : papel ; 209 x 145 mmManuscrito copiado Camillo Zanetti (Camillo Veneto). -- Aunque este copista parece haber estado en España hacia 1576, la profesora Martínez Manzano mantiene "de forma cautelar la producción de este códice entre los "manuscritos tridentinos"" (pág. 224)Manuscrito comprado por Diego de CovarrubiasProcede del Colegio de Ovied
2743. Biographie et famille de Clément IV
No full text2743. Biographie et famille de Clément IV. In: Molinier Auguste. Les Sources de l'histoire de France - Des origines aux guerres d'Italie (1494). III. Les Capétiens, 1180-1328. Paris : A. Picard et fils, 1903. p. 161
[Belgium and France 1:40,000], G.S.G.S. 2743 /
No full textVarious editions. Military map overprinted on base map showing rivers, creeks, roads, tracks, railways, canals, buildings, woods, lines, switches and brigade headquarters. Relief shown by contours and spot heights.; Panel title, index to adjoining sheets and glossary on verso of some sheets.; Maps, and index indicating National Library of Australia holdings, in an online version at: http://nla.gov.au/nla.map-vn6414425
Haverly, Jessie R. (SC 2743)
Get PDFFinding aid only for Manuscripts Small Collection 2743. Paper titled History of Level Green Christian Church which is about a church in Laurel County, Kentucky. The paper was written by Jessie R. Haverly for a Education class at Eastern Kentucky University
Block Card 2743 Monroe 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: American four and a half square | 2743 Monroe Street (Toledo, Ohio) | duplexes | Englewood Addition (Toledo, Ohio) | Auburndale Area (Toledo, Ohio
Block Card 2743 Rathbun 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: End gabled | Durtch Colonial Style | Dwelling | Parkdale Addition | Auburndale Area (Toledo, Ohio) | 2743 Rathburn Drive (Toledo, Ohio
Block Card 2743 Nebraska Avenue
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: Folk House Style | 2743 Nebraska Avenue (Toledo, Ohio) | Dwelling | Laurelwood (subdivision) (Toledo, Ohio) | Scott Park Area (Toledo, Ohio) | Gable front house
Spectroscopic confirmation of the galaxy clusters CARLA J0950+2743 at z = 2.363 and CARLA-Ser J0950+2743 at z = 2.243
Get PDFGalaxy clusters are the largest gravitationally bound structures in the Universe and therefore are a powerful tool for studying mass assembly at different epochs. At z > 2, they provide the unique opportunity to place solid constraints not only on the growth of the dark matter halo, but also on the mechanisms of galaxy quenching and morphological transformation when the Universe was younger than 3.3 Gyr. However, the currently available sample of confirmed z > 2 clusters remains very limited. We present the spectroscopic confirmation of the galaxy cluster CARLA J0950+2743 at z = 2.363 ± 0.005 and a new serendipitously discovered cluster, CARLA-Ser J0950+2743 at z = 2.243 ± 0.008, in the same region. We confirm eight star-forming galaxies in the first and five in the second cluster by detecting [OII], [OIII], and Hα emission lines. The analysis of an archival X-ray Chandra dataset that covers the cluster position revealed a counterpart with a total luminosity of L0.5−5keV = 2.9 ± 0.6 × 1045 erg s−1. Because the depth of the X-ray observations is limited, we cannot distinguish the 1D profile of the source from a point spread function model, but our statistical analysis of the 2D profile favors an extended component that might be associated with a thermal contribution from the intracluster medium. If the extended X-ray emission is due to the hot intracluster medium, the total combined dark matter mass for the two clusters would be M200 ≈ 3.0−0.23(stat)+0.20 −0.85(sys)+1.13 × 1014 M⊙, assuming a ∼30% contribution from the active galactic nucleus. Our two clusters are therefore interesting targets for studies of the structure growth in the cosmological context. However, future investigation will require deeper high-resolution X-ray and spectroscopic observations to rule out the hypotheses that the emission is entirely due to the active galactic nucleus or that it originates from other contaminating radio galaxies and structures
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