3,531 research outputs found

    Mr. Melvin J. Collier, RWWL AUC, June 2011

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    This video is a conversation with Mr. Melvin J. Collier. Mr. Collier talks about his book, "From Mississippi to Africa: A Journey of Discovery". Daniel Le, AUC Woodruff Library, is the interviewer

    Letter from Bishop Patrick Collier to Hagan

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    Holograph letter from Bishop Patrick Collier, Sion House, Kilkenny, to (Hagan). Enclosing Peter's Pence and an accompanying letter in presentation; also enclosing notes in terna for the replacement of the dean, naming Archdeacon Tobias Walsh, Canon James Doyle, Canon James Dunphy; the replacement of the parish priest of St. Canice's, naming Canon John Doody, Fr. Martin Kealy, and Fr. Charles Cavanagh; likewise for a parish priest of Slieverne, naming Fr. Edward Brennan, Fr. John Clohessy, Fr. John Bergin; recommending the first-named in each case. (With notes by Curran.

    Sarah Mildred Collier Cagle Genealogical Collection - Accession 665

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    The Sarah Mildred Collier Cagle Genealogical Collection consists of photocopied genealogical documents of the following families John Collier; Fancher; Wilkie/Wilkey collected by Sarah Mildred Collier Cagle (b. 1915). Most of the collection consists of photocopies of genealogical books. Also included are photocopies of miscellaneous genealogical material related to the Wilkie family and allied families including muster rolls, letters, notes, short histories, and pension applications. Some of the prominent family surnames included are: Barefield/Barfield; Barham; Blankenship; Bowen; Brooke; Brown; Bryan; Carter; Chandler; Christiansen; Clark; Collier; Davidson; Davis; Denton; Franklin; Frith; Funston; Giannini; Greene; Harris; Henderson; Holeman; Jackson; Jenkins; Jones; Johnson; Lewis; Martin; McGreger; McNeely; Miller; Moore; Peterson; Randle; Richardson; Roberts; Smith; Terry; Thomas; Thompson; Tinsley; Tirey; Walker; Watts; White; Wilkie/Wilkey; Williams; Wilson;https://digitalcommons.winthrop.edu/manuscriptcollection_findingaids/1570/thumbnail.jp

    ICARUS building 185 and 156 - Visit with Charlotte Warakaulle, Martin Steinacher, Paul Collier, Miguel Jimenez and Roberto Losito.

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    ICARUS building 185 and 156 - Visit with Charlotte Warakaulle, Martin Steinacher, Paul Collier, Miguel Jimenez and Roberto Losito

    A vindication of the Reasons and Defence, &c. Part 1. [electronic resource] : Being a reply to the first part of No sufficient reason for restoring some prayers and directions of King Edward Vi's first Liturgy. By the author of the Reasons and Defence.

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    The author of the Reasons = Jeremy Collier.Also issued as part of: 'A collection of tracts written by the late Reverend .. Jeremy Collier, ..', London, 1736.With a half-title.Electronic reproduction.English Short Title Catalog,Reproduction of original from British Library

    "Economic Aid to Post-conflict Countries: A Methodological Critique of Collier and Hoeffler"

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    This paper retests the analysis of "Aid Policy and Growth in Post-Conflict Societies," by Paul Collier and Anke Hoeffler (October 2002 and forthcoming in European Economic Review). It finds that their data and analysis do not support their conclusions and policy recommendations on the optimal timing and amounts of aid. These conclusions depend on very few observations (13 for the period of peace-onset, 13 for years 4 to 7 when a growth spurt is said to make aid particularly effective, and 8 for the period when aid should taper off); are vulnerable to the same methodological misspecifications identified in the Burnside and Dollar approach on which this analysis is based; and are not grounded in any theoretical formulation about the special relation between aid and growth in post-conflict conditions. Conventional econometric procedures are often not followed; recoding the sample to exclude cases that are not civil wars reduces the effect of aid on growth in post-civil war countries to less than half of what they claim; and the difference with the relationship for "normal" countries becomes negligible (0.26 percentage points), although it depends on identification of the sample. Their claims on the poverty-efficiency of aid are assumed, not analysed. The confidentiality of their policy measure (CPIA) prevented testing the aid-policy relationship.Economic aid Post-conflict Methodology

    Supplemental Material, sj-pdf-2-ptd-10.1177_08968608211035952 - A pilot project evaluating a fixed drainage system (U-Drain) for automated peritoneal dialysis

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    Supplemental Material, sj-pdf-2-ptd-10.1177_08968608211035952 for A pilot project evaluating a fixed drainage system (U-Drain) for automated peritoneal dialysis by Dimitrios Poulikakos, Joanne Martin, Joanne Collier and David Lewis in Peritoneal Dialysis International</p

    Supplemental Material, sj-pdf-1-ptd-10.1177_08968608211035952 - A pilot project evaluating a fixed drainage system (U-Drain) for automated peritoneal dialysis

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    Supplemental Material, sj-pdf-1-ptd-10.1177_08968608211035952 for A pilot project evaluating a fixed drainage system (U-Drain) for automated peritoneal dialysis by Dimitrios Poulikakos, Joanne Martin, Joanne Collier and David Lewis in Peritoneal Dialysis International</p

    Distribution and evolution of starspots on the RS CVn binary II Pegasi in 2004

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    This work is supported by National Natural Science Foundation of China through grants Nos. 10373023, 10773027 and 11333006, Chinese Academy of Sciences through project KJCX2-YW-T24.We present Doppler images of RS CVn-type binary II Peg based on two data sets obtained in 2004 February and November. In order to improve signal-to-noise ratio and reliability,we apply least-squares deconvolution technique to calculate average profiles from 2032 photospheric absorption lines. Both of the resulting surface images show a wide latitude distribution of starspots. Most spots are concentrated at a high-latitude belt above 60° and a low-latitude belt near equator. The starspots evolved dramatically between two observing runs, which may indicate shorter time-scale evolution in this epoch, especially for low-latitude belt. There is no stable preferred active longitude that can be found in our images. We also find out a possible phenomenon that the intermediate-latitude spot migrated poleward and merged with the high-latitude spot to make it stronger, which may reveal a more complex behaviour of starspots on II Peg. A potential change of orbital ephemeris zero-point was detected. This may imply an orbital period change of II Peg like other active close binaries.Peer reviewe
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