Symphony 6, "Pathetique," B minor. Op.74.

Mode of access: Internet.

Nominations before the Senate Armed Services Committee, second session, 106th Congress : hearings before the Committee on Armed Services, United States Senate, One Hundred Sixth Congress, second session, on nominations of Rudy de Leon; Douglas A. Dworkin; Bernard D. Rostker; Gregory R. Dahlberg; Madelyn R. Creedon; Adm. Vernon E. Clark; Gen. John A. Gordon; Lt. Gen. Tommy R. Franks; Lt. Gen. William F. Kernan; Donald Mancuso; Roger W. Kallock; James E. Baker; Lt. Gen. Peter Pace; Lt. Gen. Charles R. Holland; Maj. Gen. Robert B. Flowers; and Robert B. Pirie, Jr., February 8; March 21; April 11; May 16, 24; June 27; July 26; September 6; October 3, 19, 2000.

Shipping list no.: 2001-0213-P.

An argument in favor of the reduction of the tax on manufactured tobacco, and against the transfer of the tax to the leaf, addressed to Jas. B. Casey and Frank Prague, delegates to the Tobacco convention, to be held in Washington, D.C., February 6, 1867 ...

Mode of access: Internet.

Report of the discussion between Robert Owen, Esq., and the Rev. Wm. Legg, B.A. : which took place in the Town Hall, Reading, March 5 & 6, 1839, on Mr. Owen's new views of society.

Goldsmiths'-Kress no. 31273.

Sendschreiben an Se. Hochwürden Herrn Dr. Joh. Fried. Röhr, betreffend die aus seiner kritischen Prediger-Bibliothek (1835 B. 16. H. 6.) hier abgedruckte Kritik des Buches: "Religionsbekenntnisse zweier Vernunftfreunde u.s.w."

Mode of access: Internet.

Two drawings of a house: Sheet no. 2, plan upper level, 5/2/52 revised 6/28/52; sheet no. 5, section B-B & section F-; F, 5/2/52 revised 6/28/52

Lance Burghardt bracketed his exposures and provided 3 different shots of these items (2 tifs, 1 jpg). Each shares same housescan number, differentiated by suffix 1of3, 2of3, or 3of3....

Left to right - Cuyler Lee, H.B. Joy, and Ernie," page 6

2 scans made - 1of1 includes caption pasted below, 2of2 = image only

Left to right - A.F. Bement, H.B. Joy, Cuyler Lee," page 6

2 scans made - 1of1 includes caption pasted below, 2of2 = image only

Hypervalent iodine in synthesis 92. A facile synthesis of 3-substituted-5,6-dihydroimidazo[2,1-b]thiazoles by cyclocondensation of alkynyl(phenyl)iodonium salts and imidazolidine-2-thione

A simple method for the synthesis of 3-substituted 5,6-dihydroimidazo[2,1-b]thiazoles is achieved by cyclocondensation of alkynyl(phenyl)iodonium salts with imidazolidine-2-thione.

Distinct Differentiation Programs Triggered by IL-6 And LPS in Teleost IgM+ B Cells in the Absence of Germinal Centers

We would like to thank Lucia Gonzalez and Maria Sanz for technical assistance. Professor Øystein Evensen is also acknowledged for providing us with the inactivated IPNV. This work was supported by the European Research Council (ERC Starting Grant 2011 280469) and by the European Commission under the 7th Framework Programme for Research and Technological Development (FP7) of the European Union (Grant Agreement 311993 TARGETFISH). T. W. received funding from the MASTS pooling initiative (The Marine Alliance for Science and Technology for Scotland). MASTS is funded by the Scottish Funding Council (grant reference HR09011).

The HARPS-N Rocky Planet Search. I. HD 219134 b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun

We know now from radial velocity surveys and transit space missions thatplanets only a few times more massive than our Earth are frequent aroundsolar-type stars. Fundamental questions about their formation history,physical properties, internal structure, and atmosphere composition are,however, still to be solved. We present here the detection of a systemof four low-mass planets around the bright (V = 5.5) and close-by (6.5pc) star HD 219134. This is the first result of the Rocky Planet Searchprogramme with HARPS-N on the Telescopio Nazionale Galileo in La Palma.The inner planet orbits the star in 3.0935 ± 0.0003 days, on aquasi-circular orbit with a semi-major axis of 0.0382 ± 0.0003AU. Spitzer observations allowed us to detect the transit of the planetin front of the star making HD 219134 b the nearest known transitingplanet to date. From the amplitude of the radial velocity variation(2.25 ± 0.22 ms-1) and observed depth of the transit(359 ± 38 ppm), the planet mass and radius are estimated to be4.36 ± 0.44 M⊕ and 1.606 ± 0.086R⊕, leading to a mean density of 5.76 ± 1.09 gcm-3, suggesting a rocky composition. One additional planetwith minimum-mass of 2.78 ± 0.65 M⊕ moves on aclose-in, quasi-circular orbit with a period of 6.767 ± 0.004days. The third planet in the system has a period of 46.66 ± 0.08days and a minimum-mass of 8.94 ± 1.13 M⊕, at0.233 ± 0.002 AU from the star. Its eccentricity is 0.46 ±0.11. The period of this planet is close to the rotational period of thestar estimated from variations of activity indicators (42.3 ± 0.1days). The planetary origin of the signal is, however, thepreferredsolution as no indication of variation at the corresponding frequency isobserved for activity-sensitive parameters. Finally, a fourth additionallonger-period planet of mass of 71 M⊕ orbits the starin 1842 days, on an eccentric orbit (e = 0.34 ± 0.17) at adistance of 2.56 AU.The photometric time series and radial velocities used in this work areavailable in electronic form at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr(ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/584/A72

Prevalencia de estrías posteriores en córnea de pacientes usuarios de 6 meses de lentes de contacto Lotrafilcon b

Tesis (Maestría en Ciencias de la Visión).-- Universidad de La Salle. Maestría en Ciencias de la Visión, 2014