<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Casella, C.</style></author><author><style face="normal" font="default" size="100%">Costantini, H.</style></author><author><style face="normal" font="default" size="100%">Lemut, a.</style></author><author><style face="normal" font="default" size="100%">Limata, B.</style></author><author><style face="normal" font="default" size="100%">Bemmerer, D.</style></author><author><style face="normal" font="default" size="100%">Bonetti, R.</style></author><author><style face="normal" font="default" size="100%">Broggini, C.</style></author><author><style face="normal" font="default" size="100%">Campajola, L.</style></author><author><style face="normal" font="default" size="100%">Cocconi, P.</style></author><author><style face="normal" font="default" size="100%">Corvisiero, P.</style></author><author><style face="normal" font="default" size="100%">Cruz, J.</style></author><author><style face="normal" font="default" size="100%">D'Onofrio, a.</style></author><author><style face="normal" font="default" size="100%">Formicola, a.</style></author><author><style face="normal" font="default" size="100%">Fülöp, Z.</style></author><author><style face="normal" font="default" size="100%">Gervino, G.</style></author><author><style face="normal" font="default" size="100%">Gialanella, L.</style></author><author><style face="normal" font="default" size="100%">Guglielmetti, a.</style></author><author><style face="normal" font="default" size="100%">Gustavino, C.</style></author><author><style face="normal" font="default" size="100%">Gyurky, G.</style></author><author><style face="normal" font="default" size="100%">Loiano, a.</style></author><author><style face="normal" font="default" size="100%">Imbriani, G.</style></author><author><style face="normal" font="default" size="100%">Jesus, a. P.</style></author><author><style face="normal" font="default" size="100%">Junker, M.</style></author><author><style face="normal" font="default" size="100%">Musico, P.</style></author><author><style face="normal" font="default" size="100%">Ordine, a.</style></author><author><style face="normal" font="default" size="100%">Parodi, F.</style></author><author><style face="normal" font="default" size="100%">Parolin, M.</style></author><author><style face="normal" font="default" size="100%">Pinto, JV</style></author><author><style face="normal" font="default" size="100%">Prati, P.</style></author><author><style face="normal" font="default" size="100%">Ribeiro, J P</style></author><author><style face="normal" font="default" size="100%">Roca, V.</style></author><author><style face="normal" font="default" size="100%">Rogalla, D.</style></author><author><style face="normal" font="default" size="100%">Rolfs, C</style></author><author><style face="normal" font="default" size="100%">Romano, M.</style></author><author><style face="normal" font="default" size="100%">Rossi-Alvarez, C.</style></author><author><style face="normal" font="default" size="100%">Rottura, a.</style></author><author><style face="normal" font="default" size="100%">Schuemann, F.</style></author><author><style face="normal" font="default" size="100%">Somorjai, E.</style></author><author><style face="normal" font="default" size="100%">Strieder, F.</style></author><author><style face="normal" font="default" size="100%">Terrasi, F.</style></author><author><style face="normal" font="default" size="100%">Trautvetter, H. P.</style></author><author><style face="normal" font="default" size="100%">Vomiero, a.</style></author><author><style face="normal" font="default" size="100%">Zavatarelli, S.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">{A new setup for the underground study of capture reactions}</style></title><secondary-title><style face="normal" font="default" size="100%">Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment</style></secondary-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">160</style></keyword><keyword><style  face="normal" font="default" size="100%">169</style></keyword><keyword><style  face="normal" font="default" size="100%">2002</style></keyword><keyword><style  face="normal" font="default" size="100%">489</style></keyword><keyword><style  face="normal" font="default" size="100%">a</style></keyword><keyword><style  face="normal" font="default" size="100%">a new setup for</style></keyword><keyword><style  face="normal" font="default" size="100%">b</style></keyword><keyword><style  face="normal" font="default" size="100%">bemmerer d</style></keyword><keyword><style  face="normal" font="default" size="100%">bonetti a</style></keyword><keyword><style  face="normal" font="default" size="100%">broggini e</style></keyword><keyword><style  face="normal" font="default" size="100%">c</style></keyword><keyword><style  face="normal" font="default" size="100%">campajola c</style></keyword><keyword><style  face="normal" font="default" size="100%">capture reactions</style></keyword><keyword><style  face="normal" font="default" size="100%">casella a</style></keyword><keyword><style  face="normal" font="default" size="100%">cocconi b</style></keyword><keyword><style  face="normal" font="default" size="100%">corvisiero b</style></keyword><keyword><style  face="normal" font="default" size="100%">costantini b</style></keyword><keyword><style  face="normal" font="default" size="100%">cruz f</style></keyword><keyword><style  face="normal" font="default" size="100%">d</style></keyword><keyword><style  face="normal" font="default" size="100%">h</style></keyword><keyword><style  face="normal" font="default" size="100%">in physics research a</style></keyword><keyword><style  face="normal" font="default" size="100%">j</style></keyword><keyword><style  face="normal" font="default" size="100%">l</style></keyword><keyword><style  face="normal" font="default" size="100%">lear instruments and methods</style></keyword><keyword><style  face="normal" font="default" size="100%">lemut b</style></keyword><keyword><style  face="normal" font="default" size="100%">limata c</style></keyword><keyword><style  face="normal" font="default" size="100%">onofrio g</style></keyword><keyword><style  face="normal" font="default" size="100%">p</style></keyword><keyword><style  face="normal" font="default" size="100%">r</style></keyword><keyword><style  face="normal" font="default" size="100%">the underground study of</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2002</style></year></dates><volume><style face="normal" font="default" size="100%">489</style></volume><pages><style face="normal" font="default" size="100%">160–169</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;For the study of astrophysically relevant capture reactions in the underground laboratory LUNA a new setup of high sensitivity has been implemented. The setup includes a windowless gas target, a 4$π$ BGO summing crystal, and beam calorimeters. The setup has been recently used to measure the d(p,$\gamma$)3He cross-section for the first time within its solar Gamow peak, i.e. down to 2.5keV c.m. energy. The features of the optimized setup are described. © 2002 Elsevier Science B.V. All rights reserved.&lt;/p&gt;
</style></abstract><notes><style face="normal" font="default" size="100%">n/a</style></notes></record></records></xml>