EURECA
Kraus H., Armengaud E., Augier C., Bauer M., Bechtold N., Benoit A., Bento A., Berge L., Blümer J., Bornschein L., Broniatowski A., Brown A., Camus P., Censier B., Chantelauze A., Chapellier M., Chardin G., Ciemniak C., Collin S., Coron N., Coulter P., Cox A., Crauste O., Danevich FA., Daw E., De Jésus M., De Marcillac P., Deuter G., Domange J., Drexlin G., Dumoulin L., Eitel K., Feilitzsch FV., Filosofov D., Gandit P., García E., Gascon J., Gerbier G., Gironnet J., Godfrin H., Graffin P., Grohmann S., Gros M., Hauff D., Henry S., Huff P., Ingleby S., Isaila C., Jochum J., Juillard A., Kiefer M., Kikuchi C., Kimmerle M., Kluck H., Kobychev VV., Kozlov V., Kudovbenko VM., Kudryavtsev VA., Lanfranchi JC., Loaiza P., Lubashevsky A., Marnieros S., Martinez ML., Mikhailik VM., Monfardini A., Nagorny SS., Navick XF., Nieder H., Niinikoski T., Nikolaiko AS., Olivieri E., Ortigoza Y., Pari P., Pattavina L., Paul B., Petricca F., Pfeiffer M., Pfister S., Pobes C., Poda DV., Podviyanuk RB., Polischuk OG., Ponsot P., Potzel W., Pröbst F., Puimedón J., Robinson M., Rolón T., Roth S., Rottler K., Rozov S., Sailer C., Salinas A., Sanglard V., Sarsa ML., Schäffner K., Schmaler J., Schmidt B., Scholl S., Scorza S.
EURECA (European Underground Rare Event Calorimeter Array) is an astro-particle physics facility aiming to directly detect galactic dark matter. The Laboratoire Souterrain de Modane has been selected as host laboratory. The EURECA collaboration unites CRESST, EDELWEISS and the Spanish-French experiment ROSEBUD, thus concentrating and focussing effort on cryogenic detector research in Europe into a single facility. EURECA will use a target mass of up to one ton, enough to explore WIMP - nucleon scalar scattering cross sections in the region of 10-9 - 10-10 picobarn. A major advantage of EURECA is the planned use of more than just one target material (multi target experiment for WIMP identification). © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.