Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Franco Colleoni"'
Autor:
Patrick J. Ingraham, Andy W. Clements, Tiago Ribeiro, Michael A. Reuter, Merlin Fisher-Levine, Joshua Hoblitt, Robert H. Lupton, Sandrine Thomas, Christopher W. Stubbs, Kirk Arndt, Nick Callahan, CHarles F. Claver, Franco Colleoni, Luis Corral, Peter Doherty, Frossie Economou, Angel Fausti, Tim Jeness, Htut Khine, Simon Krughoff, Nicholas Mondrik, Felipe Menanteau, David J. Mills, William O'Mullane, Kevin A. Reil, Mario Rivera, Brian Stalder, Jacques Sebag, Ian Shipsey, Roberto Tighe, Adam J. Thornton, Andres Villalobos, Oliver Wiecha
Publikováno v:
Software and Cyberinfrastructure for Astronomy VI.
Autor:
Tomislav Vucina, Edward Stover, Dave Mills, Christian Aguilar, Bo Xin, Freddy Muñoz, Brian Johnson, Oli Wiecha, Edward Hileman, Juan Lopez, Christopher Contaxis, Claudio Araya, Ron Harris, Douglas R. Neill, Gary Muller, Michael Booth, Franco Colleoni, Felipe Daruich, Ian Ordenes, Jacques Sebag, Jeff Urban, Eric Coughlin, Sandrine Thomas, Constanza Araujo, Neill Mills, Andy W. Clements, Garry Knight
Publikováno v:
Ground-based and Airborne Telescopes VIII.
The Vera C. Rubin Observatory is currently under construction on Cerro Pachon, in Chile. It was designed to conduct a 10-year multi-band survey of the southern sky with frequent re-visits (with both an intra- and extra-night cadence) to identify tran
Autor:
Pablo Zorzi, Christophe Granet, Nicolas Reyes, Leonardo Bronfman, Franco Colleoni, Jose Pizarro, F. P. Mena
Publikováno v:
Journal of Infrared, Millimeter, and Terahertz Waves. 33:17-24
A corrugated spline-profile horn has been designed to meet the stringent specifications and constraints of a receiver for Band 1 (31.3–45 GHz) of the Atacama Large Millimeter Array (ALMA). Given the physical restrictions of the receiver, the horn w
Autor:
Leonardo Bronfman, Patricio Mena, Ricardo Finger, Nicolas Reyes, Jose Pizarro, Francisco Navarrete, Franco Colleoni, Pablo Zorzi, Claudio Jarufe
Publikováno v:
SPIE Proceedings.
The lowest spectroscopic band devised for the Atacama Large Millimeter Array (ALMA), the so-called Band 1, covers the frequency range from 31 to 45 GHz. This band was not implemented during the rst construction phase of the telescope, but will be inc