Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Jose Piraces"'
Autor:
Freddy Muñoz, Jacques Sebag, Jose Piraces, Rolando Cantarutti, Roberto Tighe, Mario Rivera, Patricio Schurter
Publikováno v:
Ground-based and Airborne Telescopes VIII.
The optical axis of a Nasmyth telescope should be perpendicular to the Elevation axis and pass through the rotational center of the Tertiary mirror turret rotator. Realized by aligning a laser beam to the rotational center of the two field derotators
Publikováno v:
Ground-based and Airborne Telescopes VIII.
The Southern Astrophysical Research (SOAR) 4.1m telescope, located in Cerro Pachon, Chile, has an active optics system that uses a Shack Hartmann wave front sensor to achieve optimal image correction and focus. This Calibration Wave Front Sensor (CWF
Autor:
Claudio Araya, Nicole David, Rodrigo Alvarez, Jose Piraces, Guillermo Dubo, Vicente Vergara, Roberto Tighe, Cristian Moreno, Rossano Rivera
Publikováno v:
Ground-based and Airborne Telescopes VIII.
The SOAR telescope was designed to have a bare Aluminum coating. This coating is performed in the Gemini-South sputtering facility. Two coatings have been done on the SOAR mirror (2004 and 2009). On both occasions, the reflectivity obtained for the U
Autor:
Ron Probst, Chuck Henderson, J. H. Elias, Katelyn N. Allers, David James, Terry Herter, Everett Schlawin, Patricio Schurter, Nicole David, Roberto Tighe, Marco Bonati, Jose Piraces, John Wilson, Sean Points, Michael Warner
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy VIII.
We describe the design and implementation of a fourth version of the TripleSpec near-infrared spectrograph (TSpec4). This version of the instrument was designed for and first implemented on the 4-m Blanco telescope on Cerro Tololo, and subsequently c
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy VII.
The 4.1-m SOAR telescope needs fast tip-tilt guiding and active correction of focus and astigmatism to reach good image quality allowed by the excellent site seeing. A concept of the new guider with a 2×2 wavefront sensor is presented. It uses the X