Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Alberto Maurizio Chavan"'
Publikováno v:
SPIE Proceedings.
In order to provide ALMA users with a comprehensive view of their observing projects, we developed the ALMA Snooping Project Interface (SnooPI) application. The simple and intuitive interface allows scientists to follow the status of their projects,
Autor:
E. Villard, E. Akiyama, S. L. Tanne, S. Randall, B. Vila Vilaro, R. Kurowski, Alberto Maurizio Chavan
Publikováno v:
Observatory Operations: Strategies, Processes, and Systems VI.
Data produced by ALMA for the community undergoes a rigorous quality assurance (QA) process, from the initial observation ("QA0") to the final science-ready data products ("QA2"), to the QA feedback given by the Principal Investigators (PIs) when the
Autor:
G. Raffi, Jeff Kern, Brian Glendenning, Alberto Maurizio Chavan, J. Ibsen, Joseph Schwarz, George Kosugi, Erich Schmid
Publikováno v:
SPIE Proceedings.
At the end of 2012, ALMA software development will be completed. While new releases are still being prepared following an incremental development process, the ALMA software has been in daily use since 2008. Last year it was successfully used for the
Autor:
P. Nass, D. Dorigo, K. Haggouchi, D. Sforna, Alberto Maurizio Chavan, Fabio Sogni, Michele Peron, L. E. Tacconi-Garman, Nathalie Fourniol, Markus Dolensky
Publikováno v:
Observatory Operations: Strategies, Processes, and Systems II.
ESO introduced a User Portal for its scientific services in November 2007. Registered users have a central entry point for the Observatory's offerings, the extent of which depends on the users' roles - see [1]. The project faced and overcame a number
Autor:
Alberto Maurizio Chavan, Michele Peron, P. Nass, Tim Canavan, L. E. Tacconi-Garman, Fabio Sogni
Publikováno v:
SPIE Proceedings.
The European Southern Observatory (ESO) is in the process of creating a central access point for all services offered to its user community via the Web. That gateway, called the User Portal, will provide registered users with a personalized set of se
Autor:
Marcus Schilling, Heiko Sommer, Alan Bridger, Leonardo Testi, David A. Clarke, Alberto Maurizio Chavan, Joseph Schwarz
Publikováno v:
SPIE Proceedings.
A number of tools exist to aid in the preparation of proposals and observations for large ground and space-based observatories (VLT, Gemini, HST being examples). These tools have transformed the way in which astronomers use large telescopes. The ALMA
Autor:
Michele Peron, Judith Anwunah, Alberto Maurizio Chavan, Fabio Sogni, Nick Kornweibel, Tim Canavan, D. Dorigo
Publikováno v:
SPIE Proceedings.
All ESO Science Operations teams operate on Observing Runs, loosely defined as blocks of observing time on a specific instrument. Observing Runs are submitted as part of an Observing Proposal and executed in Service or Visitor Mode. As an Observing R
Autor:
Walter Jaffe, Andrea Richichi, Markus Wittkowski, Peter J. Quinn, Benoit Pirenne, Pierre Kervella, Pascal Ballester, Andreas Wicenec, Stefano Zampieri, Rainer Wilhelm, Markus Schöller, Carlos Guirao, Alberto Maurizio Chavan, Cyrus Sabet, Andreas Glindemann, Bruce Wiseman, Michele Peron
Publikováno v:
Observatory Operations to Optimize Scientific Return III.
In this article we present the Data Flow System (DFS) for the Very Large Telescope Interferometer (VLTI). The Data Flow System is the VLT end-to-end software system for handling astronomical observations from the initial observation proposal phase th
Autor:
D. Dorigo, Andreas Wicenec, Nicolas Devillard, Cynthia Mavros, Fabio Sogni, Carlo Izzo, Francesco Ricciardi, Alberto Maurizio Chavan, J. Vinther, Pascal Ballester, Stefano Zampieri, Andrea Modigliani, Karim Haggouchi, Klaus Banse, Tim Canavan, Michele Peron, J. Knudstrup, Yves Jung, Carlos Guirao, Ralf Palsa, Gerhard Mekiffer, Nick Kornweibel, Peter J. Quinn, Bruce Wiseman, Cyrus Sabet
Publikováno v:
Observatory Operations to Optimize Scientific Return III.
The VLT Data Flow System (DFS) has been developed to maximize the scientific output from the operation of the ESO observatory facilities. From its original conception in the mid 90s till the system now in production at Paranal, at La Silla, at the ES
Autor:
Andreas Wicenec, Alberto Maurizio Chavan, Benoit Pirenne, Michele Peron, Vincent Coudé du Foresto, Pierre Kervella, Andreas Glindemann, Bill Cotton, Isabelle Percheron, Peter J. Quinn, Markus Wittkowski, Walter Jaffe, Pascal Ballester, Than Phan Duc, Rainer Wilhelm, Carlos Guirao, Andrea Richichi, Antonio Longinotti, Markus Schoeller, Stefano Zampieri
Publikováno v:
SPIE Proceedings.
The Data Flow System is the VLT end-to-end system for handling astronomical observations from the initial observation proposal phase through the acquisition, processing and control of the astronomical data. The VLT Data Flow System has been in place