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http://hdl.handle.net/10553/46023
Título: | GIANO-B Online Data Reduction Software at the TNG | Autores/as: | Harutyunyan, Avet Rainer, Monica Hernandez, Nauzet Oliva, Ernesto Guerra, Jose Lodi, Marcello Juan, Jose San Bignamini, Andrea Ghedina, Adriano Ghinassi, Francesca Molinari, Emilio Benatti, Serena Carleo, Ilaria Claudi, Riccardo Micela, Giuseppina Tozzi, Andrea Baffa, Carlo Baruffolo, Andrea Biliotti, Valdemaro Buchschacher, Nicolas Cecconi, Massimo Cosentino, Rosario Falcini, Gilberto Fantinel, Daniela Fini, Luca Galli, Alberto Giani, Elisabetta Gonzalez, Carlos Gonzalez-Alvarez, Esther Gonzalez, Manuel Gratton, Raffaele Diaz, Marcos Hernandez Iuzzolino, Marcella Malavolta, Luca Maldonado, Jesus Origlia, Livia Poretti, Ennio Ventura, Hector Perez Puglisi, Alfio Riverol, Carlos Riverol, Luis Sanna, Nicoletta Scuderi, Salvatore Seeman, Ulf Sozzetti, Alessandro Sozzi, Mauro |
Clasificación UNESCO: | 22 Física | Fecha de publicación: | 2018 | Publicación seriada: | Proceedings of SPIE - The International Society for Optical Engineering | Resumen: | GIANO-B is the high resolution near-infrared (NIR) spectrograph of the Telescopio Nazionale Galileo (TNG), which started its regular operations in October 2017. Here we present GIANO-B Online Data Reduction Software (DRS) operating at the Telescope. GIANO-B Online DRS is a complete end-to-end solution for the spectrograph real-time data handling. The Online DRS provides management, processing and archival of GIANO-B scientific and calibration data. Once the instrument control software acquires the exposure ramp segments from the detector, the DRS ensures the complete data flow until the final data products are ingested into the science archive. A part of the Online DRS is GOFIO software, which performs the reduction process from ramp-processed 2D spectra to extracted and calibrated 1D spectra. A User Interface (UI) developed as a part of the Online DRS provides basic information on the final reduced data, thus allowing the observer to take decisions in real-time during the night and adjust the observational strategy as needed. | URI: | http://hdl.handle.net/10553/46023 | ISBN: | 9781510619654 | ISSN: | 0277-786X | DOI: | 10.1117/12.2312690 10.1117/12.2312690 |
Fuente: | Proceedings of SPIE - The International Society for Optical Engineering[ISSN 0277-786X],v. 10706 (1070642) |
Colección: | Actas de congresos |
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