RAINER, MonicaMonicaRAINERHARUTYUNYAN, AVETAVETHARUTYUNYANCARLEO, IlariaIlariaCARLEOOLIVA, ErnestoErnestoOLIVABENATTI, SERENASERENABENATTIBIGNAMINI, ANDREAANDREABIGNAMINICLAUDI, RiccardoRiccardoCLAUDIGonzalez-Alvarez, EstherEstherGonzalez-AlvarezSANNA, NicolettaNicolettaSANNAGhedina, AdrianoAdrianoGhedinaMICELA, GiuseppinaGiuseppinaMICELAMOLINARI, Emilio CarloEmilio CarloMOLINARITOZZI, AndreaAndreaTOZZIBAFFA, CarloCarloBAFFABARUFFOLO, AndreaAndreaBARUFFOLOBuchschacher, NicolasNicolasBuchschacherCecconi, MassimoMassimoCecconiCOSENTINO, RosarioRosarioCOSENTINOFALCINI, GilbertoGilbertoFALCINIFANTINEL, DanielaDanielaFANTINELFINI, LucaLucaFINIGALLI, ALBERTOALBERTOGALLIGhinassi, FrancescaFrancescaGhinassiGIANI, ElisabettaElisabettaGIANIGonzalez, CarlosCarlosGonzalezGonzalez, ManuelManuelGonzalezGRATTON, RaffaeleRaffaeleGRATTONGUERRA, JOSEJOSEGUERRAHernandez Diaz, MarcosMarcosHernandez DiazHernandez, NauzetNauzetHernandezIUZZOLINO, MarcellaMarcellaIUZZOLINOLodi, MarcelloMarcelloLodiMalavolta, LucaLucaMalavoltaMALDONADO PRADO, JesusJesusMALDONADO PRADOORIGLIA, LiviaLiviaORIGLIAPEREZ VENTURA, HECTORHECTORPEREZ VENTURAPUGLISI, Alfio TimothyAlfio TimothyPUGLISIRiverol, CarlosCarlosRiverolRiverol, LuisLuisRiverolSan Juan, JoseJoseSan JuanScuderi, SalvoSalvoScuderiSeeman, UlfUlfSeemanSOZZETTI, AlessandroAlessandroSOZZETTISOZZI, MAUROMAUROSOZZI2020-10-232020-10-232018978151061957997815106195860277-786Xhttp://hdl.handle.net/20.500.12386/27974The NIR echelle spectrograph GIANO-B at the Telescopio Nazionale Galileo is equipped with a fully automated online DRS: part of this pipeline is the GOFIO reduction software, that processes all the observed data, from the calibrations to the nodding or stare images. GOFIO reduction process includes bad pixel and cosmic removal, flat-field and blaze correction, optimal extraction, wavelength calibration, nodding or stare group processing. An offline version of GOFIO will allow the users to adapt the reduction to their needs, and to compute the radial velocity using telluric lines as a reference system. GIANO-B may be used simultaneously with HARPS-N in the GIARPS observing mode to obtain high-resolution spectra in a wide wavelength range (383-2450 nm) with a single acquisition. In this framework, GOFIO, as part of the online DRS, provides fast and reliable data reduction during the night, in order to compare the infrared and visible observations on the fly.ELETTRONICOenConference paper10.1117/12.23121302-s2.0-85051477246000452664300150https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10702/2312130/Introducing-GOFIO--a-DRS-for-the-GIANO-B-near/10.1117/12.2312130.short?SSO=12018SPIE10702E..66RFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering