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2024-07-24
The status of the NIR arm of the SOXS Instrument toward the PAE
Fabrizio VitaliMatteo GenoniMatteo AlivertiKalyan RadhakrishnanFederico BattainiPaolo D'AvanzoFrancesco D'AlessioGiorgio ParianiLuca OggioniSalvatore ScuderiDavide RicciEugenio MartinettiAntonio MiccichèGaetano NicotraMirko ColapietroSergio D'OrsiMatteo MunariLuigi LessioSimone Di FilippoAndrea ScaudoGiancarlo BellassaiRosario Di BenedettoGiovanni OcchipintiMarco LandoniMatteo AccardoLeander MehrganDerek IvesCarlotta ScirèSergio CampanaPietro SchipaniRiccardo ClaudiGiulio CapassoMarco RivaRicardo Zanmar SanchezJosé Antonio Araiza-DuránIair ArcaviAndrea BaruffoloSagi Ben-AmiAnna BrucalassiRachel BruchEnrico CappellaroRosario CosentinoMarco De PascaleMassimo Della ValleAvishay Gal-YamMarcos Hernandez DíazOfir HershkoJari KotilainenHanindyo KuncarayaktiGianluca Li CausiLaurent MartySeppo MattilaHector Pérez VenturaGiuliano PignataMichael RappaportAdam RubinBernardo SalasnichStephen SmarttMaximilian StritzingerDavid Young
文献摘要
The Son Of X-Shooter (SOXS) is a single object spectrograph, built by an international consortium for the 3.58-m ESO New Technology Telescope at the La Silla Observatory [1]. It offers a simultaneous spectral coverage over 350-2000 nm, with two separate spectrographs. In this paper we present the status of the Near InfraRed (NIR) cryogenic echelle cross-dispersed spectrograph [1], in the range 0.80-2.00 μm with 15 orders, equipped with an 2k x 2k Hawaii H2RG IR array from Teledyne, working at 40K, that is currently assembled and tested on the SOXS instrument, in the premises of INAF in Padova. We describe the different tests and results of the cryo, vacuum, opto-mechanics and detector subsystems that finally will be part of the PAE by ESO.
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