Skip navigation
  • INAF logo
  • Home
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects
  • Explore by
    • Research outputs
    • Researchers
    • Organization units
    • Projects
  • Login:
    • My DSpace
    • Receive email
      updates
    • Edit Account details
  • Italian
  • English

  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/24127
Title: The spectral imaging facility: Setup characterization
Authors: DE ANGELIS, Simone 
AMMANNITO, ELEONORA
Di Iorio, Tatiana
DE SANCTIS, MARIA CRISTINA 
Manzari, Paola Olga
Liberati, Fabrizio
Tarchi, Fabio
Dami, Michele
Olivieri, Monica
Pompei, Carlo
Mugnuolo, Raffaele
Issue Date: 2015
Journal: REVIEW OF SCIENTIFIC INSTRUMENTS 
Number: 86
Issue: 9
First Page: 093101
Abstract: The SPectral IMager (SPIM) facility is a laboratory visible infrared spectrometer developed to support space borne observations of rocky bodies of the solar system. Currently, this laboratory setup is used to support the DAWN mission, which is in its journey towards the asteroid 1-Ceres, and to support the 2018 Exo-Mars mission in the spectral investigation of the Martian subsurface. The main part of this setup is an imaging spectrometer that is a spare of the DAWN visible infrared spectrometer. The spectrometer has been assembled and calibrated at Selex ES and then installed in the facility developed at the INAF-IAPS laboratory in Rome. The goal of SPIM is to collect data to build spectral libraries for the interpretation of the space borne and in situ hyperspectral measurements of planetary materials. Given its very high spatial resolution combined with the imaging capability, this instrument can also help in the detailed study of minerals and rocks. In this paper, the instrument setup is first described, and then a series of test measurements, aimed to the characterization of the main subsystems, are reported. In particular, laboratory tests have been performed concerning (i) the radiation sources, (ii) the reference targets, and (iii) linearity of detector response; the instrumental imaging artifacts have also been investigated. <P />
Acknowledgments: Acknowledgments We wish to thank the Italian Space Agency (ASI) for fully supporting the facility realization and laboratory activities.
URI: http://hdl.handle.net/20.500.12386/24127
URL: https://aip.scitation.org/doi/10.1063/1.4929433
ISSN: 0034-6748
DOI: 10.1063/1.4929433
Bibcode ADS: 2015RScI...86i3101D
Fulltext: open
Appears in Collections:1.01 Articoli in rivista

Files in This Item:
File Description SizeFormat 
SDeAngelis - spim_articolo_tecnico_rev1.pdfpostprint2.35 MBAdobe PDFView/Open
Show full item record

Page view(s)

15
checked on Jan 27, 2021

Download(s)

4
checked on Jan 27, 2021

Google ScholarTM

Check

Altmetric


Items in DSpace are published in Open Access, unless otherwise indicated.


Explore by
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects

Informazioni e guide per autori

https://openaccess-info.inaf.it: tutte le informazioni sull'accesso aperto in INAF

Come si inserisce un prodotto: le guide a OA@INAF

La Policy INAF sull'accesso aperto

Documenti e modelli scaricabili

Feedback
Built with DSpace-CRIS - Extension maintained and optimized by Logo 4SCIENCE