Calibration of MAJIS (Moons And Jupiter Imaging Spectrometer). II. Spatial calibration.


Journal

The Review of scientific instruments
ISSN: 1089-7623
Titre abrégé: Rev Sci Instrum
Pays: United States
ID NLM: 0405571

Informations de publication

Date de publication:
01 Apr 2024
Historique:
received: 17 02 2024
accepted: 05 04 2024
medline: 23 4 2024
pubmed: 23 4 2024
entrez: 23 4 2024
Statut: ppublish

Résumé

MAJIS, Moons and Jupiter Imaging Spectrometer, is one of the scientific payloads aboard European Space Agency's Jupiter Icy Moons Explorer mission. This instrument underwent a comprehensive characterization and calibration campaign before integration on the spacecraft. In this work, we report on the measurements of the instrumental spatial responses, including the slit and pixel functions, the knife edge function, the ensquared energy, and the keystone aberration. The measurements were repeated in several positions of the field of view and within the range of MAJIS temperatures during science observations. The goal was to characterize the instrument's response under a wide set of conditions and at different visible-infrared wavelengths. The experimental setups employed to perform calibrations are described in detail, and the methodology applied to derive the instrumental spatial responses is discussed. After launch, minor changes in the instrument response and the coalignment between the two spectral channels were identified by comparing on-ground data with the first in-flight data returned by MAJIS.

Identifiants

pubmed: 38651987
pii: 3284549
doi: 10.1063/5.0203872
pii:
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Informations de copyright

© 2024 Author(s). Published under an exclusive license by AIP Publishing.

Auteurs

Gianrico Filacchione (G)

INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00133 Rome, Italy.

Paolo Haffoud (P)

Institut d'Astrophysique Spatial, CNRS-Université Paris-Saclay, Orsay 91400, France.

Francois Poulet (F)

Institut d'Astrophysique Spatial, CNRS-Université Paris-Saclay, Orsay 91400, France.

Giuseppe Piccioni (G)

INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00133 Rome, Italy.

Yves Langevin (Y)

Institut d'Astrophysique Spatial, CNRS-Université Paris-Saclay, Orsay 91400, France.

Leonardo Tommasi (L)

Leonardo Company, via delle Officine Galileo, 1, Campi Bisenzio, Florence 50013, Italy.

Alessandra Barbis (A)

Leonardo Company, via delle Officine Galileo, 1, Campi Bisenzio, Florence 50013, Italy.

John Carter (J)

Institut d'Astrophysique Spatial, CNRS-Université Paris-Saclay, Orsay 91400, France.

Irene Guerri (I)

Leonardo Company, via delle Officine Galileo, 1, Campi Bisenzio, Florence 50013, Italy.

Cydalise Dumesnil (C)

Institut d'Astrophysique Spatial, CNRS-Université Paris-Saclay, Orsay 91400, France.

Simone De Angelis (S)

INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00133 Rome, Italy.

Mathieu Vincendon (M)

Institut d'Astrophysique Spatial, CNRS-Université Paris-Saclay, Orsay 91400, France.

Stefania Stefani (S)

INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00133 Rome, Italy.

Cedric Pilorget (C)

Institut d'Astrophysique Spatiale, CNRS-Universite Paris-Saclay, Orsay 91400, France and Institut Universitaire de France, Paris, France.

Federico Tosi (F)

INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00133 Rome, Italy.

Sebastien Rodriguez (S)

Institut de Physique du Globe de Paris, CNRS-Université Paris-Cité, Paris 75005, France.

Classifications MeSH