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Euclid. IV. The NISP Calibration Unit

Euclid Collaboration F. Hormuth K. Jahnke M. Schirmer C. G. Lee T. Scott +495 lainnya
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Abstrak

The near-infrared calibration unit (NI-CU) on board NISP is the first astronomical calibration lamp based on LED to be operated in space. is a mission in ESA's Cosmic Vision 2015--2025 framework to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5 accuracy in a survey homogeneously mapping sim \,14\,000\,deg$^2$ of extragalactic sky requires a very detailed characterisation of NIR detector properties as well as constant monitoring of them in flight. To cover two of the main contributions -- relative pixel-to-pixel sensitivity and non-linearity characteristics -- and to support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous ($<$\,12 variations) and temporally stable illumination (0.1--0.2 over 1200\,s) over the NISP detector plane with minimal power consumption and energy dissipation. NI-CU covers the spectral range sim \,nm -- at cryo-operating temperature -- at five fixed independent wavelengths to capture wavelength-dependent behaviour of the detectors, with fluence over a dynamic range of gtrsim \,100 from sim $. For this functionality, NI-CU is based on LED . We describe the rationale behind the decision and design process, the challenges in sourcing the right LED and the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities, and performance as well as its limits. NI-CU has been integrated into NISP and the satellite, and since launch in July 2023, it has started supporting survey operations.

Topik & Kata Kunci

Physics

Penulis (500)

E

Euclid Collaboration F. Hormuth

K

K. Jahnke

M

M. Schirmer

C

C. G. Lee

T

T. Scott

R

R. Barbier

S

S. Ferriol

W

W. Gillard

F

F. Grupp

R

R. Holmes

W

W. Holmes

B

B. Kubik

J

J. Macías-Pérez

M

M. Laurent

J

J. Marpaud

M

M. Marton

E

E. Medinaceli

G

G. Morgante

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R. Toledo-Moreo

M

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H

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A

A. Secroun

M

M. Seiffert

P

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C

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C

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A

A. Amara

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M

M. Baldi

A

A. Balestra

S

S. Bardelli

P

P. Battaglia

R

R. Bender

C

C. Bodendorf

D

D. Bonino

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E. Branchini

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M. Brescia

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J. Brinchmann

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S. Camera

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V. Capobianco

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C. Carbone

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V. Cardone

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S. Casas

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C. Conselice

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J

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A

A. Engineering

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17 Goethestr.

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69181 Leimen

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Germany

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17 Konigstuhl

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69117 Heidelberg

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von Hoerner Sulger GmbH

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8. Schlossplatz

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68723 Schwetzingen

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1. EumetsatAllee

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CNRSIN2p3

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I. Lyon

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Umr 5822

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Villeurbanne

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F-69100

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France

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A. Universit'e

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Cppm

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Marseille

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85748 Garching

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1. Scheinerstrasse

8

8. Munchen

S

Surrey Satellite Technology Limited

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Tycho House

2

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Surrey Research Park

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Guildford

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GU2 7YE

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Uk

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Pasadena

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Italy

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38200

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Tenerife

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Surrey

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Format Sitasi

APA MLA BibTeX
Hormuth, E.C.F., Jahnke, K., Schirmer, M., Lee, C.G., Scott, T., Barbier, R. et al. (2024). Euclid. IV. The NISP Calibration Unit. https://doi.org/10.1051/0004-6361/202450345

Akses Cepat

Lihat di Sumber doi.org/10.1051/0004-6361/202450345
Informasi Jurnal
Tahun Terbit
2024
Bahasa
en
Total Sitasi
2×
Sumber Database
Semantic Scholar
DOI
10.1051/0004-6361/202450345
Akses
Open Access ✓