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Euclid

ESA
Mission
with
Participation
from
NASA

 

Euclid
NASA
Science
Center
at
IPAC

Euclid has two instruments: a wide-field visible light imager, and a near-infrared imaging photometer and slitless spectrometer:

VIS instrument:

  • Focal plane array: 6×6 CCDs (4k×4k pixels each) with 0.101 arcsec pixel platescale
  • Field of view: 0.56 (deg)2
  • Wavelength coverage: one wide visible band (550-900 nm)
  • System point-spread function: 0.16 arcsec (FWHM) excluding pixelisation

NISP instrument:

  • Focal plane array: 4×4 HgCdTe NIR detectors (2k×2k pixels each) with 0.3 arcsec per pixel and 2.3 µm cut-off wavelength.
  • Imaging bands: Y (0.95  to 1.192 µm), J (1.192  to 1.544 µm), H (1.544  to 2 µm)
  • Grisms: 1 blue grism (0.92  to 1.3 µm); 3 identical red grisms (1.25  to 1.85 µm) at position angles 0 deg, 90 deg, 180 deg.
  • Spectral resolution: constant Δλ at  λ/Δλ ˃ 380 for an object of 0.5 arcsec diameter
  • FoV: 0.55 (deg)

FoV common to VIS & NISP:  0.53 (deg)2