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The JWST NIRCam pupil and filter wheels include the filters, weak lensesgrisms, and coronagraph Lyot stops that may be used in combination.


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Introduction

Parent page: NIRCam Instrumentation

Each NIRCam module has short wavelength (0.6–2.3 μm) and long wavelength (2.4–5.0 μm) channels, each with a pupil wheel and filter wheel of 12 elements each. Many combinations of pupil and filter wheel elements are allowed as described below. These elements include:

  • extra-wide-, wide-, medium-, and narrowband filters with R = λ/Δλ ~ 1, 4, 10, and 100, respectively;
  • coronagraph Lyot stops to suppress diffracted light that passes the occulting masks on the focal plane;
  • grism elements in the long wavelength channel—two elements are available, dispersing light along detector rows and columns, respectively;
  • weak lenses to defocus light from bright sources to avoid detector saturation, and also used for telescope alignment;
  • clear positions (empty holes) in the pupil wheel to be used in combination with filter wheel elements;
  • dark elements used for calibration; 
  • other elements used only for wavefront sensing and telescope alignment, including the PAPPA (pupil alignment pinhole projector assembly), DHS (dispersed Hartman sensing), and IPR Wedge (internal phase retrieval).

 


Pupil and filter wheels characteristics

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Figure 1. NIRCam pupil and filter wheels


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Each NIRCam module contains the optical elements depicted above, including pupil and filter wheels that hold a total of 48 optical elements. Filters are color-coded by wavelength. Wider filters are shown in the figure as more transparent than narrower filters.



Table 1. NIRCam pupil and filter wheel elements

Short wavelength channel
(0.6–2.3 μm)

  

Long wavelength channel
(2.4–5.0 μm)


Pupil wheel

CLEAR

Dark

PAPPA

WL +8

DHS 0°

WL -8

Lyot round

F162M CO

DHS 60°

Lyot bar

F164N [Fe II]

IPR Wedge


 


Filter wheel

F070W

F090W

F115W

F150W

F200W

F212N H2

WL+4 +F212N2

F187N Pa-α

F210M

F182M

F140M

F150W2


  


Pupil wheel

CLEAR

Dark

IPR Wedge

PAPPA

F405N Br-α

F323N H2

Lyot round

Grism R V2

F466N CO

Grism C V3

F470N H2

Lyot bar


 


Filter wheel

F277W

F356W

F444W

F300M

F480M

F410M

F360M

F430M

F460M

F250M

F335M

F322W2



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Notes:

  • Black: bandpass filters named W2W, M,  have R = λ/Δλ ~ 1, 4, 10, 100, respectively

  • Orangecoronagraphic Lyot stops in the pupil wheels used in conjunction with filters and focal plane occulting masks

  • Green: grism elements disperse spectra along detector rows (R) or columns (C), used in conjunction with filters

  • Magenta: WL, weak lens, used to defocus for mirror alignment or bright star imaging without saturation

  • Gray: CLEAR positions, empty holes in the pupil wheel

  • Wavefront sensing/calibration (not available for science)

    • DHS, dispersed Hartman sensing (sub-aperture grisms): coarse phasing alignment of JWST's mirrors

    • PAPPA, pupil alignment pinhole projector assembly: align NIRCam with the JWST Optical Telescope Element (OTE)

    • IPR, internal phase retrieval, wedge: measure NIRCam wavefront errors using LEDs mounted on coronagraphs

    • Dark: blocks incoming light for dark current measurements



Allowed combinations between pupil and filter wheel elements

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Figure 2. Allowed combinations of optical elements in the NIRCam short wavelength channel

Figure 2. Allowed combinations of optical elements in the NIRCam short wavelength channel

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Filter wheel elements (left column) may be paired with pupil wheel elements (top row) as listed below. Pupil wheel elements in gray on the right are only available for wavefront sensing and calibration, not science.
Pair availability
- Green: available for science
- Yellow: restricted use for wavefront sensing, calibration, or engineering"
- Red: disallowed; not useful
Names of wide, medium, and narrow filters are formatted as bold, regular, and italic, respectively.



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Figure 3. Allowed combinations of optical elements in the NIRCam long wavelength channel

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Available pupil and filter wheel pairings for the long wavelength channel. Same color codes as Figure 2.
- Green: available for science
- Yellow: restricted use for wavefront sensing, calibration, or engineering"
- Red: disallowed; not useful
Names of wide, medium, and narrow filters are formatted as bold, regular, and italic, respectively. 

335, 430: the filters allowed in combination with a round coronagraph Lyot stop depend on the occulting mask used: MASK335R1 or MASK430R.


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References

JWST technical documents

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Last updated

Published December 28, 2016


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Published March 02, 2017