HCI NIRISS Limiting Contrast
Treatment of limiting contrast (Climit) is based on current information about telescope aberrations and the expected performance of JWST NIRISS AMI.
Limiting-contrast, Climit(s), is the companion-to-host flux ratio of the minimum detectable companion. It is the detection limit and the best that can be done.
The article HCI Contrast Considerations provides a general treatment of "contrast" (C), including Climit(s).
Climit(s) is a function of essentially everything related to high-contrast imaging (HCI): myriad eclectic technical factors and procedures, end-to-end. This treatment of Climit(s) for NIRISS AMI is based on Greenbaum et al. (2015).
Figure 1 shows the best available treatment of Climit(s) for the NIRISS AMI. This graphic is adapted from Figure 6 in Greenbaum et al. (2015).
The "technical factors" or assumptions behind the curves in Figure 1 include:
- Theoretical binary target
- Good flat field measurements with subpixel accuracy by precise positioning
- No variation of sensitivity within a pixel (intra-pixel sensitivity, or IPS)
Negligible phase closure errors due to static piston in the pupil
- Companion-to-host flux ratio Cflux = 10–2 (solid curves) and Cflux = 10–3 (dashed curves)
- False alarm probability (unknown)
- Currently available estimates of JWST aberrations (outdated)
- Filters F277M and F430M
Under those assumptions, Figure 1 shows the estimated limiting contrast ratio for 5-sigma detection of a faint companion near a bright host as a function of their apparent separation s in mas.
If the user's operating point (s, Cflux) lies above a color curve, that source is detectable under the technical and procedural assumptions of Greenbaum et al. (2015).
This is the best information on limiting performance for NIRISS AMI at the current time. In the future, with a better understandings of wavefront errors and other technical factors, or when users become interested in different combinations of technical factors, improved calculations of Climit(s) will be made available.
Meanwhile, users may be able to extrapolate estimates of Climit(s) using the Exposure Time Calculator (ETC) and other proposal tools.
Greenbaum, A.Z., Pueyo, L., Sivaramakrishnan, A., et al. 2015, ApJ, 798, 68
An Image-Plane Algorithm for JWST's Non-Redundant Aperture Mask Data