Created by: Kevin Volk, Gabriel Brammer, Deepashri Thatte, Joseph Filippazzo & Jason Rowe
The following data consist of simulations of four observing configurations of the JWST Near-Infrared Imager and Slitless Spectrograph (NIRISS) instrument:
Imaging
Aperture-Masking Interferometry (AMI)
Wide-Field Slitless Spectroscopy (WFSS)
Single-Object Slitless Spectroscopy (SOSS)
The simulations are summarized below.
For details, see the extensive description of the NIRISS_Data_Simulations from the team, and the even more detailed description of the WFSS simulations in the README file.
The simulations include the following effects:
Detector noise, bad pixels, and bias drift
Spectral traces and spectral dispersions as measured in ground testing
The expected sensitivities of the various NIRISS modes
Note that detector non-linearity is not simulated.
All simulations adopt NISRAPID read-out (NB: each frame constitutes a separate group in the integration).
Detector characteristics match what was measured in ground-testing.
The following instrument configurations and targets were simulated:
Observing Configurations & Operating Modes
Configuration
Optical Element
Read Mode
Scene
Imaging
F200W
Full
4-point dither within the PHAT survey of M31
AMI
P750L
Subarray (80×80)
Binary star, and a star + exoplanet system
WFSS
F200W+GR150C
Full
4-point dither of the GOODS-S field
F200W+GR150R
SOSS
F1130W
Subarray (2048×256)
Planet host GJ 436 (aka Ross 905)
Data Files
Use the links in the following tables to download the files of interest.
The contents of the *_uncal files contain data as processed to Level-1b[1] (i.e., assembled image, ready to be calibrated), including associated metadata.
The contents of the *_rate and *_rateints files contain data as processed to Level-2a (i.e., countrate or countrate per integration images, respectively, derived from ramps and ready for instrument signature removal).
[1] The format and organization of the raw data and metadata in the FITS files is the same as that expected for Level-1b products (ca. 2017 Mar). Thus, these files could be run through the JWST pipeline.