Input Data Specifications

Spacecraft/Telescope Architecture (ARCH)

Nominal JWST orbit -- large L2 Lissajous (2012.092 to 2027.124; 15-yr duration)

Alternative JWST orbit -- worst-case stray-light orbit (2011.254 to 2021.219; 10-yr duration)

Other: * See Note.

Integrated Science Instrument Module (ISIM)

JWST Requirements

JWST Goals

Other: * See Note.

Observation Parameters

Target
Coordinates	, degrees
Coord. System	Equatorial (RA,Dec) Ecliptic (Long,Lat) Galactic (Long,Lat)
Diameter (arcsec)
SI Configuration
Sci Instrument	SELECT FGS_guider1 FGS_guider2 FGS_guider3 FGS_tf_lw FGS_tf_sw NIRCam_sw NIRCam_lw NIRSpec_grating NIRSpec_prism NIRSpec_cam MIRI_cam MIRI_spec_lores MIRI_ifu_1A MIRI_ifu_1B MIRI_ifu_2A MIRI_ifu_2B
Num. of positions in dither pattern
Wavelength	NONE	microns			Note: You must also specify a wavelength sampling range in the following section, even if you wish to compute the sensitivity at a single wavelength.
Spectral Resolution	NONE
Aperture Photometry	Optimal	pixels
S/N Ratio
Exposure Time	hours
Wavelength Sampling
Range	to microns
Interval	samples in wavelength log-wavelength steps

*Note: User-supplied filenames should have a .txt extension.

Processing and Reporting Options

 Run in batch mode.

 Report input data as well as results.

The results are based on a data set consisting of values calculated at equally spaced points around an orbit. For each observation, the following report options are available:

 Display the median data set value
 Display the minimum, median and maximum data set values
 Display the minimum and maximum data set values
 Display the entire data set (all time points -- only applicable with single-visit input)

Stray Light model: Finite-element Two-element - for the OTA, sunshield, and background sources. NOTE that the finite-element model may take several hours to complete with the full DRM.

Comment string: (will be included in output file)