pynrc.nrc_utils

pyNRC utility functions

Functions

bias_dark_high_temp(darks_80K_dir[, T, sca])	Extrapolate a bias and dark at some temperature
channel_select(bp)	Select wavelength channel
dark_ramp_80K(darks_80K_dir[, sca])	Return dark ramp over time
do_charge_migration(image[, satmax, niter, ...])	Migration of charge from saturated pixels to immediate neighbors
do_fft(a[, n, axis, norm, inverse, real, ...])	Perform FFT using either numpy or MKL FFT
gen_unconvolved_point_source_image(nrc, ...)	Create an unconvolved image with sub-pixel shifts
grism_background(filter[, pupil, module, ...])	Returns a 1D array of grism Zodiacal/thermal background emission model, including roll-off from pick-off mirror (POM) edges.
grism_background_com(filter[, pupil, ...])
grism_background_image(filter[, pupil, ...])	Create full grism background image
make_grism_slope(nrc, src_tbl, tel_pointing, ...)	Create grism slope image Parameters
nproc_use_convolve(fov_pix, oversample[, npsf])	Attempt to estimate a reasonable number of processes to use for multiple simultaneous convolve_fft calculations.
offset_bar(filt, mask)	Bar mask offset locations
pickoff_image(ap_obs, v2_obj, v3_obj, flux_obj)	Create an unconvolved image of filled pixel values that have been shifted via bilinear interpolation.
pickoff_xy(ap_obs_name)	Return pickoff mirror FoV x/y limits in terms of science pixel coordinates
pix_noise([ngroup, nf, nd2, tf, rn, ktc, ...])	Noise per pixel
place_grism_spec(nrc, sp, xpix, ypix[, ...])	Create spectral image and place ref wavelenght at (x,y) location
place_grismr_tso(waves, imarr, siaf_ap[, ...])	Shift image such that undeviated wavelength sits at the SIAF aperture reference location.
segment_pupil_opd(hdu, segment_name[, npix])	Extract single segment pupil from input full OPD map
var_ex_model(ng, nf, params)	Variance Excess Model
zodi_euclid(locstr, year, day[, ...])	IPAC Euclid Background Model
zodi_spec([zfact, ra, dec, thisday])	Zodiacal light spectrum.