Index

A | B | C | D | E | F | G | I | K | L | M | N | P | R | S | U

A

Accumulate Images
ADI with LOCI
Aggressive destripe assuming there is no signal in the image. (for darks only)
Apply Reference Pixel Correction
Assemble Datacube
Assemble Polarization Cube
Assemble Spectral Datacube
(bp)
Assemble Spectral Datacube using mlens PSF
Assemble Undispersed Image

B

Basic ADI

C

Calibrate astrometry from binary (using 6th orbit catalog)
(using separation and PA)
Calibrate Photometric Flux
Calibrate Photometric Flux - Polarimetry
Calibrate Photometric Flux and save convertion in DB
Calibrate Photometric Flux of extented object
Checks quality of data based on FITS keywords.
Clean Cosmic Rays
Collapse datacube
Combine 2D dark images
Combine 2D images
Combine 2D images and save as Thermal/Sky Background
Combine 3D cubes
Combine Polarization Sequence
Combine Wavelength Calibrations
Combine Wavelength Calibrations locations
Correct GPI distortion
Create a microphonics noise model.
Create Bad Pixel Map from text list of pixels
create Low Frequency Flat 2D

D

Destripe science frame
Display raw data with GPItv
Divide by Polarized Flat Field
Divide by Spectral Flat Field
Divide spectral data by telluric transmission

E

Extract one spectrum via aperture photometry
Extract one spectrum, plots
Extract telluric transmission from datacube
Extract telluric transmission from sat. spots

F

Find Bad pixels from darks or qe map
Find Cold Pixels from a set of Flats
Find Hot Pixels from a set of Darks

G

Generate Combined Bad Pixel Map

I

Interpolate bad pixels in 2D frame
Interpolate Wavelength Axis

K

KLIP algorithm noise reduction

L

Load Instrumental Polarization Calibration
Load Polarimetry Spot Calibration
Load Satellite Spot locations
Load Wavelength Calibration

M

Measure GPI distortion from grid pattern
Measure locations of Emission Lines
Measure Polarization Spot Calibration
(parallelized)
Measure satellite spot flux ratios from unocculted image
Measure satellite spot locations
Measure satellite spot locations with GPItv
Measure satellite spot peak fluxes
Measure telluric transmission
Measure the contrast
Measure Wavelength Calibration
Median ADI data-cubes

N

Noise and Flux Analysis
Normalize polarimetry flats

P

Persistence removal of previous images
Plot the satellite spot locations vs. the expected location from wavelength scaling
Populate Shifts vs Elevation Table

R

Remove Flat Lamp spectrum
Rotate Field of View Square
Rotate North Up

S

Save Output
Set Calibration Type
Shift 2D Image
Simple SSDI
Simple SSDI of median ADI residual
Speckle alignment
Subtract Dark Background
Subtract Thermal/Sky Background if K band

U

Update Spot Shifts for Flexure
Update World Coordinates