Index

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

Symbols

2D Wavelength Solution

A

Accumulate Images
ADI with LOCI
Advanced KLIP ADI for Pol Mode
Apply Reference Pixel Correction
Assemble Polarization Cube
Assemble Spectral Datacube
(bp)
Assemble Undispersed Image

B

Basic ADI

C

Calibrate astrometry from binary (using 6th orbit catalog)
(using separation and PA)
Calibrate Photometric Flux
Check Data Quality
Check for closed-loop coronagraphic image
Clean Cosmic Rays
Clean Polarization Pairs via Double Difference
Collapse datacube
Combine 2D dark images
Combine 2D images
Combine 2D Thermal/Sky Backgrounds
Combine 3D Datacubes
Combine Polarization Sequence
Combine Polarization Sequence via Double Difference
Combine Wavelength Calibrations
Combine Wavelength Calibrations locations
Correct Distortion
Create 2D Low Frequency Flat
Create Lenslet Flat Field
Create microphonics noise model
Creates a thermal/sky background datacube

D

Destripe for Darks Only
Destripe science image
Display raw image with GPItv
Divide by Lenslet Flat Field
Divide by Polarized Flat Field
Divide by Spectral Flat Field

E

Extract 1D spectrum from a datacube
Extract one spectrum, plots

F

Find Cold Bad Pixels from Flats
Find Hot Bad Pixels from Darks
Flag Quicklook

G

Generate Combined Bad Pixel Map

I

Insert Planet into datacube
Interpolate bad pixels in 2D frame
Interpolate bad pixels in cube
Interpolate Wavelength Axis

K

KLIP ADI for Pol Mode
KLIP algorithm Angular Differential Imaging
KLIP algorithm Angular Differential Imaging With Center Forced
KLIP algorithm Spectral Differential Imaging

L

Load Instrumental Polarization Calibration
Load Polarimetry Spot Calibration
Load Wavelength Calibration

M

Measure Contrast
Measure GPI distortion from grid pattern
Measure Polarization Spot Calibration
Measure satellite spot locations
Measure satellite spot peak fluxes
Measure Star Position for Polarimetry
Measure Wavelength Calibration
Median Combine ADI datacubes

N

Noise and Flux Analysis
Normalize polarimetry flat field

P

Pad Wavelength Calibration Edges
Plot the satellite spot locations vs. the expected location from wavelength scaling
Populate Flexure Shifts vs Elevation Table

Q

Quality Check Wavelength Calibration
Quick Wavelength Solution Update

R

Remove Flat Lamp spectrum
Remove Persistence from Previous Images
Rotate Field of View Square
Rotate North Up

S

Save Output
Simple SDI of post ADI residual
Simple Spectral Differential Imaging
Smooth a 3D Cube
Speckle alignment
Stores calibration in dataset
Subtract Dark Background
Subtract Mean Stellar Polarization
Subtract Thermal/Sky Background Cube if K band
Subtract Thermal/Sky Background if K band

U

Update Spot Shifts for Flexure
Update World Coordinates