Index

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