Index

A | B | C | D | E | F | G | H | I | L | M | N | O | P | R | S | T | W | Z

A

Absolute photometry
Direct approach (using field sources)
Indirect approach (using standard stars)
Selected individual images (direct approach)
Airglow
Animate images
Astrometry
Method: Scamp
Reference catalogs

B

B-V color calibration
Background
Create the illumination correction image
Superflat
Background model
Additive or multiplicative?
Superflat; Static background model
Background modelling (near-IR)
1-pass
Iterative; 2-pass
Bad columns
Bias frames
Dark frames
Binaries (executables)
Binned mosaics
Blank fields
Blooming
Masking blooming spikes
Removing blooming spikes

C

Celestial type
Check-plots
Chop-nod sky subtraction
Co-averaging
Coaddition
Blending overlap regions
Celestial types
Choosing the output pixel scale
Masked stellar cores
Moving targets
Outlier rejection
Projection types
Reference coordinates
Resampling kernels
Collapse correction
Color calibration
Color images
Background estimation
Color calibration
FITS to TIFF conversion
Narrow-band combination
Synthetic luminance channel
Combining a set of images
Configuration files
Cosmics
Cross-talk

D

Dark frames
Rescaling with exposure time
Data organisation
Defect detection
Directory tree
Dithering
Reasons for dithering
Downloading THELI

E

Empty fields
Executables
Extinction correction (relative)

F

FITS header
FITS header correction
Flat-fields
Flux calibration
Fringing
Airglow
Create a fringe model

G

Global weights
Gradient correction (horizontal or vertical)

H

Headers
Hot pixels

I

Image analysis
Image coaddition
Image combination
Image defects
Image preview
Image statistics
Imalyzer
Infrared
Initialising THELI
Installation
Graphical user interface
Pipeline core
Pre-requisites
Updating THELI
Instruments
Configuration files (storage place)
Define a new instrument
Pre-configured near-infrared cameras
Pre-configured optical cameras
Splitting script

L

Linked file system
Create links
Resolve links
LOG file
Location
Low surface brightness targets

M

Masking
Cosmics
Hot pixels
Image defects (automatic)
Image defects (manual)
Non-linear pixels
Satellites
Stellar cores
Mid-infrared
Moving targets
Multi-chip cameras
Processing of individual chips
Multi-color data sets
Astrometry
Coaddition
Data organisation
Efficient processing
Same image size for all coadded images

N

Near-IR
Background modelling
Co-averaging
Reset anomaly
Non-linearity
Correction
Masking non-linear pixels

O

Object catalogs
Observing
Dithering
Low surface brightness targets
Planning
Standard stars
OFC (in file names)
Overscan correction

P

Parallelisation
Parallel manager
Photometric color calibration (PCC method)
Photometry
Absolute (flux calibration)
Relative (atmospheric extinction correction)
Pre-processing
Preview images
Processing status
Projections
Proper motion targets
PSF analysis

R

Raw data
Header correction
Sorting file types
Splitting
Reference catalog
astrometric
astrometric: available catalogs
photometric
Relative photometry
Resampling kernels
Reset anomaly
Correction

S

Satellite masking
Scamp
Interpreting check-plots
Scripts
SKY fields
Sky projections
Sky subtraction
Background modelling
Extended targets
Splitting raw data
Stacking images
Standard star selection
Status
Status string ("OFC" etc ...)
Superflat
Dithering
Dynamic background model
Swapping
Synthetic luminance

T

Temporary files
Choose different storage place
Transparency correction (relative)

W

Weighting
Cosmic and hot pixel detection
Global weights
Individual weight maps
Masked stellar cores
Supressing non-linear pixels

Z

Zeropoint determination
For individual exposures (using field sources)
Using field sources
Using standard stars