Blocks#
A Block is a single unit of processing acting on the Image object, reading and writing its attributes. Blocks documentation include the following information:
read: the
Imageattributes read by theBlockwrite: the
Imageattributes written by theBlockmodify data: indicates that the
Image.datais modified by theBlock
Detection#
Source Extractor detection. |
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DAOPHOT stars detection with |
PSF#
Extract square image cutouts centered on |
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Get median psf from image. |
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Fast empirical FWHM |
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Fit an elliptical 2D Gaussian model to an image effective PSF |
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Fit an elliptical 2D Moffat model to an image effective PSF |
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Fit a symetric 2D Gaussian model to an image effective PSF |
Alignment, Centroiding#
Compute the linear shift between two point clouds. |
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Affine transform computation for images registration |
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Apply an affine transformation to image and/or stars |
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TODO: change name of this. |
Centroiding using |
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Centroiding using |
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Centroiding using |
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Centroiding with ballet. |
Photometry#
Aperture photometry using the |
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Utils#
Flat, Bias and Dark calibration |
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Extract square image cutouts centered on |
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Flip an image according to a reference |
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Stores the last Image |
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A Block that does nothing |
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Save reduced FITS images. |
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Sets specific attribute to every image |
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Build a FITS stack image of the observation |
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Image trimming. |
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All#
Apply an affine transformation to image and/or stars |
|
Compute the linear shift between point clouds using |
|
Centroiding with ballet. |
|
Flat, Bias and Dark calibration |
|
Centroiding using |
|
TODO: change name of this. |
|
Extract square image cutouts centered on |
|
DAOPHOT stars detection with |
|
Fit a symetric 2D Gaussian model to an image effective PSF |
|
Flip an image according to a reference |
|
Fast empirical FWHM |
|
Fit an elliptical 2D Gaussian model to an image effective PSF |
|
Centroiding using |
|
Stores the last Image |
|
Get median psf from image. |
|
Fit an elliptical 2D Moffat model to an image effective PSF |
|
A Block that does nothing |
|
Centroiding using |
|
Save reduced FITS images. |
|
Source Extractor detection. |
|
Sets specific attribute to every image |
|
Build a FITS stack image of the observation |
|
Image trimming. |
|
Affine transform computation for images registration |
|
Write image to FITS file |
|
Compute the linear shift between two point clouds. |