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Open Source VLBIVery Long Baseline Interferometry
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FITS Format disclaimer

email: email@example.com
First name: VLBI
Last name: User
Last access: 2021-09-23 13:56:41
2023-11-162023-11-16

WARNING: The workflow chart will not work on Mobile browsers because the drag&drop function does not work. Workflows are then available to be used and saved on Desktop browsers only.

Processing diagram
The flowchart can be used to generate models. The models uploaded or generated in any way are selectable and draggable into the desktop. There also some operators that can work on the models. To use the flowchart just drag and drop the models or operators into its desktop and link them. After saving you can run the workflow to generate a model or more models.
Models:
Operators:
Get model
Copy
Shift
Mask
Stack
Diff
Convolution
DFT
IDFT
Delete item
Name
Save workflow
Your workflows:
name
actions
Your models
name
time updated
Upload picture
upload
Upload new picture
Contexts are correlations of more nodes. You have to enter the celestial coordinates of the object and make sure that all the nodes uploaded were observing the same object. You can work on the observing frequency to change the magnification. Sample rates of all nodes should be the same as entered on this form. After running a context, a new model will be generated.
Your correlations
name
width
height
RA
Dec
frequency
SPS
type
status
Name
Width
Height
Right Ascension
Declination
Frequency
Sample Rate
Type
Actions
A node is a single dish observation in FITS format. To create a node, upload the FITS with observation data and all the needed information by filling the needed keywords. INDIlib radio and detector drivers generate a compatible FITS with this format.
Your observations
name
latitude
longitude
elevation
RA
Dec
frequency
bandwidth
SPS
date
Upload new FITS
upload
Upload new FITS

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