Main interface

When launching Siril, the main interface opens.

Note

Click anywhere onto the image below to display its functions.

Main interface

Image area

This area displays the currently loaded image. Click on Red, Green or Blue to switch between the different layers (color images only, a single BW tab is available for mono images).

Right-click on the image to display a contextual menu:

Right-click

Tip

When no image is loaded, double-clicking on the image area pops the Open dialog.

Undo

Undoes the most recent operation.

Redo

Redoes the most recently undone operation.

PSF

Computes a PSF for the current selection and carries out quick photometry.

PSF for the Sequence

Computes a PSF for the current selection for all images in the current sequence.

Pick a Star

Applies star detection to the current selection. The result is opened in the Dynamic PSF dialog. Note this operation is more lenient than the full image star finder routine as it assumes that you have picked a selection containing a star: it can therefore be used to pick stars that have been missed by the full image star finder function.

Selection

Applies constraints to the selection box.

Crop

Provides an interface to the Crop and Crop & rotate functions.

ROI

Provides an interface to set or clear the Region of Interest for ROI processing. Note: this menu entry is not available if the ROI mode is set to "Automatic from selection" in the UI preferences tab.

RGB align

Aligns the image RGB channels. This supports a range of registration methods for alignment:

  • 2-pass global star alignment This uses the 2-pass global star alignment routine with COG framing (so the image dimensions are preserved). This algorithm adjusts with 8 degrees of freedom so it can correct for image shift, rotation and skew. This is the recommended algorithm for images containing stars. This algorithm is global and does not require a selection to be made.

  • KOMBAT alignment This uses the KOMBAT alignment method. It is primarily intended for planetary alignment, but can also work for deep space images. It provides shift registration only, but is fast. This algorithm requires a selection to be made.

  • One star registration This is an older algorithm that provides shift-only registration based on the movement of a single star. This is very fast but the registration cannot cope with as many degrees of freedom as the 2-pass global star alignment. It may be suitable if you are certain you only need to correct for image shift. This algorithm requires a single star to be selected.

  • Image pattern alignment This method performs alignment using the image Fourier transforms. It works for deep space and planetary images but provides only shift registration and is quite slow. This algorithm uses a square selection: a selection must be made, and non-square selections will be corrected to be square.

Warning

The tool is RGB align. It is not intended for, and will not work for, aligning unaligned LRGB compositions. In order to do this you must either align the layers to be composed before composition, or align using the RGB alignment tool.

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Open

Click on these icons (from left to right) to:

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Livestack

Click on this button to start a Livestacking session.

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Undo/Redo

Use these buttons to undo/redo last actions. This is only available if last action has been done through GUI, not by typing a command.

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Image processing

Click on this button to display the Processing menu.

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Tools

Click on this button to display the Tools menu.

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Scripts

Click on this button to display and launch the scripts.

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Information bar

This bar displays the current version of Siril and the path to the current working directory.

  • To the right, informationabout available RAM and disk space id also given.

  • You can change the available number of threads used by Siril using the +/- signs.

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Save

These buttons are used to save your results:

  • save (overwrites) the current image.

  • save with a different name and/or extension.

    starnet dialog

    Save dialog box.

    The drop-down list at the bottom right allows you to choose the type of image recorded. It automatically adds the extension to the file name. However, by staying in the Supported Image Files mode, it is possible to add any extension supported by Siril by hand and it will save in the correct file format.

  • take a snapshot of the current view (as seen on the screen, meaning preview strecthing, if any, is applied). There are two possible options. Either the snapshot is saved in the clipboard, or directly copied to the disk in the working directory.

  • change the bitdepth of the current image. The choice is between 16-bit and 32-bit.

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Burger menu

Opens the main menu, also called burger menu. Gives access to Preferences, the documentation and much more.

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Tabs

Selects one of the tabs. You can also switch between the different tabs using F1 to F7 shortcuts.

More details can be found there:

Tabs

Keys

Conversion

F1

Sequence

F2

Calibration

F3

Registration

F4

Plot

F5

Stacking

F6

Console

F7

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Tab window

Displays the specifics of the currently selected tab.

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Mouse behaviour

Siril uses GTK primary, secondary and middle mouse button mappings. These are usually mapped to left, right and middle (scroll wheel button) physical mouse buttons, however they may be mapped differently in specific setups (e.g. left-handed users may have configured swapped left and right buttons).

  1. Primary mouse button

    The primary mouse button is used for a number of purposes:

    • To select areas of the image

    • With Ctrl pressed (or Cmd on MacOS), to pan the image

    • When the intensity profiling tool is active, to drag the line along which the intensity profile is to be drawn, and to select points corresponding to known wavelengths / wavenumbers in the spectroscopy setting

    • In the RGB composition tool, to select the rotation center when using manual alignment

    • In the gradient removal tool, to draw samples

    • In photometry mode, to perform photometry on a star

    • To select the positions for the registration previews

    • Double clicking the primary mouse button with no image loaded will bring up the Open dialog.

  2. Secondary mouse button

    The secondary mouse button is used for a number of purposes:

    • To bring up the image context menu (except when in photometry mode)

    • In the gradient removal tool, to remove samples

    • In photometry mode, to perform photometry on the selected star for all frames of the currently loaded sequence (if no sequence is loaded, this has no effect)

  3. Middle mouse button

    The middle mouse button is used for the following purposes:

    • To pan the image at the current zoom level

    • With Ctrl pressed (or Cmd on MacOS), to make a square selection suitably sized for photometry

    • Double clicking adjusts the zoom level to a preset value. The behaviour is configurable in the User Interface tab in the Preferences dialog. The choices are: - Always zoom to fit - Always zoom to 100% centered on the mouse cursor - Toggle between zoom to fit and zoom to 100% centered on the mouse cursor

  4. Scroll wheel

    • The scroll wheel is used to adjust the zoom level.

Command line

Type in a command and press Enter.

  • You can press the button at the end of the line to get some help on the usage.

  • You can also abort the process being currently executed by clicking on the Stop button.

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Expand

Click on this bar to expand/retract the whole tab/tab window area.

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Image sliders

Use the top and bottom sliders to adjust the white and black points of the previewed image (in Linear mode).

Tip

Click on the name of the Image or Sequence loaded to copy its name to the clipboard (useful to paste in a command).

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Preview mode

Select the preview mode for the loaded image, between the following choices:

  • Linear

  • Logarithm

  • Square root

  • Squared

  • Asinh

  • Autostretch (tick the High Definition box to use a deeper (up to 24-bit, configurable in Preferences) LUT instead of the default 16-bit one)

  • Histogram

In Autostretch mode with color images, the toggle to the right activates/deactivates channel linking. When unlinked, the 3 layers are stretched independantly so as to give a more balanced image.

Warning

This is just a preview of the image, not the actual data (except if Linear mode is selected). Do not forget to stretch your images before saving them.

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Special views

Use these toggles to show previewed images:

  • in inverted colors

  • in false colors

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Astrometry tools

Use these toggles to show:

Warning

The loaded image needs to be plate-solved for these buttons to be active.

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Quick photometry

Use this toggle to trigger the quick photometry mode.

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Intensity profile

Use this toggle to trigger the intensity profile mode.

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Zoom

Use these buttons to:

  • Zoom out

  • Zoom in

  • Zoom to fit the avaialble window space

  • Zoom to actual size

Tip

Ctrl+left clic will allow to navigate into the picture

Tip

Ctrl+mouse scroll will zoom in/out and Ctrl + 0 / 1 will zoom to fit/100%.

Tip

Ctrl+Shift and drag with the primary mouse button will measure the distance between two points. If sufficient metadata is available the measurement will be given in degrees, minutes and arcseconds, otherwise it will be given in pixels.

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Geometric transformations

Use these buttons to:

  • Rotate left

  • Rotate right

  • Mirror about horizontal axis

  • Mirror about vertical axis

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Frame selection

Click on this button to open the frame selector.

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