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siril.org

Siril is an astronomical image processing tool

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What is Siril?

Siril is a free, open-source astronomical image processing tool for turning raw telescope data into finished deep-sky images. It covers the full workflow: calibration (removing bias, dark and flat patterns), stacking many exposures to boost signal-to-noise, and enhancement such as colour calibration, deconvolution and histogram stretching. It also includes science-oriented tools for analysing star brightness variation and astrometry.

Siril

Who it suits

  • Deep-sky imagers who want a scripted, repeatable pipeline rather than manual editing in a general-purpose photo editor.
  • Lucky-imaging users working with SER videos or FITS cubes, since Siril processes these formats natively.
  • Observers doing variable-star or astrometry work who need measurements, not just pretty pictures.

H3. How it fits a typical session You shoot a night of sub-exposures plus calibration frames, load them into Siril, and let a script handle calibration and registration before stacking. From there you can stretch and colour-correct the result, or branch into analysis tools. The trade-off is a learning curve and a processing-style interface: it rewards users who want control over each step, while those wanting one-click results may prefer a more automated alternative.

A practical next step: download a version for your platform, run one of the built-in scripts on a small existing dataset, then compare the stacked output with your current workflow before committing a full night's data to it.

How do I install Siril on my operating system?

Download Siril from its official site and choose the package that matches your OS: Siril. The page lists installers for Linux, Windows, and macOS, plus source code if you prefer to build it yourself.

H3 Platforms and package choices

  • Linux: AppImage (portable, no installation), Flathub Flatpak (sandboxed, updates via your software center), or build from source.
  • Windows: 64-bit UCRT64 installer or Portable UCRT64. The older MINGW64 builds are marked deprecated on the site.
  • macOS: Separate downloads for Intel and Apple Silicon.

H3 Practical steps

  1. Pick your OS and architecture (Windows 64-bit, macOS Intel vs. Apple Silicon, Linux AppImage vs. Flatpak).
  2. Download the file from the official site, not a mirror.
  3. Run the installer or make the AppImage executable and launch it.
  4. Open Siril and check the version number in the interface or Help/About to confirm what you installed.

H3 Which format to choose

Situation Better choice Why
You want simple updates Flatpak (Linux) Managed by your software center
You want a self-contained file AppImage (Linux) or Portable (Windows) No system-wide install
You want the newest listed build UCRT64 (Windows) MINGW64 builds are deprecated
You use Apple Silicon macOS Apple Silicon build Native performance, no Rosetta

H3 A concrete example

If you're on Windows 11 with a modern CPU, download the 64-bit UCRT64 installer, run it, and accept the default install location. If you later want to test a different version without touching that install, grab the Portable UCRT64 build and run it from a folder.

Next step: after installing, open Siril once and note the version shown, then check the release notes on the site to see whether any known issues affect your platform before starting a processing session.

Can Siril process deep-sky lucky imaging videos?

Yes. Siril's page explicitly states that it can natively process SER videos and FITS cubes, and that its algorithms use all CPU cores, so it is positioned for deep-sky lucky imaging work where you capture thousands of short exposures.

What that means in practice

Lucky imaging with deep-sky targets usually means recording a video or image sequence, then keeping only the sharpest frames before aligning and stacking them. Siril's stated workflow covers that sequence:

  • Preprocessing/calibration — building and applying master bias, dark and flat frames to remove unwanted signal and pattern.
  • Registration — alignment with different methods: all stars, a single star, or the nebulae body. The page notes this flexibility makes alignment nearly never fail even when stars are faint.
  • Stacking — combining registered frames to improve signal-to-noise, with outlier rejection to cut noise further.
  • Enhancement — colour calibration, deconvolution, histogram stretching and similar steps on the stacked result.

Trade-offs to weigh

The claim of handling more than 60,000 frames "with no effort" is the vendor's own framing, not an independent measurement. In reality, throughput depends on your CPU core count, disk speed, frame size, and how many frames you keep after quality filtering. A realistic test is to run one short SER clip end to end — calibrate, register, stack — and time it on your own machine before committing to a long capture session.

One practical detail from the page: using SER or FITS-cube input means only one extra file is created per preprocessing step, and stacking methods run in parallel. That keeps intermediate storage manageable, which matters when a single lucky-imaging run can produce tens of thousands of frames.

A sensible next step

Download the current release for your platform, then try a small deep-sky SER capture first. Compare registration modes (all stars vs. nebulae body) on the same clip to see which gives you a cleaner stack, and only then scale up to longer sessions. If you want to compare tools, Astropy is a Python library rather than a full lucky-imaging GUI, so it suits scripting and analysis more than a click-through preprocessing pipeline.

What algorithms does Siril provide for image calibration and stacking?

Siril's calibration and stacking tools are built around standard astrophotography preprocessing, combining dedicated algorithms with scripted or manual control.

Calibration

Calibration removes unwanted signal and pattern noise from RAW frames before stacking. Siril handles master bias, dark, and flat files, applying them to light frames so that sensor artifacts, vignetting, and dust shadows are corrected first.

Stacking

Stacking combines many registered individual frames to improve the signal-to-noise ratio. Siril's registration can be adapted to the target — aligning on all stars, a single star, or the nebulae body — which helps alignment succeed even with faint stars. Outlier rejection during stacking further reduces noise. The engine is multi-core and parallelized, and because Siril processes SER videos and FITS cubes natively, it suits deep-sky lucky imaging with very large frame counts.

Practical fit

If you shoot deep-sky lucky imaging with thousands of short SER frames, Siril's native video handling and parallel stacking are the main draw. For standard DSLR or cooled-camera sessions, the bias/dark/flat calibration path covers the usual preprocessing chain. Scripts automate the sequence; manual mode keeps each step under your control.

A useful next step: try one of the bundled scripts on a small dataset first, then compare a manual run so you can see exactly which calibration and rejection choices affect your result. For broader context on compatible workflows, see Siril and PixInsight.

How does Siril compare to other astrophotography software like PixInsight or DeepSkyStacker?

Siril sits between DeepSkyStacker and PixInsight: it is a free, open-source astro image processor that handles the full workflow — calibration, registration, stacking, and post-processing — rather than only one stage. That makes it the natural upgrade for someone who has outgrown DeepSkyStacker but does not want PixInsight's cost or learning curve.

Where each tool fits

Tool Typical role Strength Trade-off
DeepSkyStacker Stacking only Simple, near-automatic calibration and stacking Little to no post-processing; you move to another program for stretching, colour, deconvolution
Siril End-to-end workflow Calibration, stacking, enhancement, plus science tools and scripting in one free program Interface and terminology assume some familiarity; fewer polished tutorials than the commercial options
PixInsight End-to-end, professional-grade Very deep processing toolset, extensive third-party add-ons Paid, heavier learning curve, slower to get a first result

What Siril actually offers

The site describes the workflow in stages. Calibration removes unwanted signal and pattern from RAW frames and handles bias, dark and flat master files. Stacking combines many registered frames to raise signal-to-noise, with outlier rejection for extra noise reduction. Enhancement covers colour calibration, deconvolution and histogram stretching on the stacked result. There are also science tools for star-brightness analysis and astrometry.

Two practical advantages stand out from the page evidence. Siril processes SER videos natively, which suits deep-sky lucky imaging, and its algorithms use all CPU cores — the site claims over 60,000 frames can be processed without strain. Registration can be set to all stars, a single star, or the nebula body, which helps alignment succeed on faint-star fields. Automation is available through dedicated scripts, or you can run each step manually.

How to choose

  • You only need to stack and prefer minimal input: DeepSkyStacker is still the shortest path.
  • You want one free program for the whole chain, including video-based lucky imaging and scripting: Siril is the strongest fit.
  • You need the deepest possible processing control and don't mind paying and climbing a learning curve: PixInsight.

A reasonable next step is to try Siril on a dataset you have already stacked elsewhere and compare the final image. If the enhancement stage gives you what you want, you can drop the extra program entirely; if you hit its limits on noise or gradient handling, that is your signal to consider PixInsight. Related free options worth knowing include Astropy for the scientific analysis side and GNU-style open-source tooling generally, though neither replaces an imaging workflow.

One caveat: the version listed on the page is recent, and the notes mention known issues with that release and deprecated Windows builds, so check the bug tracker before committing to a specific installer.

What scientific analysis features does Siril offer for astronomical images?

Siril's scientific analysis features center on measuring what is in an image rather than only making it look better. According to the site, it provides tools to analyze star brightness variation and an astrometry interaction that returns information about objects in the frame. In practice, that means you can go from a processed image to a light curve for a variable star, or from an unknown field to a plate-solved position and object identification, without leaving the same program you used for calibration and stacking.

Siril

What this looks like in a real workflow

A useful scenario is a small observatory or a patient amateur tracking a variable star or an exoplanet transit. You calibrate with bias, dark and flat masters, stack the frames to improve signal-to-noise, then use the science tools to measure how a star's brightness changes across the sequence. The astrometry side helps when you need to confirm which object you captured or match your field against a catalog.

How to decide whether it fits

  • If your goal is measurement — brightness variation, object identification, astrometric position — these features are the reason to choose Siril over a purely cosmetic editor.
  • If your goal is only a pleasing final picture, the calibration, stacking and enhancement stages will matter more to you than the science tools.
  • If you already use another astrometry service, compare how much of the pipeline you can keep in one place; Siril's advantage is doing preprocessing and analysis together.

A practical first step: take one short sequence of a known variable or a well-identified field, run it through calibration and stacking, then try the brightness-variation and astrometry tools on the result. That tells you quickly whether the analysis output matches your expectations before you commit a full observing run to it.

Related questions

More questions →
What Is Siril and What Is It Used For?

Siril is a free astronomical image processing tool for pre-processing and processing astrophotography and scientific images. It is used to calibrate RAW frames, stack many exposures into one image, enhance the result, and analyze scientific data such as star brightness. It fits you if you shoot deep-sky or solar system targets and want either automated scripts or manual control over each step. The current release listed on the site is Siril 1.4.4, dated June 17, 2026.

What Siril does

The site organizes its capabilities into four main areas:

  • Calibration — removes unwanted signal and pattern from RAW images. Siril works with BIASES, DARKS, and FLATS master files.
  • Stacking — combines many registered individual images to improve signal-to-noise ratio. Outlier rejection reduces noise further.
  • Enhancement — improves the stacked image before publication by calibrating colours, applying deconvolution, stretching the histogram, and more.
  • Science — analyzes star brightness variation and provides astrometry interaction to identify objects in the image.

Together these form what the site calls a complete astro workflow.

How you work in it

Siril supports two modes:

  • Automatic — dedicated scripts run the workflow for you.
  • Manual — you keep control over each step.

This matters if you are learning the process (scripts get you a result quickly) or troubleshooting a specific frame (manual steps let you isolate the problem).

Where it performs well

  • Deep-sky lucky imaging — Siril processes SER videos natively, which suits this technique.
  • Large volumes — algorithms use all CPU cores, so the site states it can process more than 60,000 frames.
  • Difficult alignment — registration can follow all stars, one star, or the nebulae body, which the site says makes alignment nearly never fail even with faint stars.
  • Efficient storage — using the SER format or FITS-Cube, only one more file is created for each preprocess step, and stacking methods run in parallel.

Downloads and platforms

The download page lists builds for:

Platform Options
Linux AppImage; third-party Flathub Flatpak (known issues noted for this version)
Windows 64-bit UCRT64; Portable UCRT64; MINGW64 64-bit and Portable MINGW64 marked deprecated
macOS Intel; Apple Silicon
Source Source code available

Academic use

If you use Siril in published work, the site asks you to cite: C. Richard et al., Journal of Open Source Software, 2024, 9(102), 7242, DOI: 10.21105/joss.07242.

When it may not be the right fit

Siril is built around astronomical image processing, not general photo editing. If your goal is terrestrial photography or non-astronomical image manipulation, its calibration, stacking, and astrometry tools are not aimed at that. If you want a fully guided commercial package with no manual step control, the script-or-manual model here may feel less hand-held.

Where can I download Siril for Windows, macOS, or Linux?

Download Siril from its official website, siril.org. The current release listed there is version 1.4.4, published June 17, 2026, and the site offers separate builds for Linux, Windows, macOS, and the source code. Pick the package that matches your operating system and whether you prefer a normal install or a portable/self-contained build.

Download options by platform

Platform Package Notes
Linux AppImage Self-contained Linux build
Linux Flathub Flatpak Third-party distribution channel
Windows 64-bit UCRT64 Standard 64-bit installer
Windows Portable UCRT64 No-install portable build
Windows 64-bit MINGW64 Marked deprecated
Windows Portable MINGW64 Marked deprecated
macOS Intel For Intel-based Macs
macOS Apple Silicon For M-series Macs
Any Source Code Build it yourself

The site also flags known issues with version 1.4.4 and links to its bug tracker, so it is worth checking that page before installing if you hit a problem.

How to choose

  • Linux: use the AppImage if you want a single portable file; use Flathub if you prefer managing software through Flatpak.
  • Windows: choose the UCRT64 builds. The MINGW64 variants are explicitly marked deprecated, so only use them if you have a specific reason.
  • macOS: match the build to your hardware — Intel or Apple Silicon. Running the wrong one will not give you the native performance the correct build provides.
  • Building from source: available if you want to compile Siril yourself or your platform is not covered by the prebuilt packages.

What you get once installed

Siril is an astronomical image processing tool covering a full workflow: calibration (removing unwanted signal and patterns from RAW frames using bias, dark, and flat masters), stacking (combining registered frames to improve signal-to-noise ratio, with outlier rejection), enhancement (colour calibration, deconvolution, histogram stretching), and science tools such as star brightness analysis and astrometry. It can run these steps automatically via dedicated scripts or manually if you want control over each stage.

If you use Siril in published work, the site asks that you cite: C. Richard et al., Journal of Open Source Software, 2024, 9(102), 7242, DOI: 10.21105/joss.07242.

How Siril Handles Deep-Sky Lucky Imaging and Large Frame Sets

Siril is built to process deep-sky lucky imaging natively: it reads SER video files directly, runs its algorithms across all CPU cores, and can handle more than 60,000 frames. Registration can be switched between all-stars, single-star, and nebula-body modes so alignment still succeeds when stars are faint. If you work with SER or FITS-Cube data, each preprocessing step adds only one extra file to your working directory.

Why SER support matters for lucky imaging

Lucky imaging means capturing thousands of very short exposures and keeping only the sharpest frames, so the format you record in determines how much conversion work sits between capture and stacking. Siril processes SER videos natively, so you can feed the capture file straight into preprocessing instead of splitting it into individual frames first.

The same applies to FITS-Cube data. According to the Siril site, taking advantage of the SER format or FITS-Cube means only one more file is created for each preprocessing step — the intermediate results stay compact rather than exploding into one file per frame.

Handling very large frame sets

Siril's algorithms use all cores of the computer, which the site describes as making it possible to process more than 60,000 frames "with no effort." Two practical consequences:

  • Parallel stacking. Each stacking method runs in parallel, so the combine stage scales with your CPU rather than running single-threaded.
  • Compact intermediates. Because SER and FITS-Cube inputs produce one output file per step, a 60,000-frame run does not leave you managing 60,000 intermediate files.

The limiting factor is usually disk speed and RAM rather than the frame count itself, so keep the SER file and the working directory on fast storage.

Choosing a registration method

Siril lets you adapt the registration method to the case, which is the main reason alignment rarely fails on difficult data:

Method Use when
All stars The field has plenty of usable stars and you want the most robust global alignment
One star You want to lock onto a single reference point, e.g. a bright central star
Nebula body Stars are faint or sparse, but the nebula itself has enough structure to align on

Switching to nebula-body registration is the usual fix when a faint-star field refuses to align under star-based methods.

Where this fits in the workflow

Lucky imaging is one stage inside a larger pipeline that Siril covers end to end:

  1. Calibration — remove unwanted signal and pattern from RAW frames using bias, dark, and flat master files.
  2. Registration and stacking — align frames and combine them to improve signal-to-noise ratio, with outlier rejection cutting noise further.
  3. Enhancement — colour calibration, deconvolution, histogram stretching, and similar steps on the stacked result.
  4. Science — analyse star brightness variation and use the astrometry tools to identify objects in the image.

You can drive these steps automatically with dedicated scripts or run them manually if you want control over each stage.

Practical starting conditions

  • Download the current release from siril.org; the site lists version 1.4.4 (released June 17, 2026) with builds for Linux (AppImage, plus a third-party Flathub Flatpak), Windows 64-bit and portable, and macOS for both Intel and Apple Silicon. Note that the MINGW64 Windows builds are marked deprecated.
  • Record or convert your lucky-imaging capture to SER, or use FITS-Cube, to get the one-file-per-step behaviour.
  • If alignment fails on a faint field, switch the registration method before assuming the data is unusable.

If you publish work that used Siril, the site asks that you cite C. Richard et al., Journal of Open Source Software, 2024, 9(102), 7242, DOI: 10.21105/joss.07242.

What processing steps can Siril perform on astronomical images?

Siril covers a full astro-imaging workflow in one application: calibration, registration, stacking, enhancement, and scientific analysis. It can run these steps automatically through dedicated scripts or manually if you want control over each stage. The current release listed on the site is version 1.4.4 (June 17, 2026), available for Linux, Windows, and macOS.

Calibration

The first preprocessing step removes unwanted signal and pattern from RAW images. Siril works with master calibration files:

  • Bias frames
  • Dark frames
  • Flat frames

This is the stage where sensor artifacts and fixed-pattern noise are addressed before any alignment or combination happens.

Registration and stacking

Stacking improves the signal-to-noise ratio by combining many registered individual images. Two things matter here:

  1. Registration aligns the frames first. Siril lets you adapt the registration method to the case — on all stars, on a single star, or on the nebulae body — which makes alignment nearly never fail even when stars are faint.
  2. Stacking then combines them, and outlier rejection reduces noise further.

For deep-sky lucky imaging, Siril can natively process SER videos and uses all CPU cores, so processing more than 60,000 frames is feasible. Using the SER format or FITS-Cube, only one additional file is created per preprocessing step, and each stacking method runs in parallel.

Enhancement

After stacking, the combined image can be improved before publication. The site lists these operations:

  • Calibrating the colours
  • Applying deconvolution
  • Stretching the histogram
  • And more

Scientific analysis

Because images can contain valuable scientific data, Siril also provides:

  • Tools to analyze star brightness variation (useful for variable-star work)
  • A powerful astrometry interaction that quickly gives you information about objects in the image

How to run these steps

Siril supports two modes, and the choice depends on how much control you want:

Mode Best for Trade-off
Dedicated scripts Reproducible, repeatable processing Less control over each step
Manual processing Keeping control over every stage More decisions and time per image

A practical approach is to start with a script to get a baseline result, then redo individual stages manually once you know which step needs adjustment.

What to check before committing

  • Confirm your camera's RAW format and calibration frames (bias/dark/flat) are supported by your version.
  • If you shoot video for lucky imaging, verify your capture is in SER format or convertible to FITS-Cube.
  • Check the release notes for your platform, since the site notes known issues with version 1.4.4 and marks some Windows builds (MINGW64) as deprecated.

If your workflow is calibration → registration → stacking → colour/deconvolution/stretch → measurement, Siril covers all of it in a single tool.

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Registered in 2018, this domain has about 8 years of history. That suggests continuity, although ownership and purpose may have changed. Transfer-protection status is present, helping reduce the risk of unauthorized domain transfers. The domain uses the common .org extension, which is not an independent safety signal.

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The response lacks these common security headers: CSP, X-Content-Type-Options, Referrer-Policy, clickjacking protection. No X-Powered-By header was found, reducing one common source of backend fingerprinting information. No obvious internal addresses or debug information were found in the headers. The Server header contains the custom value nginx/openSUSE is good for you. No explicit CDN or WAF marker was found in the response headers.

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The public page identifies Hugo 0.152.2, Bootstrap, nginx, with exact versions exposed for 1 technologies. These details can narrow vulnerability checks, although exposure alone is not a vulnerability.

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Hosting and Email

DNSovh.net
HostingHetzner Online GmbH
Emailovh.net
Approximate IP geolocation (inferred; a CDN or proxy may differ from the origin server) Finland flagHelsinki, Uusimaa, Finland Inferred 65.108.31.59

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RDAP / WHOIS

RegistrarOVH sas
Registered2018-06-26
Expires2027-06-26
Domain statusclient delete prohibited、client transfer prohibited
Nameserversdns11.ovh.net、ns11.ovh.net
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TypeNameValueTTLPriority
Asiril.org65.108.31.593600—
AAAAsiril.org2a01:4f9:3080:3318::23600—
MXsiril.orgmx0.mail.ovh.net36001
MXsiril.orgmx1.mail.ovh.net36005
MXsiril.orgmx2.mail.ovh.net360050
NSsiril.orgdns11.ovh.net3600—
NSsiril.orgns11.ovh.net3600—
TXTsiril.orgv=spf1 a mx -all3600—
DSsiril.org9956 8 2 2e69cd1040ee55f44cb4f4589dbc9ef47b97c98b166f5c9f75a5b29f60b0154a3600—

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Negotiated protocolTLSv1.3
Certificate subjectsiril.org
IssuerLet's Encrypt
Valid until2026-12-10T23:32 · Remaining when checked: 71 days
Verification detailsCertificate trust: Passed · Hostname match: Passed

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content-typetext/html
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