VLT Instrument Pipelines
Jan 12, 2018: EFOSC pipeline version 2.3.0 released!
The EFSOC 2.3.0 release includes basic support for Reflex workflows.
Dec 22, 2017: SPHERE pipeline version 0.31.0 released!
The SPHERE 0.31.0 release fixes issues with the IFS wavelength calibration, the IRDIS and ZIMPOL zero-points and the ZIMPOL Strehl ratio along with a number of technical issues with the pipeline.
Nov 16, 2017: GRAVITY pipeline version 1.0.11 released!
The GRAVITY 1.0.11 release supports the new DPR keywords of the GRAVITY raw data and a number of other improvements and fixes.
Oct 19, 2017: UVES, UVES-FIBRE, X-shooter pipelines documentation updated!
Updated pipeline and reflex user manuals of UVES, UVES_FIBRE and X-shooter pipelines to clarify some sections and fix some typos.
Oct 4, 2017: MUSE pipeline version 2.2 released!
The MUSE 2.2 release provides initial support for WFM-AO observations, and a number of other improvements and fixes.
Jul 14, 2017: MUSE pipeline version 2.0.3 released!
The MUSE 2.0.3 release is a maintenance release which fixes a backwards compatibility issue when using an old-style standard response as input for .
Jul 3, 2017: X-shooter pipeline version 2.9.3 released!
The X-shooter 2.9.3 release fixes portability problems to Mac OS.
Jun 2, 2017: X-shooter pipeline version 2.9.1 released!
The X-shooter 2.9.1 release fixes a bug in the reflex oca rules that was preventing reduction of X-shooter offset NIR data.
May 15, 2017: SOFI pipeline version 1.5.8 released!
The SOFI 1.5.8 release offers improvements in supported platforms and fixes an issue that prevents product creation for some of its recipes.
For the start of period 99 updated versions of all Instrument Pipeline Packages are now available.
- For the installation of RPM packages (Fedora 20 to 25, Scientific Linux 7) continue here
- For the installation of MacPorts packages (OS X 10.9 to 10.12) continue here
- For the source kit installation go here
To get announcements of new pipeline releases, send an email to email@example.com.
- Install the pipeline(s) using RPM packages, MacPorts packages or Source Kits.
- Detailed usage information can be found in the individual user manuals and tutorials available here
Three Ways to Run a Pipeline
- Reflex is the recommended environment to reduce ESO data. It automatically organizes input files according to their category and runs the entire reduction chain at the push of a button. It supports break points in the reduction sequence in order to inspect and interact with intermediate and final products and rerun the corresponding step if necessary.
- Gasgano is a Java-based data file organizer developed and maintained by ESO. It can be used to manage and organize in a systematic way the astronomical data observed and produced by all VLT compliant telescopes. Gasgano is a graphics-based software tool for organising and viewing data files produced by the VLT Control System. Gasgano offers functionalities for data viewing, grouping, sorting, classification, searching, and filtering of data. And, of course, Gasgano will run any requested CPL recipe on the selected data.
- Esorex, a command-line utility for running pipeline recipes is also available. It may be embedded by users at their home institute into data reduction scripts for the automation of processing tasks.
The underlying algorithms and recipes are the same for a given instrument pipeline, irrespective if Reflex, Gasgano or Esorex is used.
Fedora Linux, Scientific Linux and macOS
Currently ESO provides binary packages for:
- Fedora Linux (20 to 25)
- Scientific Linux 7
- macOS (10.9 to 10.12)
Please follow the installation instructions for RPM packages or MacPorts packages.
Source Kit package installation
Users of operating systems for which no RPM or MacPorts packages are currently available should follow the instructions in this section.
Please consult the Software Prerequisites page before installing the pipelines or Reflex from source.
Installations without Reflex
If you want to install pipeline packages without Reflex support please follow the instruction in this section. It applies to all pipeline packages.
- Download the desired pipeline kit(s) from the Source Kit column in the table below into an empty, temporary directory.
- Download the Source Kit installer into the same directory.
- If necessary, make it executable:
- Execute the command:
- After the installation the temporary directory with its contents can be deleted.
Reflex based Pipeline Installations
For an installation of pipeline packages with Reflex support please follow the instructions in this section.
- Download the install_esoreflex script.
Important: As of June 2017 there is a new version of the script. Please make sure you use that one.
- If necessary, make it executable:
- Execute the command and follow the instructions:
- If you make use of any of these workflows in a scientific publication, please consider citing Reflex. You may reference the following paper: Automated Data Reduction Workflows for Astronomy: The ESO Reflex Environment, 2013, Freudling, W., et al., Astron.Astrophys., 559, A96 (Bibtex entry)
Instrument Pipeline Packages
Table rows marked with a blue background indicate Reflex workflow availability.
Сьюзан рассеянно кивнула, но тут же вспомнила, как Танкадо отдал им Северную Дакоту. Она вглядывалась в группы из четырех знаков, допуская, что Танкадо играет с ними в кошки-мышки. - Туннельный блок наполовину уничтожен! - крикнул техник.
На ВР туча из черных нитей все глубже вгрызалась в оставшиеся щиты.