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User’s Guide The ESA/ESO/NASA FITS Liberator v.3.0 Colophon This User’s Guide w

User’s Guide The ESA/ESO/NASA FITS Liberator v.3.0 Colophon This User’s Guide was written by Robert Hurt, Lars Lindberg Christensen, Kaspar K. Nielsen and Teis Johansen. The team behind the ESA/ESO/NASA FITS Liberator: Project Executive: Lars Lindberg Christensen (lars@eso.org) Technical Project Manager: Lars Holm Nielsen Developers: Kaspar K. Nielsen & Teis Johansen Technical, scientific support and testing: Robert Hurt & Davide de Martin Acknowledgements FITS is an abbreviation for Flexible Image Transport System. FITS has been a standard since 1982 and is recognised by the International Astronomical Union. The ESA/ESO/NASA FITS Liberator uses NASA’s CFITSIO library, libtiff, TinyXML, Boost C++ Libraries, Object Access Library and Intel Threading Building Blocks. Adobe® and Photoshop® are either registered trademarks or trademarks of Adobe Systems Incorporated in the United States and/or other countries. We kindly ask users to acknowledge the use of this program in publicly accessible products (web, articles, books etc.) with the following statement: This image was created with the help of the ESA/ESO/NASA FITS Liberator. Cover: This is a 34 by 20-degree wide image of the area near the galactic centre. The image shows the region spanning the sky from the constellation of Sagittarius (the Archer) to Scorpius (the Scorpion). The very colourful Rho Ophiuchi and Antares region features prominently to the right, as well as much darker areas, such as the Pipe and Snake Nebulae. The image was obtained by observing with a 10-cm Takahashi FSQ106Ed f/3.6 telescope and a SBIG STL CCD camera, using a NJP160 mount. Images were collected through three different filters (B, V and R), “liberated” with the FITS Liberator and then stitched together. This mosaic was assembled from 52 different sky fields made from about 1200 individual images totalling 200 hours exposure time, with the final image having a size of 24 403 x 13 973 pixels. Credit: ESO/S. Guisard. This image was created with the help of the ESA/ESO/NASA FITS Liberator. The ESA/ESO/NASA FITS Liberator User’s Guide 3 Table of Contents 1 Introduction to the FITS Liberator ........................................................................ 4 2 Installing the FITS Liberator ................................................................................ 7 2.1 FITS Liberator v. 3.0 System Requirements ............................................... 8 2.2 Windows Installation .................................................................................... 8 2.2.1 Installing with the Setup Program ............................................................ 8 2.2.2 Manual installation under Windows ......................................................... 8 2.3 Mac OS X Installation .................................................................................. 8 2.3.1 Automatic installation ............................................................................... 8 2.3.2 Manual install ........................................................................................... 9 2.4 Uninstall information .................................................................................... 9 3 FITS Liberator Basics ........................................................................................ 10 3.1 The FITS Liberator Interface ..................................................................... 11 3.2 The FITS Liberator Workflow ..................................................................... 12 3.3 Handling High Dynamic Range Images ..................................................... 13 3.3.1 A Quick Example of Stretch Functions .................................................. 13 3.3.2 More about Stretch Functions ................................................................ 14 3.3.3 Scaling Images for Better Stretches ...................................................... 14 3.4 Entering Metadata ..................................................................................... 16 4 Cookbook Examples .......................................................................................... 18 4.1 Step-by-step Image Export ........................................................................ 19 4.2 Making a Colour Composite Image in Photoshop ..................................... 19 4.3 Notes on the performance ......................................................................... 20 4.3.1 Work flow optimization ........................................................................... 20 4.3.2 Operating system and physical memory (RAM) .................................... 20 4.3.3 Applying the stretch values .................................................................... 20 4.3.4 Flipping the output image ...................................................................... 21 5 Reference Guide ............................................................................................... 22 5.1 Tabs ........................................................................................................... 25 5.2 Processing Tab: Tools ............................................................................... 25 5.3 Processing Tab: Preview Window ............................................................. 26 5.4 Processing Tab: Histogram Window ......................................................... 26 5.5 Processing Tab: Image Data ..................................................................... 26 5.6 Processing Tab: Image Statistics .............................................................. 27 5.7 Processing Tab: Scaling and Stretch (Advanced) ..................................... 27 5.8 Processing Tab: Channels ........................................................................ 30 5.9 Processing Tab: Undefined Values ........................................................... 30 5.10 Processing Tab: Other Settings ................................................................. 30 5.11 Preferences Dialog .................................................................................... 31 A. More about Metadata ............................................................................................ 33 B. Behind the scenes ................................................................................................ 36 The ESA/ESO/NASA FITS Liberator User’s Guide 4 1 Introduction to the FITS Liberator The Wide Field Camera 3 (WFC3), a new camera aboard the NASA/ESA Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. Credit: NASA, ESA and the Hubble SM4 ERO Team The ESA/ESO/NASA FITS Liberator User’s Guide 5 he release of version 3 of the popular ESA/ESO/NASA FITS Liberator image processing software means that it is even easier and faster to create colour images using raw observations from a range of telescopes, including the NASA/ESA Hubble Space Telescope, NASA’s Spitzer Space Telescope, ESO’s Very Large Telescope and ESA’s XMM-Newton Telescope. Version 1 of the ESA/ESO/NASA FITS Liberator was completed in July 2004 by imaging scientists at the European Space Agency, the European Southern Observatory and NASA. FITS stands for Flexible Image Transport System. This single file format archives nearly all images of stars, nebulae and galaxies produced by major telescopes around the world. Before July 2004 this file format was primarily accessible to scientists working with highly specialised image processing tools. More than 60,000 laypeople, educators and amateur astronomers have started using the Liberator since the release of v.1 in July 2004. The FITS Liberator has also become the industry standard for professional imaging scientists at the European Space Agency, the European Southern Observatory and NASA. Stunning images such as the iconic Hubble image Pillars of Creation (Figure 1) can be created in a matter of minutes using the FITS Liberator. Version 3.0 of the ESA/ESO/NASA FITS Liberator provides the following new features: o FITS Liberator is now a stand-alone application, which means that Photoshop is no longer required. o Processing medium-sized images is now up to 35% faster, thanks to significantly improved memory management. o Processing large images are also faster thanks to delayed application of stretch functions. o FITS Liberator saves TIFF files that open in virtually any image processing software. o Open-source code base available on http://code.google.com/p/fitsliberator. Versions 2.0, 2.1, 2.2 and 2.3 had several notable improvements over v.1.0: o FITS images with up to 4 billion greyscale levels can be processed (32-bit support). o FITS images with up to 500 million pixels or more can be processed (100 times larger than standard images from a digital camera). o An improved user interface and a redesigned order of operations simplify the overall process – for example, the program now remembers previous settings. o New options for advanced Scaling and Stretching to fine tune images for optimal results. o A whole section dedicated to inputting metadata, i.e. information about the image and what it shows. Metadata will be an important tool for future efforts to make archives of ‘pretty pictures’ more accessible. o User access to a text version of the original FITS header. Universal Binary for Mac allows native CS3 operation on Intel-based systems. o Flip image checkbox allows image orientation to be selected on import. o Root functions (x1/2, x1/3, x1/4, x1/5) now operate antisymmetrically about x=0. o Version 1.1 of the Astronomy Visualization Metadata (AVM) standard is now fully supported. For more information see http://www.virtualastronomy.org o The import of coordinate metadata from the FITS header has been improved. o Full support for Photoshop CS4 (on both Mac and Windows). T The ESA/ESO/NASA FITS Liberator User’s Guide 6 o Significant performance (speed) enhancement through the usage of multiple CPUs and CPU cores as well as an improved memory management strategy (helpful especially for large images). o Support for planetary images through the PDS image format. o Metadata editing support for Photoshop CS4. o Options for the histogram markers stretched mean, stretched median, peak level and background level. o It is now possible to change the default initial guess between three different modes (a specified percentage of the histogram for the black and white levels, the mean +/- the standard deviation or the median +/- the standard deviation). o The World Coordinate System (WCS) coordinates are now given when the user sweeps the image pixels with the mouse pointer. Figure 1 Version 3 of the FITS Liberator makes it even easier to create stunning images. The iconic Hubble image Pillars of Creation, seen here, can be created in a matter of minutes. The three-colour dataset used to create this image can be downloaded from: http://www.spacetelescope.org/projects/fits_liberator/eagledata.html. The advantages of using FITS Liberator over professional image processing tools are indicated in the right-hand image: 1. Added detail in the shadows. 2. Increased gamut (colour space, more nuances). 3. Slightly better noise characteristics. 4. Easier access to advanced cosmetic cleaning tools as demonstrated by the removal of ghosts. The ESA/ESO/NASA FITS Liberator User’s Guide 7 2 Installing the FITS Liberator Figure 2 Image of part of a stellar remnant whose explosion was recorded in 185 AD. By studying this remnant in detail, a team of astronomers was able to solve the mystery of the Milky Way’s super- efficient particle accelerators. The team shows that the shock wave visible in this area is very efficient at accelerating particles and the energy used in this process matches the number of cosmic rays observed on Earth. North is toward the top right and east to the top left. The image is about 6 arc minutes across. Credit: ESO/E. Helder & NASA/Chandra The ESA/ESO/NASA FITS Liberator User’s Guide 8 2.1 FITS Liberator v. 3.0 System Requirements Minimum requirements: o Windows PC uploads/Litterature/ user-guide 98 .pdf