... Tools . ... SoFiA (from Greek ????? = wisdom), the So urce Fi nding A pplication, is a new H i source finding pipeline for finding and parametrising galaxies in three-dimensional H i data cubes. The software is still under development, and the latest version of SoFiA can be obtained from GitHub . ... SoFiA test data set (14.3 MB) . ... While SoFiA comes with its own, built-in user manual available through the graphical user interface, we also generated a printable PDF file for convenience: . ...

... AstroImageJ (AIJ) .. ... Reads and writes FITS images with standard headers . ... Provides a time and coordinate converter tool with capability to update/enhance FITS header content (AIRMASS, BJD, etc.) ... Creates color images and with native ImageJ processing power . ... AstroImageJ_Updater . Update operation now updates AIJ version number in Info.plist CFBundleVersion and CFBundleShortVersionString (MacOSX only) . ... AstroImageJ is ImageJ with astronomy plugins and macros installed. ...

... We have developed a suite of analysis tools and an on-line database for both the primary ChaMPlane X-ray data (source catalogs) as well as the optical counterpart data. ... The ChaMPlane VO provides access to our deep Mosaic optical (V,R,I,Halpha) images, catalogs of their optical photometry, Chandra images with exposure-map correction, X-ray source data and details of X-ray sources with identified optical counterparts. ... Chandra sources are displayed (right) in a smoothed Chandra X-ray . ...

... Up: Archives and Information Services . Previous: Search and Retrieval of the AXAF Data Archive on the Web using Java . ... Our Web interface to the HST archive (WDB) was substantially augmented during the past few months: A seamless integration of Java applets and CGI interfaces to the database now allows basic manipulation and visualization of data. ... These applets only require a common Web browser and offer very helpful features to facilitate archive data selection. ...

... Example images using the `cubehelix' colour scheme using AIPS . ... I have written up the implementation of a colour scheme -- called `cubehelix' -- which is intended to be perceived as increasing in intensity. ... There is no single `cubehelix', as there are several parameters that control this family of colour schemes: . ... This page gives several other colour wedges made with different parameters (along with the corresponding colour scheme files for use in DS9 or kvis , see Section 3.2 below). ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... python . ... base . loadInst.py . ... 8 љ import tcc.base . ... 12 љ def loadInst (instDir, instName, gcViewName=None, writeToUsers=None, cmd=None): . 13 љ """!Create an instrument block for the specified instrument . ... 15 љ @param[in] instDir path to instrument dir (typically tcc.base.getInstDir()) . ... 67 љ inst = tcc.base.Inst() . ... 73 љ # override the few values that are set based on file name (instead of file contents) . ... tcc.base . ...

... Meade Instruments Corporation . ... Section 3: File Menu . ... Displays the dialog to open an existing image: . ... Saves the current image as a new file name or new file type, or both. ... This can be useful to prevent having 20 or more images open at once, and saves having to close them manually. ... This is done by creating a text file with the same name as the image file. ... Note that Image Information is saved within the FITS file, so there will not be a text file to accompany these files. ...