- #TOPCAT TOOL MAC OS#
- #TOPCAT TOOL ARCHIVE#
- #TOPCAT TOOL FULL#
- #TOPCAT TOOL SERIES#
- #TOPCAT TOOL DOWNLOAD#
Breger, 2005, Period04 User Guide,Ĭommunications in Asteroseismology, 146, 53 Patrick Lenz, Institute of Astronomy, University of Vienna Platforms, Windows and Linux options are also available. The Java Runtime Environment (JRE) on your local machine.
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Identity power within time series and perform Period04 is designed for the statistical analysis of largeĪt the University of Vienna, Period04 supports the Theory and Observation of Pulsating Stars We invite users and developers to suggest more resources to add to this list. The interpretation of photometric time series.
#TOPCAT TOOL ARCHIVE#
Here we provide links to publicly available software that may be useful to GOs and archive users for PyKE can be installed on all PYRAF supported platforms from here. Contributions of new tasks or enhanced functionality of existing tasks by the community are welcome. Tasks to perform data analysis developed for the author's science programs are also included. The main purposes of these tasks are to i) re-extract light curves from manually-chosen pixel apertures and ii) cotrend and/or detrend the data in order to reduce or remove systematic noise structure using methods tun-able to user and target-specific requirements. PyKE was developed to provide alternative data reduction, tunable to the user's specific science goals. PyKE, on the other hand, is a group of python tasks developed for the reduction and analysis of Kepler Simple Aperture Photometry (SAP) data of individual targets with individual characteristics. Systematic reduction in the Kepler pipeline is optimized to yield the highest number of potentially-detectable exoplanet transits from a sample of 160,000 stars. Differing scientific goals are likely to have differing requirements for systematic mitigation. For every target there is a level of subjectivity required to reduce systematics. This pipelined reduction includes the removal of time-series trends systematic to the spacecraft and its environment rather than the targets. The Kepler archive contains raw and calibrated time-series data in both light curve and pixel form. Which the data have been published or made public are also indicated.
GALEX sources located within the frame are marked with symbols and user-selectable. The user to examine individual channels within an FFI image. MAST FFI VIEWER: MAST maintains am online
#TOPCAT TOOL DOWNLOAD#
The standalone python tool is available for download here. Individual pixels are chosen interactively by tapping upon them. KeplerFFI also creates a custom pixel mask by allowing users to select pixels for inclusion within a target aperture. KeplerFFI: This FFI inspection tool is used to examine the sources surrounding a target, assess crowding, identify artifacts, and understand the effects of the photometric aperture on the light curves.
#TOPCAT TOOL FULL#
We have founds DS9 to be of most employment inspecting Kepler's Full Frame Images. Multiple images together and contains scaling and zoom options. TOPCAT can be obtainedĭS9: SAOImage DS9 is an image visualization application, developedīy the Smithsonian Astrophysical Observatory. An example of TOPCAT inspection of a light curve product is provided here. Most convenient, powerful and useful software for inspection of Kepler light curve files.
Interactive graphical viewer and editor for tabular data. TOPCAT: Tool for Operation on Catalogs and Tables, a Java-based
#TOPCAT TOOL MAC OS#
Versions are available for Unix, Linux, Mac OS and Windows platforms. FV has proved to be the most efficient tool for inspecting Kepler's target pixel files. While by know means a complete list, we have found the tools listed here to be of most common employment in our own inspection of the Kepler data:įV: Software for display and editing FITS format tablesĪnd images, developed and distributed by NASA's High EnergyĪstrophysics Science and Archive Research Center. The content and format of each file are defined in the Kepler Archive Manual.Ī variety of free software exists for FITS data inspection. Each Kepler FITS product contains a combination of header keywords containing scalar data, time-dependent data stored as tables and/or detector pixel-level data stored as two-dimensional images.
A primer on the FITS format can be found here. General FITS documentation is maintained by the Office for Guest Investigator Programs (OGIP) FITS Support Office at NASA GSFC. Kepler data is encoded using the Flexible Image Transport System (FITS).