Release Notes for Science Data Archive
User Interface (Version 1.6)

Release Date: Tuesday, 29 October 2002

Introduction

The release of v1.6 of the Science Data Archive (SDA) user interface (UI) includes many new tools and functions that were originally designated for the upcoming release of v2.0. Because these new tools significantly enhance the navigation of the UI and access to the data, we chose to release them now rather than wait for all the goals for v2.0 to be completed. Described below are the hardware and software requirements for v1.6, the basic functionality of v1.6, a summary of changes since v1.0, the known limitations of v1.6, and the planned improvements for v2.0.

Hardware Requirements for UI v1.6

There are no specific hardware requirements for operating the UI. Any computer that accommodates efficient WWW browsing will be sufficient for basic UI functionality. However, computers should have sufficient memory and processing speed to display and manipulate drizzled WFC images.

Software Requirements for UI v1.6

The UI is a WWW-based interface to the SDA database and image storage media (RAID). The UI has been designed with strict adherence to the XHTML and DOM HTML (through JavaScript/ECMAscript bindings) standards, so it will perform well with any WWW browser that fully supports these standards. The recommended browsers for the UI are:

Netscape 4.7x (for any platform) and Internet Explorer 5.x (for Windows and Unix) do not properly execute the UI and are therefore not supported by the ACS archive group.

Proper use of the UI requires the following browser options be set:

These options are default settings on most browsers. For Mozilla and Netscape, they are changed via the "Edit Preferences" menu option --> "Advanced" category --> "Scripts and Windows" subcategory.

Finally, a FITS image viewer must be installed to properly display FITS images through the UI. Such viewers include:

To enable your browser to spawn the FITS viewer, edit your browser preferences to include a MIME type of "image/x-fits" for extension "fits " and the correct path to the executable for the FITS viewer.

Basic Functionality of UI Version 1.6

The UI has two basic functions:

Whereas both functions were performed via a common query form in v1.0, the search and retrieval of images are now performed via a dynamically generated data inventory page. Searches for detected objects are still performed through the query form. This form has a tabbed format, meaning that the basic steps of a query (defining search criteria, selecting output fields, and viewing results) are accessed through a tabbed menu.

Image search and retrieval

The SDA stores selected images generated by CALACS and APSIS. The CALACS images are produced by on-the-fly calibration through MAST. Only the calibrated FLT and CRJ files, which are the input products of APSIS, are stored in the SDA. All other CALACS files must be retrieved through MAST. The APSIS image products that are stored in the SDA are:

All archived CALACS and APSIS images can be downloaded through the UI's data inventory and/or displayed with standard FITS image viewers spawned by the WWW browser. The detection images generated by APSIS can be viewed as color PNG files through set summary pages linked to the data inventory. The ancestors and descendents of each archived image can be traced, thereby providing the user a pedigree of every archived APSIS run.

Object search and analysis

Objects in each GTO image are identified and characterized photometrically, astrometrically, morphologically, and cosmologically by APSIS. The object catalogs generated by APSIS (detection, filter, photometry, and BPZ) are transformed into searchable database tables. Object queries are formed by constraining selected parameters from each of these catalogs.

Version 1.6 of the UI offers several tools for inspecting and analyzing the results of object queries:

Changes to UI Since v1.0

Features of v1.6 that alter the appearance or functionality of the UI since the last release include:

Limitations of Version 1.6

Because v1.6 is a preview of the larger v2.0 release, it lacks some important functionality requested by the GTO team at the Summer 2002 meeting in Wyoming. Limitations of this release include:

Improvements for Version 2.0

Planned improvements for v2.0 include, but are not limited to:

Previous UI Release Notes


Contact Information

Inquiries may be directed to:
David Golimowski, Manager
Terence Allen, Programmer
William Jon McCann, Systems Administrator