... The OFWG The OFWG was set up to (1) ensure that new FITS definitions used within the OGIP do not violate any established FITS standards/conventions; (2) encourage standardization of keyword usage, data types, and FITS file formats used within the OGIP (i.e., the so­called Rationalized Data File or RDF format); and (3) disseminate OFWG recommendations to the broader High Energy Astrophysics and FITS communities to promote community­wide standardization. ...

... File Structure . ... There are five basic types of files (FITS tables) we use with the STSDAS software package Synphot and its successor pysynphot. component throughput tables (usually "_syn"): each such table gives the transmission curve for an individual element or "component" in the optical path of HST+SI. ... Master tables (For the most up-to-date files in use by pysynphot please check here ): . ... Since the set of pysynphot data files is rather large, they are distributed in separate tar files...

XMM-Newton SAS V5.1 Scientific Validation and Data . ... This page contains the Scientific Validation Report for SAS V5.1 (.ps.gz) as well as the data use for this validation. ... The SAS V5.0 Scientific Validation Page can be found here . ... Data Files Handbook (Issue 2.2). ODF/SDF Interface Control Document (Issue 2.9). The following datasets have been used for the Scientific Validation of SAS V5.1. ... Pipeline Products : Each Product Group is available separately as a .TAR file. ... ODF . ...

... ESO-MIDAS is decribed in full detail in a number of documents. ... ESO-MIDAS User's Guide ( Release 95NOV or Release 94NOV ) : . ... Describes the basic MIDAS system with all general purpose facilities such as MIDAS Control Language, all available commands, data input/output (including plotting and image display), table system (MIDAS Data Base). ... Apart for this "standard" set of documentation, the MIDAS Users community is provided with two other sources of information: . ...

... Astrophysics Group . ... Surveys and Catalogues . 10C . ... AMI-Planck . ... FIRST . ... The 15.7-GHz, 10C Survey was carried out using the Arcminute Microkelvin Imager (AMI) Large Array (LA), which is operated by the Cavendish Astrophysics Group at Lord?s Bridge, Cambridgeshire. ... The first 10C Survey results from an area of тЙИ 27 sq. degrees complete to 1 mJy and тЙИ 12 sq. degrees complete to 0.5 mJy have now been released. ... The 10C catalogue is available in ASCII and PDF formats. ...

... About ATNF overview . ... Parkes radio telescope . ... The focus of the ASKAP Community Workshop 2015 is ASKAP Early Science . This workshop will explore the scope, implementation and expected science outcomes of the ASKAP early science project, which is due to begin in 2016. ... Presentations will follow from representatives of each science area currently engaged with the ASKAP early science forum тАУ these presentations will be solicited by email through the early science forum exploder. ...