ASC-FITS-2.0.1: ASC FITS File Designers' Guide (Rots and McDowell) (1999 Jun) . ASC-FITS-REGION-1.0: FITS region document (McDowell and Rots) (1998 Mar) . ... CXC-DM-001 Introduction: Data Analysis with the Chandra Data Model (2001 Oct) . ... 1998 Feb 26: SDS-1.0: Data Product List: obsolete . ... 1998 Mar 09: SDS-10.0: (ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) . ...

Several hundred images currently available in the STIS parallel archive have been examined to give a flavour of the sort of data that has been taken and an indication of the longer term promise of this archive. The data range from low Galactic latitude star fields with bright (~16th mag) stars, to very crowded star fields in the surroundings of the M 31 dwarf companions to very sparse fields of faint galaxies. ... Galaxy Field . Star Field . ... STScI Home Page ћ Instruments ћ STIS Home Page . ...

There are 8 correlator boards that make up the wapp spectrometer. ... The correlator boards are grouped in pairs. ... When used with alfa, a single correlator board services 1 beam of alfa. Since there are only 7 alfa beams, the last correlator board (8) gets a duplicate of the last alfa beam (6 counting 0.. ... 0 based) . ... synths used (1 based) . ... Current directory base: /home/cima/Wapp/Software/Svnwork . ... real time control of wapp correlator. talks to wapp boards via edt card. ...

. Previous . Next . George Essig is a web developer for the Federal Reserve Bank of St. Louis. Since 2000, he has been using Linux, Apache, PostgreSQL, and PHP to automate the publishing of economic research and data to the web. Previously, he worked as a research analyst at the St. Louis and Chicago Feds programming macroeconomic forecasting models. He holds a Masters in Economics from Washington University in St. Louis and a Bachelors in Economics from the University of Missouri.

Next: Resampling the Data Up: Geometric Correction Previous: Getting the Dispersion . The distortion љ along the slit can be modelled using an image containing one or several spectra of (ideally: point-) sources with well defined continuum. ... If the resulting coefficients are stored in the keyword COEFY*, (*=I,R,D) and combined with suitable (if necessary: dummy) coefficients for the dispersion resolution in the keyword KEYLONG*, (*=I,R,D) , the command RECTIFY/LONG can be applied. ...

... We describe a parallel code for 3-D structure detection and morphological analysis. The method is based on a multiscale technique, the wavelet transform and on segmentation analysis. ... This paper presents a new parallel code, that allows a rapid structure detection and morphological analysis in a 3-D set of data points. ... Segmentation analysis. ... Our code is based on the programming paradigm MASTER/SLAVE . ... Finally, the morphological analysis is executed by the master. ...

... A baseline vector is oriented from telescope 1 to telescope 2, i.e. the baseline coordinates are the coordinates of station 2 minus the coordinates from station 1. In the aperture plane, the coordinate increases to the East, and the coordinate increases to the North. ... In PEARL, a map on the sky is allocated with the -coordinate corresponding to RA, which increases to the left (East). The relationship between visibility and map is then . ...

Next: In-Line Documentation Up: Program Development Previous: Program Development . ... Though you should program in standard FORTRAN, two extensions will generally be needed by the programmer. Firstly Miriad uses both upper and lower case character strings (Fortran-77 strictly supports only upper case characters. ... Secondly Miriad tasks should use the maxdim.h include file where appropriate. ... Next: In-Line Documentation Up: Program Development Previous: Program Development Miriad manager . ...