... rgssources (rgssources-5.28) [xmmsas_20041122_1834-6.1.0] . Meta Index / Home Page / Examples. ... setenv SAS_CCF <the .cif file> setenv SAS_ODF <the ODF directory> rgssources srclist=PooooooooooiiteeeSRCLI_0000.FIT or setenv SAS_CCF <the .cif file> setenv SAS_ODF <the ODF directory> rgssources srclist=rrrrooooooooooiiteee00_sources.ds or setenv SAS_CCF <the .cif file> setenv SAS_ODF <the ODF directory> rgssources srclist=<non-standard name> instrument=<rgs1 or rgs2> exposure=<exp num> . ...

... HST . ... HST Overview . ... Other important information on coronagraphy can be found in Chapter 5 of the NICMOS Data Handbook, section 5.1 of the NICMOS Instrument Handbook as well as in the following performance summaries: Performance of the Coronagraph in Cycle 7 , and Motion of the Coronagraphic Hole OverTime . ... NICMOS ISR 2005-001: NICMOS Two Gyro Mode Coronagraphic Performance . ... 2004 AAS Poster--HST/NICMOS Coronography: Prospects for Cycle 13 and Beyond-A Choice of Coronagraphic Imagers...

Next: *timsort* Up: Timing Analysis Previous: Summary of tasks in . ... Events will be time ordered in the output file. xt> timsort xdata$snr psr ``c 503 513 24'' none A light curve is then generated and plotted so we can inspect the gross properties of the sample (the sequence of good-data intervals and gaps) and any source variability. xt> ltcurv psr none psr 500 xt> ltcplot psr_ltc Finding this sample satisfactory, we search for periodicity with a fast Fourier transform. ...

... The STECF IRAF layered package impol provides five tasks specifically aimed at reduction of HST imaging polarimetry data for ACS, FOC, NICMOS and WFPC2. ... Reduction of HST polarimetry data and simulation of raw polarimetry images, together with polarization vector plotting, are covered. ... hstpolsim -- Produce simulated polarization input data frames for HST instruments from images of the total signal, the linear polarization and the position angle of the polarization vectors. ...

To compare two directories in the current directory: diff usability Usability Only in Usability: schedule diff usability/email Usability/email 2a3,4 > Jean JRS@pollux.ucs.co > Jim jim@frolix8 . diff reports that the file (or directory) schedule is unique to the directory Usability . diff then reports that there are differences between the file email in the directory usability and the file of the same name in the directory Usability . ...

... Apache HTTP Server Version 2.2 . ... On systems with multiple users, each user can be permitted to have a web site in their home directory using the UserDir directive. Visitors to a URL http://example.com/~username/ will get content out of the home directory of the user " username ", out of the subdirectory specified by the UserDir directive. ... Per-user web directories . ... the URL http://example.com/~rbowen/file.html will be translated to the file path /home/rbowen/public_html/file.html . ...

... Several HST instruments both current and decommisioned have provided imaging linear polarimetry capabilities. ... The STECF IRAF layered package impol provides five tasks specifically aimed at reduction of HST imaging polarimetry data. ... Reduction of HST polarimetry data and simulation of raw polarimetry images, together with polarization vector plotting, are covered. ... For reduction of data from imaging linear polarization instruments other than from HST, the instrument name is `SPECIAL'. ...

... The Miriad task uvgen can be used to simulate a variety of observing modes. ... Simulating a telescope approximately, let alone in some detail, requires a good many parameters. uvgen takes an appreciable number of parameters and input files to describe the telescope, correlator and source. Fortunately keyword and set-up files for some common situations exist ( e.g. simulating the ATCA and VLA). ... For example, to load typical parameters for the ATCA, use miriad% source $MIRCAT/uvgen.def.atca . ...