GHRS Instrument Handbook 4.1 111 Index 112 GHRS Instrument Handbook 4.1 A Accumulation Mode 15, 20, 34, 43--45 CENSOR 45 details 88--89 COMB 16, 44 DOPPLER 45, 104--105 FP­SPLIT 16, 44 parameter summary 44 STEP­PATT 17, 44, 84 STEP­ TIME 45 substepping 20 acquisitions 17, 18, 25, 34, 34--41 ACQ/ PEAKUP , see acquisitions , ...

ChangeLog for dpssflag =============================== Open SPRs: Version 7.0.2 - 2006-06-28 (MC) ---------------------- - Solved bug affecting propagation of flags 2,3,4,5 from summary row to instrument rows when source counts are NULL for the first instrument Version 7.0.1 - 2006-02-24 (MC) ---------------------- - Update parameter description in dpssflag.par file Version 7.0 - 2006-02-18 (MC) ---------------------- - Correct bug in Add MOS submodes W3,W4,W6 for Flag 10 settings. ...

Next: The Reduction Session Up: Echelle Reduction Previous: Standard orientation . ... The command SHOW/ECHELLE displays only those parameters which must be set according to the options and methods chosen for the reduction. ... Current parameters are saved with the command SAVE/ECHELLE name , where name is the session name. ... Current parameter values are set to the default value with the command INIT/ECHELLE , or set to the values of a previously saved session with INIT/ECHELLE name . ...

... CentralProcessor 0.11 documentation . ... The parameters listed here allow the user to configure the parset and the slurm job for continuum imaging of the science field. Some of the parameters can be set to blank, to allow cimager to choose appropriate values based on its ?advise? capability (which involves examining the dataset and setting appropriate values for some parameters. ... Number of CPUs to use on each core in the continuum imaging. ... User Parameters - Continuum Self-calibration . ...

Next: Data Analysis Applications . ... The past decade has witnessed a movement within the astronomical software community towards Open Systems . ... We present examples of user-customizable systems that can be built from existing tools, based on commonly-used infrastructure: a parameter interface library, FITS file format, Unix, and the X Windows environment. ... However, the currently available parameter file systems have serious limitations when inserted into a heterogeneous environment. ...

... spectrum . ffit . ... grids . ... These commands read in a grid of model spectra. ... Values for the parameters are taken from the input models themselves, to avoid mixups. The syntax of the command arguments is precise. model{ . ... If there is only one spectrum to fit, one should set default parameters for the secondary which lie within the model grid, with <L_2/L> being a very small value. ... The output is saved in a file <file.fit> , where <file> was the name of the spectrum being fitted. ...

... Thus all regions of the 0.94-2.50 micron wavelength range accessible from Mauna Kea can be recorded using five fixed angle gratings. ... Grating Angle .