... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . ... The purpose of this software is to apply calibration parameters to Measurement Sets. It can be run with the following command, where ?config.in? is a file containing the configuration parameters described in the next section. $ ccalapply -c config.in . ... The name of the measurement set to which the calibration parameters will be applied. calibrate.scalenoise . bool . ... ccalapply (Calibration Applicator) . ...

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• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• ccontsubtract CentralProcessor 0.11 documentation
• Input Parameters to the Self-Calibration Tasks

... dataset . Name of the event list dataset. ... The name of a dataset with a template image in its primary extension should be supplied to this parameter. ... If outputstyle =`sky', the template image is also necessary to specify the pixel dimensions and World Coordinates of the output. withdss . ... If attstyle =`binnedset' the user should supply to the present parameter the name of a dataset which contains a time series of the spacecraft attitude variation during the exposure. flatexpcubeset . ...

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Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• Stellar parameters from calibrations of spectral types
• Parameters
• Score reports

. Next: Edition of the Up: Typical Run Previous: Creation of the . All of the atomic data listed in 13.2.1. are needed by the program and are to be entered via this table. A template can be found in MID_CLOUD: ABSP.TBL . The quoted parameters are from Morton and Smith (1973) and according to the author the wavelengths are: . vaccum for 2000 ?, air for 2000 ? . Command: . The actual format of this table is described in section Auxiliary Data. Pascal Ballester . Tue Mar 28 16:52:29 MET DST 1995

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• Permanent telescope parameters
• Parameter estimation
• HyperLEDA documentation: parameter: t

... ACQ-DIST Optional Parameter for FGS 1 , 2 . ACQTYPE Optional Parameter for STIS . Acquisition modes . ... ACCUM . ... AFTER date Special Requirement . ... BINAXIS1, BINAXIS2 Optional Parameters for STIS 1 , 2 . ... BUFFER-TIME Optional Parameter for STIS . ... CHECKBOX Optional Parameter for STIS . ... Calibration Targets . ... CR-SPLIT Optional Parameter for STIS . ... DIFFUSE-CENTER Optional Parameter for STIS . ... GAIN Optional Parameter for STIS . ... PCS MODE Fine Special Requirement . ...

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• Coordinated Parallel Containers

... Apache HTTP Server Version 2.4 . ... Session encryption support . ... session_crypto_module . ... The session will be encrypted with the given key. Different servers can be configured to share sessions by ensuring the same encryption key is used on each server. ... The SessionCryptoPassphrase directive specifies the keys to be used to enable symmetrical encryption on the contents of the session before writing the session, or decrypting the contents of the session after reading the session. ...

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• Program parameters
• mod_authn_dbd - Apache HTTP Server
• mod_macro - Apache HTTP Server

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

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• Initial parameters of compact stars
• Other parameters of the evolutionary scenario
• The Gravimagnetic Parameter

CIMA configuration files offer You a conveniant way of saving CIMA set-ups to files. ... Then instead of making this selections interactively when You are observing, You can just load and apply the configuration files. ... Any other set-up will be ignored! ... In that case, You are forced to use the 'Load only' option to load the configuration file, inspect the selected set-up carefully, apply the set-up (with the 'Accept' or 'Apply' buttons) and then save a new version of the configuration file. ...

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• ALFA Calibration Diode Temperature (Full Band)
• Orbits in the period / acceleration plane
• Rotang - IDL procedure for calculating the optimum rotation angle for ALFA

... As part of the development of a new Python-based CL for IRAF tasks by the Science Software Group at STScI, we have developed a GUI-based parameter editor for IRAF tasks using Tkinter. This new parameter editor is intended to provide the equivalent functionality of the IRAF EPAR task, but to make parameter editing easier by using appropriate user interface elements, such as menu choice lists, action buttons, and file browsers. ... Figure 1: The GUI-based Python/Tkinter IRAF task parameter editor. ...

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• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
• The SRON-HeaD Data Analysis System
• Indexing and Searching Distributed Astronomical Data Archives

... Several of the tasks in the spectral package share a common set of parameters. ... Each task in the spectral package has a hidden parameter which points to the pkgpars parameter file. The parameters stored here include the observed data sets and the model descriptor, and instrument-specific parameters. ... The observed counts and error data set contained in the table file ( *_obs.tab ) produced by qpspec will be the input data for subsequent spectral tasks. ...

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• Regions and Source Parameters
• Parameters
• *imexamine* - General analysis of image containing many sources

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...

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• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

... spectrum . ffit . ... grids . ... These commands read in a grid of model