... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document “Programmatic Requirements for Gemini Instrumentation Development” states the requirements for the Software Maintenance Manual . ...

This describes the exposure window used by each instrument (the graphical interface for the hub's expose command). ... To open the expose window for a given instrument, bring up that instrument's main window, then press the Expose... button along the bottom. ... The top panel shows the status of the current exposure sequence (regardless of who started it). ... File: the file name for the current exposure, or the most recent exposure if not exposing. ... Download: exposure download preferences. ...

... Meade Instruments Corporation . ... 505 Connector Cable Set . Operating Instructions for use with the Meade? Autostar? ... The #505 Connector Cable Set provides access to three Autostar operations: . ... 2: #505 Connector Cable Set connects between two Autostar handboxes. (1) 3-foot cable. ... If you have a question concerning use of the #505 Connector Cable Set, call the Meade Instruments Customer Service Department at (949) 451-1450, or fax at (949) 451-1460. ... Autostar Downloads . ...

... pyqc.tar v2.0 (May 2014) . ... pyQC script structure . ... plot modules . ... instrument-independent module creating 2D images from a single detector (raw frame, master, comparison to reference) . ... instrument-independent module creating a simple 2D image from a raw or product file; does not need additional configuration . ... instrument-independent module creating an overview of all (or of a selected number of) extensions in a raw or product file; does not need additional configuration . ...

... Charge Coupled Devices (CCD) are currently by far the most widely used type of detector in astronomy. ... After a brief introduction to the VLT Control System, the VLT CCD Detectors Control Software is presented. The VLT Control System is a distributed system consisting of a set of UNIX Workstations, dedicated to high level operations, such as coordination of sub-system activities and interface to the users, and VME-based Local Control Units (LCU), dedicated to the control of sub-systems hardware. ...

XmTel uses the XPA interface for extensible connection to the operating system and scripting. ... Support for several commercial telescopes and controllers under Linux .. ... Software Bisque Paramount ME (requires RTS2 library) . ... In the current version of XmTel .. ... Offers command line and scripted operation using XPA . ... Version 7 includes the XPA server, telescope drivers, a client, utility software, and a standalone option that does not use XPA. ... Previous versions and support for INDI . ...

OptInt PmWiki . Pm Wiki / . Edit Page | ... MROI Delay Line Design Contract . ... AP local page . ... Backup and Restore . ... Your wiki installation contains some unique data in the following directories: . local/ Local configuration scripts cookbook/ Recipes obtained from the Cookbook pub/ Publicly accessible files wiki.d/ Wiki pages uploads/ Uploaded files (attachments) . A good backup plan will include periodically archiving these directories or at bare minimum local/ and wiki.d/ . ...

INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

... Meta Index / Home Page / Output Files / Summary File specification from There will be 6 instrument details records, one for each instrument, following the file details record. ... After each instrument details record there will be n exposure records, where n is the number of exposures during the observation for that instrument. ... Number of exposures . ... Identifies the record as an Instrument Details Record . ... If the instrument was inactive then this value is zero and no exposure records...

... ACQ in LSA with BRIGHT=RETURN. ACQ/PEAKUP to center star in SSA if that aperture is used for the science observations that follow. IMAGE, if you wish to obtain an image of the object. ... ACCUMs at wavelengths of interest. ACQ/PEAKUP in the SSA if the previous observation was in the LSA. ACCUMs for that different aperture. ... At the end of the chapter we have provided several illustrative examples. ... Image Mode . Accumulation Mode . ... Examples of GHRS Phase II Proposals . ...

... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Programs . ... apachectl is a front end to the Apache HyperText Transfer Protocol (HTTP) server. It is designed to help the administrator control the functioning of the Apache httpd daemon. The apachectl script can operate in two modes. ... If your Apache installation uses non-standard paths, you will need to edit the apachectl script to set the appropriate paths to the httpd binary. ... Starting Apache . ...