Next: The ESO VLT CCD Detectors Software . ... Up: Instrument-Specific Software . ... The framework for data calibration and analysis of the VLT instrumentation is presented, based on the concepts of a calibration plan, pipeline calibration, quality control, and archiving of calibrated data for a ground-based observatory. ... Quality Control Pipeline provides quality assessment for instrument performance data and observing conditions, and tests the results of the Reduction Pipeline. ...

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• On-The-Fly Re-Calibration of HST Observations
• HST Data Flow with On-The-Fly Reprocessing
• NICMOS Calibration Pipeline: Processing Associations of Exposures

The pipeline processing of WFPC2 data sets reformats the telemetry received from HST into group FITS format images, generates headers containing a large number of keywords taken from both the HST and WFPC2 telemetry streams, in addition to various STScI ground system databases, and applies the corrections described below. ... Bias image subtraction (depending on the gain and mode [FULL or AREA]) . ... Flat field image correction (depending on filters and mode used) . ...

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• NICMOS Data Handbook
• STIS Instrument Handbook
• FOC Data Handbook

... Science . ... Science Users Information > Science Publications > Science Announcements > Processed Calibration Files for VLT instruments Now Available . ... ESO Data . ... ESOReflex data reduction workflows can be used to customize the generation of the processed and co-added calibration frames and to apply them to the science files. A detailed step-by-step guide on how to automatically associate the appropriate calibrations, raw or processed, to the science files of interest is available . ...

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• Association: tutorial
• ESO - MUSE
• Data Flow System overview

Next: Illumination Corrected Flat Up: Additional Processing Previous: Sky Illumination Corrections . For creation of one or more sky illumination correction frames the command ( SKYCOR/CCD ) is available. ... After this calibration step, the command will smooth the reduced sky frame(s) to create the final sky illumination frame(s). ... After the illumination frame has been created, one can multiply the original flat field by the illumination frame, resulting in an adjusted flat field. ...

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• Basic Reduction Steps
• HyperLEDA Internal documentation
• List of Tables

... On­The­Fly Re­Calibration of HST Observations B. Pirenne and A. Micol Space Telescope -- European Coordinating Facility, ESO, Garching, D­85748 D. Durand and S. Gaudet Canadian Astronomy Data Centre, DAO, Victoria, BC Abstract. ... On­the­fly re­calibration data flow: from request submis­ sion to data delivery. ... On­the­fly re­calibration has another advantage for our archive sites: we only need to keep the raw data and calibration reference files on­line for the process to be automatic. ...

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• STScI NICMOS Software
• NICMOS Data Calibration and Analysis

XMM-Newton Science Analysis System Page: 1 ppssumm January 10, 2003 Abstract Produce an HTML summary page for any XMM instrument, or produce an HTML summary of the pipeline processing of an observation (including PNG or PS product le links). ... The product and processing information for the PPS Catalog information. ... NoLogoBanner (warning) (warning) corrective action: corrective action: No LOGO to be written to HTML le.NoINSTSUMMtoHTMLNo INST- SUMM records written to HTML. ...

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• Reviewtool
• XMM-Newton SAS: Watchout Page

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• The Wind Spacecraft
• SPICE System Overview .

... 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 . ...

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• ASKAPsoft processing of BETA data CentralProcessor 0.11 documentation
• Pulsar Group Observing/Tcs
• Spectral Line Processing and FITS files

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• Pulkovo NEO Page: Observations

Distributed Software for Observations in Near Infrared V. Gavryusev 1 and C. Baffa Osservatorio Astrofisico di Arcetri E. Giani Dipartamento di Astronomia, Universit`a di Firenze Abstract. ... The processes denoted for control of hardware (telescope and other instruments) should be executed currently on PC dedicated for this task under DESQview/X, while all other components (user interface, tools for the data analysis, etc.) can work also under Unix. ... 1993, Di Giacomo et al. 1993). ...

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• Lunar Occultation Group at AAO
• worker - Apache HTTP Server
• Starting Apache - Apache HTTP Server

On combined processing of different space geodetic observations . ... A software for combined processing of different space geodetic observations is developed along with the work on the co-location of various observational techniques at the observatories of Quasar VLBI network. ... Various aspects of the combined processing of different types of space geodetic observations are also discussed. ... space geodetic observations, combined processing, normal equations, software package, SINEX-format. ...

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• Intl collabration
• Keywords_65
• Keywords_27

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy

... In some cases where memory space is at a premium, it is possible to tailor the configuration to remove such features as reference clock driver support, debugging support, and so forth. ... The following lines are used in this file: . ... The DEFS_LOCAL line defines global flags that apply to all machines. Ordinarily, the only flags included are the -DDEBUG , which includes the debugging code, and -DREFCLOCK , which includes basic reference clock support. ... D_INCLUDE_BSD_SOURCE . ...

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• Sternberg Astronomical Institute
• Building and Installing the Distribution
• Bilbio

... Information processing in nonlinear systems with dynamic chaos // Доклады Международного семинара "Нелинейные цепи и системы".- ... The idea and the method for using one-dimensional nonlinear dynamic systems for storing and processing information were proposed in [1, 2]. ... The main part of the preprint is Section 4, where the "InformChaos" software pack, accomplishing the above principles of storing and processing visual information, is described in detail. ...

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• NIST Special Publication 500-223. A Framework for the Development and Assurance
• Project METI@home: Messages to ETI from home

APO/GIFS Instrument Factsheet The Goddard imager and Integral Field Spectrograph (GIFS) has recently been commissioned on the APO 3.5 m telescope. This factsheet presents a high level overview of the GIFS instrument. ... GIFS Imaging The GIFS imaging mode is used for imaging science and target acquisition for the IFS mode. ... Imaging Mode pixel scale: 0.168"/pixel · Comparison to Other APO 3.5m instruments: The GIFS field of view is smaller than SPICAM, but the filter set is far more extensive. ...

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• Spectrograph Interface Control
• Astrophysical Research Consortium - Apache Point Observatory
• TUI:Scripts:Scripting Tutorial:Get Info

... However, because ALFA was built to enable very large-scale sky surveys, NAIC seeks to encourage the formation of research teams, consortia, to take on the task of conducting ambitious sky surveys with the primary goal of creating legacy archival databases for public use. The legacy sky surveys are done as a partnership between NAIC and the research consortia, the policies and guidelines for which are summarized here. ... NAIC will archive the raw data at the Arecibo Observatory. ...

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• Radio Astronomy Backends
• Chapter 11. Specifying OpenGL Environment Variable Settings
• ALFA Front End Construction

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Support . ... Software & Firmware . ...

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• Meade Instruments - Telescopes, Solar Telescopes, Binoculars, Spotting Scopes
• Meade USB to RS-232 (Serial) Adapter - Software and Cables - Accessories -
• Meade Instruments Corp. - Meade Customer Support

Astron 193 Lecture 2, Jan.28, 2015 NOTES 1/ Data vs. ... 4/ Data Storage View Your Data Software to read the data files rrent Astronomy Formats FITS inary with standards, Cu b defined keywords, but may become not good enough for large data of the future LOFAR, SKA in radio, LSST ds9 display the data mage gui, but also access to catalogs download and image the files i event files contain all the information about the observation photons , energy, arrival times ...

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• Home Page for SAOimage: The Next Generation
• The Lynxx Tools
• Notes on IPC and PSPC Spectral Fitting

... Main . ... The RadioAstron is an international space VLBI project led by the Astro Space Center of Lebedev Physical Institute in Moscow, Russia. ... List of organizations which were taken part in developing of the project and now support the RadioAstron mission is presented here . The RadioAstron Newsletter # 29 , July 18, 2015. RadioAstron Announcement of Opportunity - 4 for observations from July 2016 to June 2017 inclusive. ... 2.7, December 17, 2015 : English version. ... Main ASC . ...

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• Список литературы и документации
• References and Documentation
• RadioAstron Mission Element Overview

To monitor the state of your processes use the ps command. ps [-option] . Used without options this produces a list of all the processes owned by you and associated with your terminal. Options for this command vary with the type of UNIX system that you are using. ... It may be that you are running more than one terminal session on the system and/or that you have processes which have no controlling terminal associated with them. ... Understanding process information . ...

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• Processes
• Restarting a suspended foreground process