recipe_editor: Recipe Editor ################# The Recipe Editor is a graphical tool for editing recipe files: changing the input files, the data processing steps, their order, or the various function parameters. ... At the center right is a table listing the primitives in the current recipe. ... To create a Recipe, first load FITS files into the input file list using the Add Files or Wildcard buttons. ... Working with Calibration Files**: Many primitives require calibration files to be specified. ...

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• Data Parser GPI Data Pipeline 1.0 documentation
• The Calibration Database GPI Data Pipeline 1.0 documentation

... The visibility datasets possibly contain correlations for different polarizations and Stokes parameters. There are two basic ways that polarization characteristics can be measured: firstly, two orthogonal feeds can be present on the antennas, and the four different polarization correlations from a baseline can be taken and recorded. ... There are two ways the user can determine which polarizations he or she wants to process, either with the select parameter, or with the stokes parameter. ...

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• ChannelSelTask CentralProcessor 0.11 documentation
• PPTA Wiki | PmWiki / Forms
• User Parameters - Preparation of the Science field data CentralProcessor 0.11

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... yes . dataset . ... Whether to construct the OOTE image directly from the event list or indirectly from a source list. ... Name of the event list dataset used to construct the OOTE image. This parameter is read if style =`evlist'. srclisttab . ... Name of the source list dataset and table used to construct the OOTE image. ... sky . ... This parameter is read if outputstyle =`sky'. ...

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• Reviewtool
• Changing parameters

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... User authentication using an SQL database . ... Database Management #Use the PostgreSQL driver DBDriver pgsql #Connection string: database name and login credentials DBDParams dbname=htpasswd user = apache password =xxxxxx #Parameters for Connection Pool Management DBDMin 1 DBDKeep 2 DBDMax 10 DBDExptime 60 #Authentication Section Directory ... SQL query to look up a password for a user . ...

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• LEDA documentation: homogenisation
• Documentation: LEDA: parameter: vopt
• HyperLEDA documentation: parameter: vrad

OptInt PmWiki : Pm Wiki / Forms . ... Forms processing can be found in the Cookbook (see below). ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...

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• OptInt PmWiki : Forms
• Supernova Remnant (SNR) Catalogue or Catalog of Galactic SNRs
• Simple logging of scripts and their parameters Bojan Nikolic web pages (r. 329)

... Apache HTTP Server Version 2.4 . ... Group Authorization and Login using SQL . ... implement functions that start and end client-side sessions. # mod_dbd configuration DBDriver pgsql DBDParams dbname=apacheauth user = apache pass=xxxxxx DBDMin 4 DBDKeep 8 DBDMax 20 DBDExptime 300 Directory /usr/www/my.site/team-private/ # mod_authn_core and mod_auth_basic configuration # for mod_authn_dbd AuthType Basic AuthName Team AuthBasicProvider dbd # mod_authn_dbd SQL query to authenticate a logged...

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• mod_macro - Apache HTTP Server
• mod_authn_dbd - Apache HTTP Server
• mod_session_crypto - Apache HTTP Server

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

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• Exploring Interactive Archive Data Presentation at the COSSC
• XHelp: A Help Navigator for the IRAF System
• TwoFitlines: An Spectrum and Line Analysis Tool

... Parameters of the Moon-perturbed orbit . ... From orbits consistent with this limitation and with the date of the launch October 1, 2000 as an example, an orbit was selected with apogee directed to the North Galactic pole at the begining and rotation of orbit plane was maximized. The initial state vector is given in the inertial coordinate system in epoch J2000.0. ... The orbit has initial perigee radius Rp=7000.0 km, initial apogee radius Ra=343000.0 km and initial period T=8.453 days. ...

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The Interball-Tail KP archive is final. ... Select a day: . Data available since August 3, 1995) . ... DAY . ... Magnetic field (PRAM) Electron density and mean energy (ELECTRON) Ion density, velocity and temperature (CORALL) Energetic particle fluxes (DOK-2 and SKA-2) H+ and O+ fluxes (PROMICS) AKR intensity (AKR) Antisunward ion flux (VDP) Plasma wave amplitudes (MIF-M/PRAM) PC index (Ground-based) INTERBALL-TAIl orbit . ... Now data in all formats are available for 1995-2000) . GIF plot . ...

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• INTERBALL-AURORAL KP plots

... Of the 4 buttons in the bottom part of the configuration screen, three deals with power level adjustments: the 'Power control' button brings up the power control window where You can adjust the power levels of the different parts of the IF/LO system, the 'Power levels' button brings up the power level monitoring window (which also can be run outside CIMA as the 'powerwin' program), and the 'Adjust Mock power' button which adjusts the power levels on the Mock spectrometer (but nowhere else). ...

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• CIMA Configuration Files
• Arecibo Observatory L-Wide Band Receiver
• Your NED Search Results

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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To construct frequency distribution (histogram) of minor planets according to value of some element/ parameter/ function user should first select Elements item in menu bar and then Histogram in drop-down menu. ... User has possibility to save histogram or to print it using standard means. To save the file select File item in menu bar and then Save As... in drop-down menu. ... To print histogram select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print . ...

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... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...

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• MCP Menu documentation
• Astrophysical Research Consortium - Apache Point Observatory

To change the Scaling Function (how pixel values are binned into color levels): . ... For example, the basic grey-scale color map specifies no intensity for any color at the lowest color level, full intensity for all colors at the highest color level, with the red, green and blue intensities varying linearly for intermediate levels. ... At low bias, low color levels (i.e., low pixel values) will have non-zero intensities, while at high bias only high pixel values will have non-zero intensity. ...

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• The Markers Menu
• A Region mask for a radial profile in concentric, elliptical annuli
• Treatment of Errors

... Search Authors: . ... Tokhchukova S., Bogod V., Detection of the long-term microwave "darkening" before the July 14, 2000 flare //Solar Physics, 212/1, pp. ... A.Nindos , C.E. Alissandrakis, G.B. Gelfreikh, V. N. Borovik, A.N. Korzhavin and V.M. Bogod Two-dimensional mapping of the sun with the RATAN-600 // Solar Physics l65: 41 - 59, 1996. ... О. Н. Шиврис Работа радиотелескопа РАТАН-600 с плоским отражателем Изв.САО 1980, 12, с.134-140. ... List of selected publications Bogod V.M . ...

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• Access via e-mail
• Writing programs that use comedi and comedilib
• SCORPIO-2: direct images

home education > resources . SEARCH ASP SITE: Match ALL words Match ANY word . ... The Universe in . ... http://cosmictimes.gsfc.nasa.gov/ (James Lochner and Barbara Mattson have compiled a rich resource of 20th-century cosmology history in the form of news reports on key events) . ... Sean Carroll (Caltech): The Origin of the Universe and the Arrow of Time (Aug. ... Adam Reiss (STScI): Dark Energy and the Fate of the Universe (March 7, 2006 at the Space Telescope Science Institute): . ...

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• ASP: Astronomy Education: A Selective Bibliography
• ASP: Mercury Winter 2011
• ASP: Mercury Magazine

. N orilsk N eutron M onitor . Cosmic rays variation . Atmospheric pressure . Year . Month . Day . Hour . Minute . From . To . Resolution . Type of Data . 1 year 1 month 27 days 1 day 12 hours 6 hours 1 hour 15 min 10 min 5 min 1 min . Corrected for Pressure Atmospheric Pressure Uncorrected for Pressure . Data are also available by FTP . All Data for all Station are available by FTP . Links . Irkutsk .

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• Sayan spectrographic cosmic ray complex Irkutsk 2000 meters
• Саянский спектрографический комплекс космических лучей г.Хулугайша 3000 метров
• Sayan spectrographic cosmic ray complex Irkutsk 475 meters

... spectrum . ... sfit . ... define >macro_name< : define a macro . ... meth_range <w1> <w2>: Set wavelength range for fit . data_spectrum <name> : data in "spectrum" format . ... data_sigma <sigma> : define mean standard error in data . ... data_line_set | ... NB: synth uses multiple calls to spectrum , so various Spectrum commands may also be required. synth : find optimum fit by adjusting abundances, v turb , v sin i , and v rad . ... save <fit> : Save the spectrum and best fit from synth . ...

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• Selecting the backup medium
• sfit help file
• SCL Sfit Genetic Commands

... Algorithm for selection of defining sources 1. ... Take the common part of the "minimum" sets Make 1. and 2. for both global solution and time series and obtain common set 319 common sources for "global solution sigmas" case Comparison of IAA list, and 380 sources OPA list, set of defining sources ICRF1 and combined set Solution · Given catalogue RA, DE, arbitrary catalogue ra, de. dRAi RAi ra i Algorithm can be improved with additional condition Sum over all deltas less than 1 degree. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/heinkelmann_swg3.pdf
• Страница Е.В.Милецкого / Page of Eugen Miletsky

... The predicted MIR's ground tracks, which pass near INSPIRE net, are available in this home page. The track consists from magnetic footprints calculated by magnetic mapping from MIR positions with 30 s step. ... For each time some of the INSPIRE net place are selected as soon as its coordinates are close to the MIR magnetic footprint (the geocentric angular distance between SP and footprint is less then 2.1 deg) . Back to the Top . ... Back to the IKI Satellite Situation Center (SSC) . ...

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• IKI SSC, INTMINS APRIL99
• Interball Data Archive Home Page