The Agile window provides complete control over the Agile high-speed photometer. ... All other parameters are specified as part of the command that starts an exposure sequence. ... To connect the filter wheel controller, issue this command in the command bar at the bottom of the Log window: agile connDev fw . ... To home the filter wheel controller, issue this command in the command bar at the bottom of the Log window: agile fwhome (there must be a filter wheel mounted in Agile for homing to succeed). ...

Below is a table of INTERBALL-2 experiments summary to remind you about specific features of each instrument. ... See bottom of the page for additional information. ... AURORAL PLASMA . ... Spectra of electrons and ions 0.03 < E < 15 keV; anisotropy of electrons and ions (M = 1, 4, 16), 30 < E < 500 keV/Q . ... IKI, Moscow, Russia . ... Electron and ion spectra and anisotropy (M = 1, 2, 4, 16), 0.005 < E < 20 keV/Q . ... Ion composition (M = 1-32) and 3-D energy distribution, 10 eV < E < 30 keV/Q . ...

... QC1 database . ... The quality information is derived in form of QC1 parameters. ... The Health Check monitor collects QC1 parameters and their scores. ... The results are presented in two views: the graphical HEALTH CHECK monitor with the full trending reports, and the QUICK-LOOK monitor with scores. ... The Health Check Monitor is a joint effort of the Quality Control Group in Garching and of Paranal Science Operations. ... You can download the QC1 parameters, and also connect to the QC1 database....

... Parameter . ... Type . ... data set . ... The name of the observation-wide attitude time series data set created by atthkgen . ... name of existing D -type column in attset . The name of the column in the attitude data set containing the time tags - passed to tabgtigen in parameter timecolumn . ... A selection switch which determines the type of selection expression that the attitude time series is filtered with. cone and pyramid select the fixed cone- and pyramid filters (see above) respectively. ...

COS Instrument Handbook for Cycle 24 . ... Cosmic Origins SpectrographInstrument Handbook for Cycle 24 > Chapter 8: Target Acquisitions > 8.9 Recommended Parameters for all COS TA Modes . ... Always follow the first ACQ/SEARCH with an ACQ/IMAGE , ACQ/PEAKXD+ACQ/PEAKD , or a second 2 в 2 ACQ/SEARCH which uses FLUX-WT weighting. ... Use NUM-POS=5 , STEP-SIZE=0.9 , and CENTER=FLUX-WT-FLR for most ACQ/PEAKD centerings. ... For ACQ/PEAKD , use of the special parameter CENTER=DEFAULT is recommended. ...

Next: Example Up: Long-Slit and 1D Previous: Command Summary . For the storage of control parameters and results, the context LONG uses a number of special keywords. They are intialised by the command SET/CONTEXT LONG , their values can at any time be listed by typing SHOW/LONG . The following table provides a brief description of the purpose of the LONG keywords: . Table: Keywords Used in Context LONG . Table: Keywords Used in Context LONG (continued) . Pascal Ballester . ...

Next: *counts_plot* - Inspection of Up: *fit* - Fit Data Previous: Fit a source with . The table of results obtained with fit can be listed with the stsdas.ttools task tprint . ... The table will be listed on the screen. tt> tprint rp90_prd prparam=yes # will list the table and its header # parameters, which include the best fit spectral parameter . Fig. 7.1a. Output from fit showing the data and best fit model folded through the instrument response (dashed line). ...

... Second, the observatory can control the configuration, test data analysis procedures, and provide calibration solutions with the help of instrument models. This paper presents the VLT object-oriented framework for the development of ETCs (Exposure Time Calculators) and data simulators. ... Instrument simulations are being developed for the purpose of predictive calibration, instrument configuration control, and evaluation of data analysis procedures. ...

... 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 . ...

... 18-1 74 40.5 0.52 Cas A . 18-1 75 38.5 0.49 Cyg A . ...

Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Moscow, 2008 Acknowledgements A.Belinskiy M.Kornilov A.Tokovinin M.Kuznetsov P.Kortunov E.Gorbovskoy SAI administration some SAI students Pulkovo solar station (KHSS) staff RFBR support MAVEG Gmbh Why to study optical turbulence and some other relevant ... Mean seeing by DIMM data for this night is 1''5. ...

OptInt PmWiki . ... Edit Page | ... Search : . ... MROI Delay Line Design Contract . ... MROI . ... This page uses custom searches. ... While it is not powered by a "search engine", it can be tweaked to produce results that are targeted and customized. Searches can be targeted to restrict the search to certain pages. ... Whether you use the search box below, or the regular search box that appears at the top of this page, any search that you run from this page will provide the customized results. ...

... NED Home . ... Redshift: Between 0.150000 and 0.270000 . Include ALL Object Type: QSO Radio . ... Number of Essential Note) RA DEC Type km/s z Qual arcmin Refs Notes Phot Posn Vel/z Assoc Images 1 30000 0.228000 0.0 26 0 8 3 0 0 Retrieve 2 30000 0.181000 0.0 5 0 4 1 0 0 Retrieve 3 30000 0.171000 0.0 67 1 1 0 0 0 Retrieve 4 30000 0.260000 0.0 90 1 16 5 0 0 Retrieve 5 30000 0.163009 0.0 170 10 5 4 3 0 Retrieve 6 30000 0.245000 0.0 27 1 1 2 1 0 Retrieve 7 30000 ...

Next: Acknowledgements Up: World Wide Web version Previous: Page contents . ... Part of the table and a cartoon figure of the track calculated for the default set of the initial parameters are shown in Fig. 1 and 2. In the future, we intend to made available calculations of a large number of binary systems assuming different intial distributions, chemical composition, etc., to construct a "Galaxy at will", as well as various interface facilities. ... Fri Jun 21 19:17:07 MSD 1996 ...

Next: Writing Shell Scripts Up: The User Interface Previous: Indirect Parameter Input . Miriad tasks can always be run by specifying their parameters on the host command line. ... For example, out=gauss sets the parameter out to the `value' gauss . ... Next, we will run a histogram task, histo , with the input image dataset gauss that we just created: % histo in=gauss . ... The command-line interface is quite appropriate for tasks that take relatively few parameters, or in shell scripts. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... ISS Russian Segment . ... ISS 45/46 . ... Microsatellite . ... Development testing of microsatellite (with mass up to 50 kg) injection from transport cargo vehicle (TCV) Progress with the use of transport-launch container fastened by operators to docking assembly (DA) ring. ... Microsatellite Chibis-M fastened on TLC as part of TCV Progress M-13M is delivered to the ISS RS. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

... 0.000 . ... IL'IN, V. B.; KRIVOVA, N. A.; MICHEL, B.; VOSHCHINNIKOV, N. V. WWW database of optical constants for astronomy . ... MANN, INGRID; KIMURA, HIROSHI; VOSHCHINNIKOV, NIKOLAI V.; IL'IN, VLADIMIR B. Radiation pressure forces on circumstellar dust particles . ... KRIVOVA, N. A.; IL'IN, V. B.; KIMURA, H. Dust shells around Herbig Ae/Be stars with Algol-like minima: results of a combined modelling of different observational data . ... ABSTRACT QUERY HELP . ... Return: Results Form . ...

... Image Quality of the VLT . Total Optical Control . First light for the ESO VLT unit telescope 1 occurred during the workshop. ... The image shown (Figure 1 ) here was obtained with the VLT on May 16, 1998, in red light (R band), i.e. while the mirror was still uncoated. ... In this diagram (FIgure 2), the measured image quality of the VLT UT1 astronomical images is plotted versus the ``seeing", as measured by the Seeing Monitor, a small telescope also located on top of the Paranal Mountain. ...

Magnetic field measurements onboard the Interball Tail spacecraft are carried out by the FM-3I instrument which consists of two flux-gate magnetometers covering two different ranges: [-200, +200] nT and [-1000, +1000] nT. Besides scientific goals, the FM-3I experiment data is used to perform the attitude control of the Interball Tail spacecraft. ... August 22, 1995 . ... October 18, 1995 . Top of the page . ... Back to the Interball Home Page . ...

... Using the uvby -photometry and proper motion data for about 5500 F stars within 80 pc from the Sun, we have studied velocity ellipsoid parameters and obtained the following results. 1) The sizw of all wllipsoid semiaxes increase systematically for groups of stars with the decrease of both temperature (at constant metallicity) and metallicity (at constant temperature). ... As a result, each of the three parameters - temperature, metallicity and velocity dispersion - is an age indicator. ...