Next: Indirect Parameter Input Up: The User Interface Previous: Miriad on the World . ... The mirbug command can be used if you encounter a bug, have a question about a task, or have a suggestion. ... Use the name `` general '' if the bug report is not about a specific task. The mirbug command places you in an editor (given by the EDITOR environment variable), with a template of a bug report, which includes the parameters most recently used for that task. ... Miriad manager . ...

Еще в разделе: (Показать все результаты (>16706) - www.atnf.csiro.au/ )

• Cosmological Parameter Survey Using the Gravitational Lensing Method
• Telescope Parameters and Search Strategy
• Task parameter manipulation

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... yes . data-set . EPIC PN raw events data-set . ... boolean . ... Accuracy of gain/cti correction . ... yes, if ``out-of-time events'' file should be created instead of ``normal events'' file (only meaningful for IMAGING modes) (considered as experimental ) . ... yes, if special soft energy function should be included in the long-term CTI corrections (considered as experimental ) . ...

Еще в разделе: (Показать все результаты (>14047) - xmm.vilspa.esa.es/ )

... HST . How precise are the parameters of my double star as measured in Transfer Mode? ... Data . ... HST Peer Review Process . ... HST Overview . Overview . ... Retrieving HST Data . ... Data Analysis . ... HST Science Year in Review . ... FGS Data Handbook . ... A: Analysis of calibration and other data has shown that the separations obtained in the analysis the Transfer Functions of double stars have a precision of around 1 milli arc-second. ...

Еще в разделе: (Показать все результаты (>13677) - www.stsci.edu/ )

• CCD Parameters table
• Surface Brightness Parameters from Deconvolved PC Images of Elliptical Galaxies
• Ferrarese Ford: Surface Brightness Parameters from Deconvolved Images

... 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 . ...

Еще в разделе: (Показать все результаты (>515) - www.apo.nmsu.edu/ )

• TUI:Scripts:Scripting Tutorial:Loops
• Echelle for Beginners

The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...

Еще в разделе: (Показать все результаты (>5994) - www.arcetri.astro.it/ )

• Program parameters
• Where are the tunable parameters of the kernel?
• Kernel tunable parameters

... The instrument modes and arms should be indicated and described, and the keywords that distinguish between different modes should be indicated (usually INS.MODE is used if it is a mode and OCS keys are used in case it is related to an arm). ... Raw frames The format of the raw frames for each mode and arm should be described. ... The design should be checked on pre-processing or processing, which involves products only (no trigger via raw frames). ... QC parameters. ...

Еще в разделе: (Показать все результаты (>4449) - www.eso.org/ )

• Preparation of parameter file
• CONSTRICTOR parameters for astrometric reductions
• Parameters

1.2 CCD Operations, Performance Parameters, and CCD . Transfer Curves . Low-light-level CCD performance parameters are grouped into four primary CCD operations: 1) Charge Generation (e.g. QE), 2) Charge Collection (e.g. MTF), 3) Charge Transfer (e.g. CTE), and 4) Charge Detection (e.g. Read Noise). ... Four Basic CCD Operations and Associated Performance Parameters and CCD Transfer Curves Used to Measure Performance . ... Charge Transfer Performance Parameters and CCD Transfer Curve Tests . ...

Еще в разделе: (Показать все результаты (>1820) - www.sao.ru/ )

• Documentation: LEDA: parameter: m21c
• Saving and Loading Session Parameters
• Mean astrophysical parameters from LEDA

... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...

Еще в разделе: (Показать все результаты (>1859) - hea-www.harvard.edu/ )

• Editing Files and Parameters
• Listing and Printing Files, Parameters, and Tables
• Model Spectra for Spectral-Fitting Program

... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Nuclear activity and environment Effect of environment on AGN is not completely clear yet. ... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Effect of the mass Mass slices ­ optical and radio AGN overall interaction one-on-one interaction relative location 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Stratified study Stratifed study that considers several strata of mass. ...

Еще в разделе: (Показать все результаты (>1255) - www.mrao.cam.ac.uk/ )

• Command line interface to libAIR and water vapour column retrieval Bojan
• De-convolution of a Gaussian beam from planetary observations Bojan Nikolic web
• Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the

... 5 1/ 2 Closing the feedback lo op: 1st option · Feedback efficiency 2NepEep f = Lp 4 3 w1 R 3 E1 w2 c E2 ( Eep E1 if E1 E2) · Pair pro duction rate Nep = · Soft (synchrotron from secondary pairs ) photon field: Eep 2 eB E2 1/2 f w w b , w2 = Es = 4 Es 2 mec2 mec · Hard ( inverse Compton from primary pairs ) photon field: 2 2 wb 3 R w1 , E1 = 3 2Ts wb = 4 R T ct 0 0 mec2 wb is thermal background energy density ...

Еще в разделе: (Показать все результаты (>200) - hea.iki.rssi.ru/ )

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

Еще в разделе: (Показать все результаты (>324) - www.ssau.ru/ )

Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...