... Forum . ... Search . ... Search by User Name User Name: Exact Name: . Find Posts from Last visit Yesterday A week ago 2 weeks ago A month ago 3 months ago 6 months ago A year ago Any date And newer And older Sort Results by Title Number of views Posting date Category Increasing order Decreasing order Jump to Result Number Show 5 Search Results Show 10 Search Results Show 15 Search Results Show 20 Search Results . ... Powered by Kunena Forum . ... MAO NASU . ...

Program: PBCORR Purpose: Corrects maps for primary beam correction Category: MANIPULATION File: pbcorr.shl Author: M. Vogelaar Keywords: INSET= Input set (and subsets). Maximum number of subsets is 2048. ... There is a cutoff in the distance: Outside the validity range, the correction is set to a value depending on OPTION= For WSRT and VLA The cutoff occurs at a primary beam sensitivity of 2.3% of the value at the beam center, i.e. where the Antenna Power Spectrum is equal to 2.3/100. ...

... Sort options Sort by date Sort by citations Sort by normalized citations Sort by author Sort by author count Sort by page (ToC sort) . ... Date . ... Pustilnik, S.; Kniazev, A.; Lyamina, Y.; Tepliakova, A. Dwarf galaxies in the nearby Lynx-Cancer void: photometry, colours and ages . ... Sort by citation count normalized citation count first author name author count date (most recent first) date (oldest first) entry date inverse author count page (ToC sort) . ... Return: Results Form for manual query...

... Study of Mg-Fe-silicate glasses of variable composition. ... With the new data, the astrophysical discussion started in Paper I was continued and focussed on the comparison of the olivine glass data with IRAS LRS spectra of O-rich circumstellar envelopes around Mira stars. ... The new olivine glasses point to the interesting consequence that the temperature for silicate dust grains at the inner edge of circumstellar envelopes must be considerably higher than the values often given in the literature....

... use frames summary class fields routine details file attributes . ... AUTHOR: Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770 craigm@lheamail.gsfc.nasa.gov UPDATED VERSIONs can be found on my WEB PAGE: http://cow.physics.wisc.edu/~craigm/idl/idl.html . PURPOSE: Compute confidence limits for chi-square statistic . ... CALLING SEQUENCE: DELCHI = MPCHILIM(PROB, DOF, [/SIGMA, /CLEVEL, /SLEVEL ]) . ... result = mpchilim( p , dof , sigma= sigma , clevel= clevel , slevel= slevel ) . ...

Next: *search_grid* - Grid of Up: Spectral Analysis Previous: Inspection of results . The results can be displayed graphically: xs> counts_plot observed spectrum [root_obs.tab] rp90 # input is rp90_prd.tab . A plot will appear on the screen, showing data points with error bars, and the predicted model as a histogram when one is present. ... d and s for plots of `observed-predicted' and `(observed-predicted)/error' respectively, and . ... These options are specific to counts_plot. ...

Find Similar Abstracts . ... Hydrodynamics of the universe . ... Fluid Dynamics Transactions, vol. 8, 1976, p. 279-287. ... 00/1976 . ... COSMOLOGY, GALACTIC EVOLUTION, GRAVITATIONAL EFFECTS, HYDRODYNAMICS, UNIVERSE, ASTRONOMICAL MODELS, EXPANSION, FLUID FLOW, NEWTON THEORY, NONLINEAR EQUATIONS, PERTURBATION THEORY . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

... Test harness updated. ... Version 0.3.1 - 2002-07-30 ------------------------ - Changed test harness to use 'cmp' to compare output. Fixed Test 13 Version 0.3 - 2002-07-11 ------------------------ - Updated parameter interface Version 0.22 - 2002-06-11 ------------------------- - Documentation fix Version 0.21 - 2002-05-31 ------------------------ - Updated dependencies (SAS 5.3.3) Version 0.2 - 2002-05-29 ------------------------ - Version number changed for upload to SAS for SAS 5.3.3. ...

NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...

Allows you to specify a drift scan: motion at a constant velocity along a great circle. ... The path starts at the new object position (though the telescope actually intersects the path later, see Subtleties ). ... Note that the units are always /sec for both axes. ... The velocity along the path is 0.01 /sec. ... The path is assumed to start when you hit the Slew button (more precisely, when the TCC parses the command). However, it takes the telescope awhile to slew to meet the specified path. ...

. sort sends its results directly to your screen. To save them to a file use the -o option. For example: sort -o mail addresses . This saves the results of sorting the file addresses in the file mail .