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1. Important Notes - Please check these
Next: Links to Manual Sections Up: Contents Previous: Contents Contents . ... All VLBA stations have two RDBE units for a total of 8 channels with the DDC. ... SCHED knows how to set up the details for most observations at most stations. ... Please see the discussion of the input parameter PRECDATE . ... Please note that all setup files intended to be used for spectral line observations using DOPPLER must have all channels distinguished, in the setup file, by frequency and polarization. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/Important_Notes_Please_chec.html -- 7.3 Кб -- 10.04.2016
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2. Thermodynamics
The First Law (1): Energy is Conserved in a closed system: . ... We usually consider work and heat flow as the two kinds of energy . The Second Law (2): The Law of Entropy: . ... The amount of disorder increases . ... You can not go from a disordered system to an ordered system without inputting more energy (this is the most important attribute of the second law) . ... In no way can we recover work of that this disordered system without putting energy into the system. ... More on Thermodynamics . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1999/ph162/l3.html -- 7.1 Кб -- 14.09.1999
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3. Subtracting models from unsaturated WFPC2 PSFs
Here are some suggestions for subtracting Tiny Tim models from unsaturated WFPC2 PSFs. ... The undersampling of the WPFC2 cameras results in the observed PSF being highly dependent on positioning at the subpixel level. A subsampled model should be generated, shifted to match the proper positioning of the observed PSF, and then rebinned to detector sampling. ... The PSF models will never be perfect matches to the observed ones, and they will likely be too symmetrical. ... Figure 1. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/software/tinytim/subpsf.html -- 4.0 Кб -- 02.04.2001
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4. http://www.astro.louisville.edu/software/archive/colorspec/colorspec-1.0/README
Programs to generate color spectra ================================== These programs were developed to produce realistic color spectra from digital data. ... The distribution here contains the original source code for colorspec and solar in C, and a version of solar written in Fortran. ... It will produce a color spectrum of any digital spectrum. ... The 800x50 image solarflux.ppm was generated by colorspec and the file fluxatlas.dat, a reformatted NSO Solar Flux Atlas in the data directory. ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/archive/colorspec/colorspec-1.0/README -- 4.8 Кб -- 23.08.2004
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5. httxt2dbm - Generate dbm files for use with RewriteMap - Apache HTTP Server
... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Programs . Available Languages: en | ... httxt2dbm is used to generate dbm files from text input, for use in RewriteMap with the dbm map type. ... f DBM_TYPE . ... Available types are: GDBM for GDBM files, SDBM for SDBM files, DB for berkeley DB files, NDBM for NDBM files, default for the default DBM type. -i SOURCE_TXT . ... Name of the output dbm files. httxt2dbm -i rewritemap.txt -o rewritemap.dbm . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/manual/de/programs/httxt2dbm.html -- 8.1 Кб -- 21.01.2013
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6. Spatial Structure of NGC 6822: An Example for Statistical Modeling of
... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/pasztorl2.html -- 11.0 Кб -- 03.11.2000
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7.