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http://ip.rsu.ru/~marsakov/paper6/p6tab2_1.htm.
http://ip.rsu.ru/~marsakov/paper6/p6tab2_1.htm.
1. Increasing number of open files parameter
The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : Tunable Kernel Parameters? . Re : Increasing number of files in system (Simon Cooper) . Keywords: kernel tuning, file handles, Bus error . Date: Sat, 25 Oct 1997 11:25:44 GMT . From: Simon Cooper < simon.cooper@snc-net.demon.co.uk > . Sorry for the typo, my (Linux loader) lilo.conf entries are: . image=/vmlinux.safe [Newline] label=LinuxS [Newline] root=/dev/hda2 [Newline] .
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Ссылки http://www.arcetri.astro.it/irlab/library/linux/khg/HyperNews/get/khg/59/2/1.html -- 2.6 Кб -- 23.03.2000
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2. Maximum number of sources.
... It may be desirable to apply (in addition to the source selection described above) some definite upper limit to the number of sources to be plotted - say, to plot only the first 50 brightest sources. Such a limit may be difficult or impossible to achieve solely by use of the expression parameter. ... produces a ds9 region file containing data for the first 10 brightest sources from the SRCLIST table in file `fred.ds' (that is, those 10 sources in the table which have the highest values of RATE ). ...
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Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/slconv/node6.html -- 5.0 Кб -- 10.01.2003
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3. Examples of GHRS Phase II Proposals
Your Phase II Proposal and Using RPS2 . ... Exposure_Number: 1 Target_Name: HD12345 Config: HRS Opmode: ACQ Aperture: 2.0 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: BRIGHT=RETURN, ! ... Number_of_Iterations: 1 Time_Per_Exposure: 13.5S Special_Requirements: ONBOARD ACQ FOR 2 Comments: STEP-TIME = 1.5 sec Exposure_Number: 2 Target_Name: HD12345 Config: HRS Opmode: ACQ/PEAKUP Aperture: 0.25 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: SEARCH-SIZE=5 ! ...
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Ссылки http://www.stsci.edu/instrument-news/handbooks/ghrs/GHRS_24.html -- 10.9 Кб -- 14.02.1996
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4. Fit a source with a small number of net counts
Next: Inspection of results Up: *fit* - Fit Data Previous: Verbose Mode . If the number of net counts for a source is less than it is impractical to fit the data in all 34 energy bits. However, if the flux is required, then a fit must be performed first. ... Fit will then calculate the normalization of the model and xflux can be used to determine the flux and luminosity of the source from the best fit model. xs> fit rebin=yes . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node153.html -- 3.9 Кб -- 01.10.2012
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5. User Parameters - Data Location & Beam Selection CentralProcessor 0.11
... CentralProcessor 0.11 documentation . ... The following parameters determine where the measurement sets are that hold the data to be processed. The default behaviour is to read the MS from the given Scheduling Block (SB) directory. ... Location (on galaxy) of the scheduling blocks. This is used when specifying SB numbers - the default is the standard location for BETA operation. ... These parameters determine which beams in the data to process. ... User Parameters - Pipeline & job control . ...
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Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/BETApipelines/DataLocationSelection.html -- 8.5 Кб -- 12.04.2016
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6. Parameters
Next: System configuration Up: How to use CONSTRICTOR Previous: Preparation of parameter file Contents . ... DayNumber: Even though this number is in the data, some packet headers have the wrong number and it makes it a whole lot easier to have the user check and enter this number correctly. ... CONSTRICTOR will add a multiple of 24 hours to the time tag when the day number changes. Remember to set the StopTime to, say, 48 hours if you use a DayNumber of one less than the actual day number. ...
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Ссылки http://www.eso.org/~chummel/oyster/manual/node229.html -- 7.3 Кб -- 28.04.2015
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7. HyperLEDA documentation: parameter: pgc
All the objects in the database, galaxies, stars, clusters, ..., are indexed with their pgc number. Historically, the pgc numbering was created to unify the names of the galaxies when the database project started in 1983. ... Still, all the objects in the database (about 5 millions) have a pgc number which is used as a unique identification across the different tables. This number should not be used to build a name , since it would not be recognized by any database, including HyperLeda. ...
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Ссылки http://www.sao.ru/fetch/HL/leda/param/pgc.html -- 3.5 Кб -- 23.12.2013
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8. Parameters of the starburst
... We assume that an instantaneous starburst occured in the region of the Galactic center, with half of the stars (in number) being formed in binaries. The total mass of the stars formed during the starburst was taken to be , as indicated by the Tamblyn & Rieke (1993) analysis. ... In fact, the number of stars in IRS 16 estimated by Tamblyn & Rieke (1993) is uncertain within a factor of 2, but this is actually of no importance as long as we only use relative numbers of different X-ray source species. ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/apj/node6.html -- 3.5 Кб -- 21.06.1996
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9. Tutorial on Fortran 90, Digital UNIX
System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...
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Ссылки http://star.arm.ac.uk/f77to90/alpha.html -- 10.4 Кб -- 13.03.1996
[ Сохраненная копия ] Ссылки http://crydee.sai.msu.ru/f90/alpha.html -- 10.4 Кб -- 13.03.1996
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[ Сохраненная копия ] Ссылки http://crydee.sai.msu.ru/f90/alpha.html -- 10.4 Кб -- 13.03.1996
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10. ATOMS by Number
... Position Switching Separation Tolerance with Arecibo in L-Band . ... Arecibo Elevation Wheel and Track Life . ... Carl Heiles . ... Dynamics of the Arecibo Radio Telescope . ... The Future: Ultra Wide Band Feeds and Focal Plane Arrays . ... 2002-03 (pdf) . ... 2002 May . ... 2001-09.pdf . ... Multi-Beam Array System Feed Selection . ... 2000-07.pdf . ... The LBW Feed: The Mueller matrix in 1999 and 2000 . ... P. Perillat . ... Feed Resonances in Wide L-Band Gregorian Feed . ... J. Cordes, J. Lazio ....
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Ссылки http://www.naic.edu/~astro/aotms/bynumber.shtml -- 22.6 Кб -- 27.02.2014
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11. FTS Dictionary Example
... MAXLEN parameter specifies maximum length of the number considered as a 'good' integer. ... If REJECTLONG = FALSE (default), than dictionary returns prefixed part of integer number with length MAXLEN . ... This is a dict_tmpl.c file. # include postgres.h # include utils/builtins.h # include fmgr.h #ifdef PG_MODULE_MAGIC PG_MODULE_MAGIC; #endif # include utils/ts_locale.h # include utils/ts_public.h # include utils/ts_utils.h typedef struct { int maxlen ; bool rejectlong ; } ...
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Ссылки http://www.sai.msu.su/~megera/postgres/fts/doc/fts-intdict-xmp.html -- 9.6 Кб -- 13.04.2008
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12. (Untitled)
There are six possible ways of object description: . a) by number(s) . ... d) by list . e) by orbital elements . ... They should be introduced as year, month, day with tenth (e.g. 20021104.1). d) Computations are performed for all objects listed in the file whose path and name should be introduced into assigned data field. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ...
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Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user9hdg.htm -- 6.7 Кб -- 10.04.2016
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13. SCL Sfit Genetic Commands
... sfit . ... commands . scl . ... Define parameters for controlling performance of genetic algorithm . ... generations . The maximum number of generations the program will go through, before stopping, if the solution is not within the given tolerance. 10 . ... The number of parents randomly generated in the first generation, and in each subsequent generation. 50 . ... This is multiplied by the number of parameters being varied to give the total string length for each parent. 16 . ... elitism . ...
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Ссылки http://star.arm.ac.uk/~csj/software_store/guide/scl_gen.html -- 7.9 Кб -- 30.08.2007
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14. Model realization and some results
... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...
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Ссылки http://www.astro.spbu.ru/DOP/A-PERC/PAPER2/node4.html -- 10.8 Кб -- 19.11.2010
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15. http://www.mrao.cam.ac.uk/~rachael/compphys/examples/cell_list.f90
... number of particles integer, parameter :: max_list = 100 ! max number of particles per cell integer, parameter :: ncell = 20 ! ... cell size real(dp) posn(3, npart) ! ... initialise cell list call init_cell_list(npart, ncell, max_list, cell_size, posn, & cell_num, cell_list) ! now go and do something interesting with it... contains subroutine init_cell_list(npart, ncell, max_list, cell_size, posn, & cell_num, cell_list) implicit none integer, parameter :: dp = kind(1.0d0) integer npart ! ...
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Ссылки http://www.mrao.cam.ac.uk/~rachael/compphys/examples/cell_list.f90 -- 3.4 Кб -- 30.09.2005
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16. CurveFitter (ImageJ API)
... public class CurveFitter . ... static int . ... Field Detail public static final int STRAIGHT_LINE . ... public static final int POLY2 . ... public static final int POLY3 . ... public static final int POLY4 . ... public static final int EXPONENTIAL . ... public static final int POWER . ... public static final int LOG . ... public static final int RODBARD . ... public static final int GAMMA_VARIATE . ... public static final int LOG2 . ... public static double f (int fit, double[] p, double x) . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/measure/CurveFitter.html -- 34.8 Кб -- 02.12.2010
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17. Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/kearnsk.html -- 12.3 Кб -- 03.11.2000
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18. MARKBACK (Aug99) --- nictools --- MARKBACK (Aug99)
markback -- mark regions in the background for performing statistics on markback association . association . calnicb style association input file with list of images to be processed and co-added. number . labels boxes with numbers on image display . ... Only the first 2 boxes will be used by asncombine. nmem . image in association to use for marking the boxes. markback displays one image of an association (the nmem'th image), and allows the to mark nbox regions on the image display. ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/markback.hlp.html -- 2.2 Кб -- 06.06.2006
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19. what to do with the trace data
... Here is a sample parameter file that is set to plot the B filter trace data. ... One can generally get by with the default graph parameters. input = B.a list of images or list files to be graphed (wx1 = 3000.) left world x-coord if not autoscaling ... autoscaling (wy2 = 100.) upper world y-coord if not autoscaling (wcs = logical ) Coordinate system for images (axis = 1) axis along which projection is to be taken (transpose = no) transpose the x and y axes of the plot (pointmode = no) ...
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Ссылки http://www.apo.nmsu.edu/Instruments/filters/tracehelp.html -- 4.8 Кб -- 22.02.2001
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20. RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, tabl
... Characteristic parameters of subsystems RR Lyrae field stars and globular clusters . ... RR Lyrae . ... 0.05 . ... lim R max , kpc . ... Z o , kpc . ... grad R [Fe/H], kpc -1 . ...
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Ссылки http://ip.rsu.ru/~marsakov/paper7/p7tab1.htm -- 9.9 Кб -- 02.02.2007
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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