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1. 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 ...
[ Сохраненная копия ]  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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2. RGS Related CAL Routines
Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents . ... The CAL functions CAL_getBadPixelList & CAL_getBadPixelMap use the CAL state variable temperature only to check that the current operating temperature is consistent with the CCF constituent BadPix . ... Used CAL State Variables . List of CCF Components used . ... Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents Michael Smith 2011-09-20 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node252.html -- 25.8 Кб -- 20.09.2011
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3. UV Variables
... A Miriad uv dataset is composed of a collection of items and ` u-v variables'. The variables are parameters that are known at the time of the observation, and include measured data, and the description of the observation set up ( e.g. correlator set up and observing centres). Table B.1 gives a list of the items that are used to build up a Miriad uv dataset. ... integer . ... antenna gain table . ... number of feeds on each antenna . ... frequency set up description table for `bandpass' . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/progguide/node60.html -- 7.1 Кб -- 05.02.2013
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4. OYSTER Lab
Fringe parameters are the complex visibility, the squared visibility amplitude, and the total count rate. These can be computed from bincounts using the functions fringevis , fringevissq , and fringenphot . v=fringevis(bincounts(1,*,*,*)) . ... Instead of computing the modulus of the complex visibility, we use a different estimator for the squared amplitude. ... I have verified with simulated fringe frames that this procedure results in the correct squared visibility amplitudes. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/lab/params.html -- 5.0 Кб -- 26.11.2007