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http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol1/node43.html.
http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol1/node43.html.
1. Conditional Statements, Branching
Next: Special Functions Up: MIDAS Command Language Previous: Local Keywords . As in FORTRAN 77 any of the following forms of the IF statement may be used: IF log_exp command ! ... If we do WRITE/KEYWORD INPUTC beer . ... N "Enter number: " . ... WRITE/KEYWORD INPUTC NONE ! ... WRITE/KEYWORD INPUTC YES !indicate, that INPUTI holds a valid number . ... Since, in the ELSE branch we know that parameter P6 is given, the default value " + " itself is never tested against the interval [22,1024]. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol1/node43.html -- 9.8 Кб -- 23.02.1996
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2. Host Command-Line Interface
Next: Writing Shell Scripts Up: The User Interface Previous: Indirect Parameter Input . Miriad tasks can always be run by specifying their parameters on the host command line. ... For example, out=gauss sets the parameter out to the `value' gauss . ... Next, we will run a histogram task, histo , with the input image dataset gauss that we just created: % histo in=gauss . ... The command-line interface is quite appropriate for tasks that take relatively few parameters, or in shell scripts. ...
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Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node19.html -- 7.9 Кб -- 10.04.2016
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3. 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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4. sfit help file
... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...
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Ссылки http://star.arm.ac.uk/~csj/software_store/guide/sfit2_help.html -- 7.6 Кб -- 18.10.2004
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5. Example of debugging a shell script
To print commands and their arguments as they are executed: cat example #!/bin/sh TEST1=result1 TEST2=result2 if [ $TEST1 = "result2" ] then echo $TEST1 fi if [ $TEST1 = "result1" ] then echo $TEST1 fi if [ $test3 = "whosit" ] then echo fail here cos it's wrong fi . This is a script called example which has an error in it; the variable $test3 is not set so the 3rd and last test [ command will fail. Running the script produces: example result1 [: argument expected . ...
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Ссылки http://comet.sai.msu.ru/UNIXhelp/scrpt/scrpt2.8.1.html -- 2.7 Кб -- 17.01.1997
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6. 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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7. http://www.naic.edu/~emuller/icred
Some Documentation for the IDL ICRED . ... This is the system which recieves all command inputs. it decodes inputs and selects tasks, parses parameter inputs and also runs the 'go', 'list' and 'help' commands. It does no error checking, for example to see if the parameter inputs are sensible (e.g. it does not check if an x-range has been entered as 'chicken', rather than a more understandable range of say 10,20). 2) the task decoders: icred_<taskname>.pro . ... Other tasks or important commands: . ...
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Ссылки http://www.naic.edu/~emuller/icred -- 8.4 Кб -- 21.10.2004
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8. Supernova 1994D and the Unexpected Universe
Astronomy Picture of the Day . ... 31.05.2015 . ... Credit Copyright: High-Z Supernova Search Team , HST , NASA Explanation: Long ago, far away, a star exploded. Supernova 1994D , visible as the bright spot on the lower left, occurred in the outskirts of disk galaxy NGC 4526 . Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... Publications with keywords: supernova - cosmology . ... A Supernova through Galaxy Dust . ...
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Ссылки http://www.astronet.ru/db/xware/msg/1337347 -- 16.2 Кб -- 11.10.1972
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9. http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_yaming_timeseries.ps
Detecting Variations in Source Intensity for Poisson Data Y. Yu, XL. Meng, D. van Dyk, V. Kashyap, and A. Zezas Abstract The analysis of light curves is an especially challenging statistical task for low-count Poisson data: Variation in the source intensity may be shadowed by the Poisson variation of the counts. Here we discuss a class of statistical models that are designed to capture trends and autocorrelations in Poisson data that are collected over time. ... Example: A downward trend? . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_yaming_timeseries.ps -- 191.6 Кб -- 13.09.2004
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10. http://www.eso.org/~qc/dfos/config/fitsreport_raw.cfg
... TO DISPLAY #------------------------------------------------------------------------------------------------------------------- Parameter Name : OBS.PROG.ID Header1 : PROG_ID Type : string Value Format : %-13s Start : 1 End : 13 Parameter Name : OBS.ID Header1 : OBS_ID Type : integer Value Format : %-10i Start : 1 End : 10 Parameter Name : OBS.TARG. NAME Header2: TYPE Type: string Value Format: %-17s Parameter Name: DPR.TECH Header1: . ...
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Ссылки http://www.eso.org/~qc/dfos/config/fitsreport_raw.cfg -- 5.2 Кб -- 04.12.2006
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11. APOD: 2015 May 31 - Supernova 1994D and the Unexpected Universe
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2015 May 31 . Supernova 1994D and the Unexpected Universe . Image Credit: High-Z Supernova Search Team , HST , NASA . Explanation: Long ago, far away, a star exploded. ... Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... About APOD | ...
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Ссылки http://www.sai.msu.su/apod/ap150531.html -- 6.2 Кб -- 10.04.2016
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12. APOD: December 30, 1998 - Supernova 1994D and the Unexpected Universe
... December 30, 1998 . Supernova 1994D and the Unexpected Universe . Credit: High-Z Supernova Search Team , HST , NASA . Explanation: Far away, long ago, a star exploded. ... Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... The large number and great distances to supernovae measured in 1998 have been interpreted as indicating that we live in a previously unexpected universe . ... About APOD > . ... NASA Technical Rep.: ...
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Ссылки http://www.sai.msu.su/apod/ap981230.html -- 5.2 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/sn94d_hiz_big.html -- 5.1 Кб -- 02.02.2001
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[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/sn94d_hiz_big.html -- 5.1 Кб -- 02.02.2001
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13. Computing dispersive atmospheric delay with AATM Bojan Nikolic web pages (r.
... Bojan Nikolic web pages (r. 329) . ... Atmospheric Modelling for ALMA . This is a short and simple illustration of how to use (A)ATM to calculate the dispersive path delay introduced by the atmosphere as well as the non-dispersive parts. ... Compute dispersive delay in the atmosphere This program is part of AATM version 0.06 GPL license -- you have the right to the source code. ... Computing dispersive atmospheric delay with AATM . ... Computing atmospheric absorption with AATM . ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/alma/aatm-dispersive.html -- 9.0 Кб -- 04.04.2016
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14. Access via e-mail
... The e-mail interface of the CATS is designed like CGI for the call of the basic procedures: select and match from the html-forms and the program is a lexical analyser, distinguishing keywords and parameters from the electronic letter sent to the address `cats@sao.ru'. ... The output of result is forseen in the same formats as in other forms of the access to the CATS. ... out[put] < arg1 arg2... > . ... ra [ < arg1 > ] < arg2 > < arg3 > ... min max [center] . ... window < arg1 arg2 ... > . ...
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Ссылки http://mavr.sao.ru/hq/vch/Publications/Eng/html/adbis97/node7.html -- 8.4 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/vch/Publications/Eng/html/adbis97/node7.html -- 8.4 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/adbis97/node7.html -- 8.4 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/vch/Publications/Eng/html/adbis97/node7.html -- 8.4 Кб -- 11.09.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/adbis97/node7.html -- 8.4 Кб -- 02.10.2012
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15. Sun orbital parameters for Computer Ephemeris for 2014 (DE200/LE200).
Computer Ephemeris for 2014 from DE200/LE200. Orbital parameters of the Sun. Date Mean Perigee Mean Paral Aberrat Epsilon Nutat longitude longitude anomaly Dec 24 272.6887 283.1787 349.5100 8.941 20.832 2326 6.72 -8.19 Jan 3 282.5451 283.1792 359.3660 8.943 20.837 6.71 -8.18 13 292.4016 283.1796 9.2220 8.942 20.834 6.76 -8.11 23 302.2581 283.1801 19.0780 8.935 20.818 6.87 -7.99 Feb 2 ...
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Ссылки http://space.univ.kiev.ua/ephem/14a/Su4.html -- 5.4 Кб -- 15.10.2013
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16. I Expected More Sense Than That. - an Astronomy Net Exploration Forum Message
Astronomy Discussion Forums . ... I Expected More Sense Than That. ... Post Message | ... Posted by Richard D. Stafford, Ph.D. on November 8, 2002 04:14:05 UTC . ... You are missing the point - harvey1 - November 8, 2002 - 13:10 UTC . I hope Stafford doesn't mind my intruding his forum - mrsouza - November 8, 2002 - 14:55 UTC . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
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Ссылки http://www.astronomy.net/forums/exploration/messages/155.shtml -- 15.4 Кб -- 09.04.2016
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17. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . ... Installation of the ground receiving station on the premises of M.V. Keldysh Institute of Applied Mathematics, the Russian Academy of Sciences, software upgrading to receive the information signal from board the ISS RS. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
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Ссылки http://www.energia.ru/en/iss/researches/techn/60.html -- 25.6 Кб -- 10.04.2016
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18. Stellarium: CLIProcessor Class Reference
Stellarium 0.12.3 . ... Classes . ... ClassљList . ... Static Public Member Functions . CLIProcessor Class Reference . ... argsGetOption (const QStringList &argList, QString shortOpt, QString longOpt) . Check if a QStringList has a CLI-style option in it (before the first ). ... Retrieve the argument to an option from a QStringList. ... Check if a QStringList has a yes/no CLI-style option in it, and find out the argument to that parameter. ... a long-form option string, e.g. "–help" . ...
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Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classCLIProcessor.html -- 17.8 Кб -- 28.02.2014
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19. IDL programs
MAKING THE PROFILES . First of all you are expected to load a FITS file ("FILE"-"LOAD"). ... By pressing the middle button you copy the profile from the first profile window to the second one. ... An example: first integral can correspond to the profile of active region and second integral can correspond to the profile of quiet chromospheric region. ... The second profile (which is subtracted from the first one) you extract after clicking on "SUBTRACT"-"MARK QUIET PROFILE" and marking the region. ...
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Ссылки http://lnfm1.sai.msu.ru/~kupry/SOFTWARE/xlook.html -- 6.9 Кб -- 15.01.2004
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20. Mirror Controller Actor
... The mirrorCtrl mirror controller actor controls one telescope mirror. It accepts desired orientation and commands mirror motion accordingly. ... It is presently designed to command a Galil mirror controller , but one may add support for other low-level motion controllers. mirrorCtrl is written pure Python. ... Home the desired actuators, where actuator list is a comma-separated list of actuator letters A through F (but some mirrors have fewer than 6 actuators). 2.5m M1 valid actuators: A-F . ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/mirrorCtrl/ -- 8.8 Кб -- 02.03.2015
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