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1. Standard Magnitudes and Colours
... Standard magnitudes can only be computed for the U, B and V filters and hence the only standard colours that can be calculated are U-B, B-V and U-V. An important point to note, is that these standard colours can be computed using the following instrumental colours - U-B, B-V, U-V, (UVW1-U), (UVW1-B), (UVW1-V), (UVW2-B) and (UVW2-V). Omsrclistcomb computes all possible standard magnitudes for each of the U, B and V filters and displays them in a vector column. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/omsrclistcomb/node5.html -- 4.6 Кб -- 16.08.2005
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2. http://zebu.uoregon.edu/1998/ph162/hw3c.html
... Questions: . ... Find some information on the design and potential of the Advanced Gas Turbine. ... Find some information on the frequency and amount of oil spills which occur in the world's oceans in a given year. ... We don't care how many you get correct. However, of the questions there, explain which one had an answer that most surprised you and how should that answer affect our future policies? ... Find some information about the history of Dam failures in the US and Canada since 1900. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1998/ph162/hw3c.html -- 4.2 Кб -- 12.05.1998
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3. Initial ``fixes'' to millimetre data
... The next step after loading is to apply a number of ``fixes'' that are important for 3-mm data. ... By default atfix applies the ``standard'' gain/elevation model for the antennas. ... As mentioned above, the ATCA uses the chopper wheel method to measure an above atmosphere system temperature. ... On the night of an ATCA reconfiguration, a solution for the antenna positions is derived. ... Task atfix corrects the data for an improved antenna location solution via the dantpos parameter. ... ATFIX . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node209.html -- 9.8 Кб -- 10.04.2016
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4. Observatory Support FAQ List
Observatory Support . ... The science header keyword ORIENTAT is populated by adding the angle between the HST V3 axis and the detector Y axis to what we will call the "commanded roll" (North to V3 through East). The V3-detY angles that were relevant at a given observation's epoch are given as a header keyword (beta_2) in the Observation Log files (aka jitter files). ... The commanded roll and the jitter file's ROLL_AVG should agree to within 0.05 degrees, usually better than 0.02deg. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/observatory/faq.html -- 8.6 Кб -- 20.02.2002
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5. Source Tree Checklist
... As an initial overview, here are the important steps in creating a skeletal Gnome source tree. ... Create a toplevel directory to hold all the components of your application, including build files, documentation, and translations. ... The po directory holds the translation files; gettextize will also create a file called po/Makefile.in.in , used to build the translations. Create a file called po/POTFILES.in listing source files which should be scanned for strings to translate. ... configure.in ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/~satr/GGAD/z68.html -- 10.1 Кб -- 12.07.2000
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6. Instructions for Authors
... 30, 2006 . ... If you retrieve these files via a Web browser, please note that you need to use the browser's "Save As..." facility. ... Figures must be provided as Encapsulated PostScript files and should be incorporated in your contribution using the standard Latex2e "graphicx" package as demonstrated in the demo file author.tex. ... Please submit the LaTeX source file of your contribution, and PostScript/PDF files of any figures, via email (!!!) to Iris Bronnert ( ibronner@eso.org ). ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~hukaufl/di_proc.html -- 8.6 Кб -- 21.08.2006
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7. PINTofALE Threads for Chandra
We provide below examples of ways to generate simulations of Chandra spectra using PINTofALE . ... cut 'n paste "threads" that walk through a specific simulation example, following all the steps with extensive comments; .par file scripts that can be run to do all the work at once. ... Cycle 09 Grating RMFs/ARFs . Note: At the time of writing, the HRC-S/LETG grating ARF files from the Cycle 09 page were incompatible with IDL. ... Simulation for Chandra ACIS-I . ... Simulation for Chandra LETGS . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PINTofALE/doc/CHANDRA_threads.html -- 4.3 Кб -- 01.10.2012
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8. mode conversion
Investigation of linear and nonlinear mode conversions in inhomogeneous plasma and finding of new effects of the principal importance including the following: . ... the higher harmonics generation under the electromagnetic wave interactions with the inhomogeneous plasma in the plasma resonance layers presence (together with V.E.Zakharov, N.S.Erokhin); this effect was confirmed experimentally and it is important, in particular, for a plasma diagnostics; . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mss04/s2.htm -- 2.9 Кб -- 04.03.2004
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mss04/s2.htm -- 2.9 Кб -- 04.03.2004
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9. Getting Started in Actor Prolog. Oil Production.
In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/Lab144/start/e_oil.html -- 12.2 Кб -- 24.09.2007
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10. Simple Universe
... What is an intelligence or an intelligent life? ... Various particular cases, new regimes, original approaches etc. being attractive as they could, all this is a pale shade of a real process of cognition. ... May an infinitely complicated object be indeed so simple? ... An intelligence could not arise in an infinitely complicated universe! ... There are two possibilities: whether our imagination of infinitely complicated object is incorrect or the surrounding world is not infinitely complicated. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~lipunov/text/ashkl/node5.html -- 8.2 Кб -- 14.02.2001
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11. Arecibo Observatory L-Wide Band Receiver
... L-Wide . ... Receiver History . ... Available Filters: . ... Use with e.g. filter 5) NOTE 2 1120-1220 3 1230-1470 4 1550-1820 5 1100-1800 6 1360-1470 7 1320 hipass NOTE 8 1180-1280 9 1280 hipass (ext Output unit. ... Consequently, the calibration for data collected using the hipass 1320 and the hipass 1370 filters only will be mis-calibrated (i.e. by using the opposite polarisation calibration data). ... It is now possible to select any bandpass filter that is not in the 1320 hipass band. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/RXstatus/Lwide/Lwide.shtml -- 22.8 Кб -- 03.02.2013
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