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http://www.stecf.org/documents/isr/ISR_NGST_2002-04.pdf.
http://www.stecf.org/documents/isr/ISR_NGST_2002-04.pdf.
1. imrm
... User Guide ] Task: imrm Purpose: Compute rotation measure image from position angle images Categories: image analysis IMRM computes rotation measure and zero wavelength position angle images from at least 2 position angle images at different frequencies. ... Key: in Up to 5 input position angle (positive N -> E) images (in degrees) at different frequencies. ... Default is 0. ... The default is no output RM images. ... This is also true if you give IMRM position angle images at two frequencies only. ...
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Ссылки http://www.atnf.csiro.au/computing/software/miriad/doc/imrm.html -- 10.6 Кб -- 10.04.2016
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2. http://www.naic.edu/~phil/ter/terfoc.html
... connection points . ... The point P3 is the connection between the horizontal and vertical actuators and is the axis of rotation for the tail gunner motion. processing: survey/020204/reduc We can compute P3,P5 (the moveable points) in dome centerline coordinates if we have the actuator distances and we know the positions of the above connection points in dome centerline coordinates for a given position of the tertiary (say the nominal focus position).(see actuator distances to dome centerline ). ...
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Ссылки http://www.naic.edu/~phil/ter/terfoc.html -- 11.5 Кб -- 04.08.2002
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3. Hypercat help
A celestial position may be passed in different coordinate systems (B1950, J2000 or Galactic) or can be the position of an object. coordinates: The first letter of the string may be used to specify the coordinate system. ... Equatorial coordinates may be passed in decimal or sexagesimal "free" format. ... To precise it is the position of an object in NED or in Simbad, it may be written: ned:M81 or simbad:M81 Valid examples: 121314+122025 , B1950 position (default is B1950 if no system is given) . ...
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Ссылки http://www.sao.ru/fetch/HL/help/Hcoofo.html -- 3.1 Кб -- 23.12.2013
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4. The AstroStat Slog Blog Archive different views
... Archives . ... If you do not mind the time predictor, it is hard to believe that this is a light curve, time dependent data. ... It?s hard to say this data set is designed for time series analysis apart from the complication in statistical inference due to measurement errors. How to design the statistical study with measurement errors, huge gaps in time, and unequal time intervals is complex and unexplored. ... The following is R output without measurement errors. ... Chandra Blog . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2009/filters-are-differen/index.html -- 23.8 Кб -- 01.03.2014
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5. Administrative Newsletter
Bruce Garrett joined the Institute as a Software Systems Engineer in the Engineering and Software Services Division/ Support Services Team on January 3, 2000. ... Joy Hale assumed the position of Senior Systems Administrator in the Computing and Information Services Division on January 3, 2000. ... Stefi Baum assumed the position of Head, Engineering and Software Services in the Engineering and Software Services Division on January 3, 2000. ... Submitted: 3/22/2000) ...
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Ссылки http://www.stsci.edu/brc/Newsletter/Mar_00/aura.html -- 10.9 Кб -- 24.03.2000
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6. harak_e
The beam pattern and the polarization characteristics . of the radio telescope RATAN-600 . The Mueller matrix elements was computed via formulas [1]: . ... The BP were computed by the aperture method, proceeding from the fild distribution in the aperture of the primary mirror. The components of the main and cross-polarization components of the electric field in the vertical aperture of the primary mirror was computed in Frenel diffraction approximation. ...
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Ссылки http://mavr.sao.ru/hq/len/harak_e.htm -- 11.5 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/len/harak_e.htm -- 11.5 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/len/harak_e.htm -- 11.5 Кб -- 24.02.2010
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/len/harak_e.htm -- 11.5 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/len/harak_e.htm -- 11.5 Кб -- 24.02.2010
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7. Lunar equatorial positions. Explanations for Computer Ephemeris.
. Computer Ephemeris. Lunar equatorial positions. Explanations. Each row contains at 0 h and 12 h of Time Dynamical Terrestrial: month, day, apparent right ascension (hours, minutes, seconds), apparent declination (degrees, minutes, seconds of arc) and geocentric distance (in Earth's radii).
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Ссылки http://space.univ.kiev.ua/ephem/exp/Mo1.html -- 1.8 Кб -- 16.10.2004
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8. Wavelength dependence
... The first task assumes the searching for chemical composition and sizes of particles which give the wavelength dependence of the extinction efficiencies close to the observed dependence of . Figure 7: Wavelength dependence of the extinction efficiency factors for homogeneous spherical particles of different sizes consisting of astronomical silicate and amorphous carbon. The dashed segment shows the approximate wavelength dependence of the mean galactic extinction curve at optical wavelengths. ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node3.html -- 15.8 Кб -- 19.11.2010
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9. http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Grim/OLD/grim/dither.txt
... If you have centered the object on the chip the pattern will put the object in each of the 4 quadrants of the chip. ... They are the offset in arcseconds for the x and y inst plane offset, the exposure time in seconds, and the number of exposures at each position. ... A point about offsets should be made here. The dither program uses absolute instrument plane offsets, so you should use object plane offsets to center up on the chip so that the script starts from where you centered up. ...
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Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Grim/OLD/grim/dither.txt -- 4.3 Кб -- 21.08.2003
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10. Calculating the Position and Velocity Components of HST
... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/aket.html -- 12.3 Кб -- 03.11.2000
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11. Short Abstract; Mar. 1995 CONPAS workshop
Modern requirements stipulated for the Networking Technologies . Brief Review of the problems under solution. ... Distributed Collapsed Back Bone Technology Advantages and shortcomings of different approaches. Switches against routers. ... Position at the IS market. Position of the modern high-speed technologies. ... Review of switching technology. Review of the switch market.Classification of switches. ... Big corporate networks implementing switching and routing technologies. ...
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Ссылки http://www.iki.rssi.ru/CONPAS/Mar95a.html -- 2.7 Кб -- 13.11.1995
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12. (Untitled)
... There is an opportunity to perform O-C calculations for objects which are absent in the data base of the package. Such objects can be described by orbital elements or by initial coordinates and velocities. ... 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. ... For example, the designations of objects in the list can occupy the last position in each line. ...
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Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user69lv.htm -- 4.0 Кб -- 10.04.2016
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13. http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/readme_Aperplates
... Q 12.649 0.523 0.342 -0.108 4444 -4.647 -4.582 "n6231_ 178" 16 53 48.63 -41 51 54.1 J2000.0 ! ... A few lines are then added to the top (see readme_asc2dxf for details) to produce input for asc2dxf :in.coo: n6231cp6.dxf slot line 2.00 43.00 9.00 43.00 point 9.773 19.026 n6231 _ 171 Q 12.649 11.236 57.382 n6231 _ 178 I 14.533 ... the output of this program is as follows :n6231cp6.dxf: 0 SECTION 2 ENTITIES 0 CIRCLE 8 1 62 3 10 43.00 20 43.00 30 0.000 40 43.00 0 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/readme_Aperplates -- 3.0 Кб -- 14.02.2001
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14. StarCalc Home Page [English]
Russian version of HP . ... StarCalc is the fastest professional astronomy planetarium & star mapping program for Windows 9x/ME/NT/2000/XP (StarCalc version for PocketPC computers you can found here ). ... Extensibility : This program is based on common "Plugin StarCalc interface to catalogs and object groups", which allows program to add new modules as Plugins. ... Welcome to the Pocket StarCalc Home Page: . ... Some bugfixes in eclipses" and line" plugins - see the new versions in downloads page. ...
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Ссылки http://www.m31.spb.ru/StarCalc/ -- 12.1 Кб -- 27.12.2004
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15. http://www.gao.spb.ru/english/personal/malkin/publ/zm09c.pdf
... Several analysis strategies for computation of systematic part in the radio source velocities can be used: a) estimate source position and velocities from global solution, then fit spherical harmonics to the velocities (Gwinn et al. 1997); b) compute the coefficients of spherical harmonics as global parameters (MacMillan 2005; Titov 2008); c) compute velocities from position time series, then fit spherical harmonics to the velocities. ... Time series statistics is shown in Table 1. ...
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Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm09c.pdf -- 51.4 Кб -- 07.09.2009
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16. HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)
hstpolima -- Reduce linear polarization data for HST instruments . ... Name of STSDAS table file giving the parameters for polarization determination for the instrument corresponding to the input images. ... The upper limit on the polarization error (%) for data to be included in the output files. Pixels in output images with polarization error greater than errlim have the values set to zero in all the output images. outroot = "" [name] . ... outroot + poler - error on linear polarization (%) . ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/hstpolima.help.html -- 12.2 Кб -- 06.06.2006
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17. ET-4R The set of extension tubes
. home . product . gallery . contact .
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Ссылки http://www.astrosib.ru/ac_et-4r.html -- 3.0 Кб -- 15.05.2015
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18. Sample Identification
Next: Identifications and Efficiency Up: THE DEEP X-RAY RADIO Previous: Source Classification . ... For some sources which did not have NVSS positions before the time of optical observations, arcsecond positions from the Texas survey (Douglas et al. 1996) and NED (typically based on VLA data) were used. ... All X-ray/radio sources without counterparts on the survey plates were imaged at either the KPNO 0.9m or the CTIO 0.9m telescopes. ... Previously Identified Sources . Sample Properties . ...
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Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node7.html -- 8.0 Кб -- 03.12.2003
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19. SCL Sfit SYN Commands
... synth : find optimum fit by adjusting abundances v turb , v sin i , and v rad . ... syn_... <p1> <p2> : Initialise parameter for synth . syn_vturb <vturb> [<dv>]; Initialise v turb (km/s) for a fit using synth (default 5) . ... abundance <elid> <abun> <dabu> : Initialise abundances for synth . ... General remarks on the initialisation of abundances in synth A solar abundance will be assumed for any elements not specified. ... Initialise abundances and microturbulence for synth (obsolete) . ...
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Ссылки http://star.arm.ac.uk/~csj/software_store/guide/scl_syn.html -- 8.0 Кб -- 30.08.2007
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20. Dynamic HTML in Communicator
Contents] [Prev page] [Next page] [Index] . Navigator 4 from Netscape, which is part of the Communicator product suite, includes three new areas of functionality that taken together give you Dynamic HTML. The three components of Dynamic HTML are style sheets, content positioning, and downloadable fonts. Used together, these three components give you greater control over the appearance, layout, and behavior of your web pages. ... Introducing Downloadable Fonts . ...
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Ссылки http://crydee.sai.msu.ru/~vab/html.doc/dhtml/dynhtml/intro.htm -- 7.8 Кб -- 13.08.1997
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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