at the computer) . 8 PIN DIN "C" FEMALE at the computer. ... Not connected . ... GND . ... Audio Left . ... Audio Right . Note: Direction is Computer relative Monitor. ...

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• HwB: C16/C116/+4 Audio/Video Connector (Offline)
• HwB: VGA (9) Connector (Offline)
• HwB: ZX Spectrum 128 RGB Connector (Offline)

VGA=Video Graphics Adapter or Video Graphics Array. ... At the monitor cable) . 9 PIN D-SUB FEMALE at the videocard. 9 PIN D-SUB MALE at the monitor cable. Pin . ... RED . Red Video . ... GREEN . Green Video . ... BLUE . Blue Video . ... Red Ground . ... Green Ground . ... Blue Ground . ... Sync Ground Note: Direction is Computer relative Monitor. ...

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• HwB: C16/C116/+4 Audio/Video Connector
• HwB: ZX Spectrum 128 RGB Connector
• HwB: NeoGeo Audio/Video Connector

Name: GRXRGB Purpose: convert HLS color to RGB color Category: GRAPHICS File: pgplot.src Author: T.J. Pearson Use: see description below. Description: SUBROUTINE GRXRGB (H,L,S,R,G,B) GRPCKG: Convert a color specified in the HLS color model to one in the RGB model. ... Arguments: H,L,S (real, input): hue (0 to 360), lightness (0 to 1.0), and saturation (0 to 1.0). R,G,B (real, output): red, green, blue color coordinates, each in the range 0.0 to 1.0. ...

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• http://www.atnf.csiro.au/computing/software/gipsy/sub/grxhls.dc3
• http://www.atnf.csiro.au/computing/software/gipsy/sub/pgshls.dc2
• http://www.atnf.csiro.au/computing/software/gipsy/sub/grsncr.dc3

... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

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• APO 3.5-m Users Mail Servers

... In order to detect sources the program computed the mode of the background, and then any pixel with a value greater than or equal to nsigma * backgound mode is considered to be likely associated with a source. ... Having obtained a source list, comprising their positions, sizes, counts and background counts, aperture-photometry is then performed on each source to produce a count value for each source that is consistent with the CAL calibration procedure. ...

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• strbs: Star Tracker BoreSight calculation

... Gallery . ... Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . Title: Workshops and computer labs . ... Mechanical Workshop, 1944 . Views: 2043 . Mechanical shop, 1944 . Views: 2008 . ... Views: 1930 . ... Views: 2959 . Workshop, 1950s . Views: 2940 . ... Views: 3511 . ... Views: 3697 . Workshop construction . Views: 2947 . ... Views: 2924 . Powered by Gallery 3.0.9 (Chartres) . ...

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• Firedoors on the old spectrograph tunnel/computer room. They worked.
• Bob Shobbrook dressed for a winters night at the control computer for the
• GSAOI Instrument Description Page

makeprfcorr -- Compute the pixel response function for an image created with asncombine makeprfcorr association . association . ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...

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• ALIGNASN (Nov98) --- nictools --- ALIGNASN (Nov98)
• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)

grdgradient - Compute directional derivative or gradient from 2-D grd file representing z(x,y) grdgradient in _ grdfile -G out _ grdfile [ -A azim [/ azim2 ] ] [ -D [ c ][ o ][ n ] ] [ -L flag ] [ -M ] [ -N [ e ][ t ][ amp ][/ sigma [/ offset ]] ] [ -S slopefile ] [ -V ] grdgradient may be used to compute the directional derivative in a given direction ( -A ), or the direction ( -S ) [and the magnitude ( -D )] of the vector gradient of the data. ... If amp is not given, default amp = 1. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/grdfft.html
• http://xray.sai.msu.ru/~ivan/gmt/man/psrose.html

... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...

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• NAOS Real-Time Computer for Optimized Closed Loop and On-Line Performance
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron

Open Systems Handbook: A Guide to Building Open Systems . ... This book is designed to provide interested individuals and organizations with an overview of open systems and the work being done to achieve them. ... This section is organized using a descriptive model of an open systems environment developed by the IEEE PI 003.0 Working Group, which is developing the Guide to POSIX-based Open System Architecture. ... Standards for open systems 13 . Chapter 3: The open systems environment (OSE) 15 . ...

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• Benchmarking UNIX™ Systems
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... Science . ... Science Users Information Paranal Science Operations Visitor Information jump to navigation jump to content . Paranal Facilities . ... Offered Instruments . ... Paranal News . ... Paranal Telescopes Overview . Telescopes and Instruments . ... Overview . ... Manuals . ... Instrument Operation Team . ... Paranal Science Operations . ... Please submit one report per observing run or telescope/instrument combination. ... About ESO in general: . ... Telescope/Instrument Manuals: . ...

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• ESO Web file formats and associated viewers
• AB structure
• moveProducts

... Erie PA. ... Play Information * Episode and Level # : E1M1 Single Player : Yes Cooperative 2-4 Player : Yes Deathmatch 2-4 Player : Yes Difficulty Settings : Yes New Sounds : No New Graphics : No New Music : No Demos Replaced : None * Construction * Base : New level from scratch Editor(s) used : Deu 5.21 BSP 1.1 Known Bugs : None known as of release * Copyright / Permissions * Authors MAY use this level as a base to build additional levels. ...

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• http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom2/a-c/cue2wad.txt
• http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/xplanet-1.3.0-os2.txt
• http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/Animate-199106067.txt

... HST Phase II Proposal Instructions for Cycle 20 > Chapter 3: Fixed and Generic Targets > 3.3 Target Category and Target Description [Description] . ... Each target must be assigned a single primary category from Table 3.2 , and at least one descriptive keyword , chosen from the appropriate Table 3.3 through Table 3.9 (see Table 3.2 for which table is appropriate for each category). ... Table 3.3: Descriptive Keywords for STAR and EXT-STAR . ... Table 3.6: Descriptive Keywords for CLUSTER OF GALAXIES...

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• Finance: Budgets
• For the New User...
• Summary of on-board computers

... l - the mean galactic longitude; . ... mul - the median proper motion along galactic longitude of the stars of the OB-association, in units of 0.001 arcsec year -1 ; . dml - the estimation of mul dispersion in the OB-association, in 0.001 arcsec year -1 ; . mub - the median proper motion along galactic latitude of the stars of the OB-association, in units of 0.001 arcsec year -1 ; . dmb - the estimation of mub dispersion in the OB-association, in 0.001 arcsec year -1 ; . ...

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... The total mass of the scientific payload is about 2500 kg, of which the unfolding parabolic 10-m radio astronomy antenna's mass is about 1500 kg, and scientific package holding the receivers, power supply, synthesizers, control units, frequency standards and data transmission radio system - near 900 kg. ... The jet system is a hydrazine thrusters system: it will be used during the creation of the base system of spacecraft orientation, for unloading of the powered gyros, and for orbit corrections. ...

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... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...

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• Lecture Series 2015-2016 ? Amateur Astronomers Association of New York
• North South Lake, Haines Falls, NY ? Amateur Astronomers Association of New...
• Great Kills, Staten Island ? Amateur Astronomers Association of New York

... Posts tagged ?Stellar association? ... I?m very curious how astronomers began to use Monte Carlo Markov Chain instead of Markov chain Monte Carlo. The more it becomes popular, the more frequently Monte Carlo Markov Chain appears. ... ArXiv] 1st week, Apr. ... Tags: Bible , big bang , FFT , IMF , microlensing , misnomer , model , NGC 602 , power law , Stellar association , wavelet . ... Comment . ... Entries RSS . ... vlk on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...

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• Topics in AstroStatistics
• The AstroStat Slog visualization
• The AstroStat Slog Omni

... Description . ... The SCORPIO-2 project: . ... The multi-mode spectrograph SCORPIO-2 was developed using the experience of observations at the 6-m telescope BTA with the SCORPIO focal reducer . ... The focal reducer consists of several units ('floors') mounted in the common case in the following order (from the telescope focal plane): . ... The focal reducer is connected with the platform-adapter which used for guiding by offset stars and for illumination the spectrograph by calibration lamps. ...

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• V.Shergin's Home Page
• comedi_dio_config
• Instrumentation

... DESCRIPTION General Catalog of Variable Stars (GCVS database) . ... Kholopov P.N., Samus N.N., Durlevich O.V., Kazarovets E.V., Kireeva N.N., Tsvetkova T.M., 1990, General Catalogue of Variable Stars, 4rd ed., vol.IV, Nauka, Moscow. Kholopov P.N., Samus N.N., Durlevich O.V., Kazarovets E.V., Kireeva N.N., Tsvetkova T.M., 1992, General Catalogue of Variable Stars, 4rd ed., vol.IV, Bull. ... Kazarovets E.V., Durlevich O.V. Editor-in-Chief Samus N.N., 1998, New Catalogue of Suspected Variable Stars. ...

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Section I: Introduction to ALFA and GALFA . Section II: System Description . ... ALFA receives 7 beams, 2 polarizations per beam, each covering 1225-1525 MHz. The 14 IF signals cover nominally the 100 to 400 MHz band. ... A high-resolution, low-bandwidth spectrometer (8K channels covering a 7 MHz bandwidth) . ... Each spectrometer board handles two polarizations from one telescope beam.The baseband signals are to be digitized by four 8-bit ADCs at 100 Msamples/sec. ... Bandwidth: . ...

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• serverlList
• HF transmitter doc
• Manpage of FFTFILTER