... ABOUT ST-ECF . ... Change the relative shifts in association file . ASNCOMBINE . Process and combine images in one or two NICMOS associations . ... Examine images in an association . ... Plot magnitude as function of subpixel position . ... Group images in associations . ... Makes flatfields corresponding to the output image of asncombine . ... Compute the pixel response function for an image created with asn combine . ...

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• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• The Photometric Performance of the NICMOS Grisms

... For example, precision of the approximation was calculated for Solar system and 47 Uma star system Kepler orbital elements : Jupiter Saturn 9.537 0.0539 Uranus 19.189 0.0473 Neptune 30.070 0.0086 47 Uma b 2.10 0.032 0.10 3.76 5.83 0.89 47 Uma c 3.60 0 ... rad , rad , rad l, rad 0.0228 1.754 4.801 0.328 0.0434 1.983 5.865 5.591 0.0135 1.291 1.685 2.495 0.0309 2.300 4.636 4.673 Kepler elements for Solar ... Estimation accuracy of disturbing function (h1) expansion is presented. ...

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• Catalogue of double stars
• The Canadian S2 Correlator - Principles of Radio Interferometry
• Phase light curves of young binary systems

WDC-A Digital Exchange Format for One-Minute Geomagnetic Data (Update August 1993) 1. The logical record length is 400 coded characters containing header information, blank spaces, and data for one element for one hour. ... Each logical record contains header information and data in the following format: North polar distance, longitude, year, month, day, hour, element, observatory code, blank spaces, 60 data values, and an hourly mean. ... ORG is the origin of the data. A = Alaska Chain. ...

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• http://www.wdcb.ru/stp/data/geo_hour.val/Readme.txt
• http://www.wdcb.ru/stp/data/solar.act/sunspot/sunspot.txt
• "STP Data" STP Data

... 1915QB4_C22v12p1___ Informations. relative to: J1-Io: 201, J2-Europe: 134, J3-Ganymede: 85 reference frame: astrometric centre of frame: topocentre epoch of equinox: date time scale: GMT (UT1=GMT+12h) reduction: no information coordinates: apparent distance, position angle diff. refraction: removed receptor: heliometer telescope: Refractor, F = 2.5 m, D = 17.8 cm observers: Gill David, Finlay W.H. data included in standard data file: no Comments. no information Format. ... Year of the observation 4....

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• jg0026
• jg0008
• Links to Sites Related to Solar Physics

Available on Macintosh Mac 512KE and earlier. At the Computer) . At the Equipment) . 9 PIN D-SUB FEMALE at the computer. 9 PIN D-SUB MALE at the mouse cable. Pin . ... Don't use this one, it may be converted into output handshake in later equipment. ... Transmit Data, positive going component . ... Transmit Data, negative going component . ... Receive Data, positive going component . ... Receive Data, negative going component Note: Direction is Computer relative Equipment. ...

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• Order Definition
• HwB: C16/C116/+4 Joystick Connector
• CCD Image Quality - PixelVision

... Meade Instruments Corporation . ... Autostar Computer Controller Instruction Manual . Autostar Computer Controller . ... NOTE: This manual covers both Model #495 Autostar and #497 ETX Autostar Computer Controllers. ... Autostar Primary Menus and Options . ... Chapter 3: Alignment . ... Guided Tour Menu . ... Chapter 5: Autostar Menu Functions . ... Meade Autostar Computer Controller . ... Meade #505 Connector Cable Set Manual . ... Copyright 2006 Meade Instruments Corporation, All Rights Reserved. ...

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• Meade Instruments Corp. - Meade Customer Support
• Meade Sports Optics - How to Select the Right Binocular
• Meade Instruments Corporation - How Telescopes Work

The Mars Flag has a different design on the reverse side. obverse side of flag . ... The orbit lines on the obverse cross the Sun on the lower half of the flag and appear to go behind the Sun on the upper half of the flag. The reverse side has the orbits lines continuing around the Sun on the upper half of the flag. ... The Mars Flag reverse side is a continuation of the obverse side and not just a different design on the back and not a mirror image of the obverse. Main Flag Background Color . ...

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• ASP: Making a Rainbow
• ASP: Using Multicultural Dimensions to Teach Astronomy

Text of these problems is available also in other languages : . ... What can one see in the Moon's sky more often - the Sun or the Earth? ... There are about of 250 millions of stars in the elliptical galaxy M32 (a satellite of Andromeda galaxy). ... The masses of Capella's components. ... You are proposed to estimate the masses of Capella's components, using our observational data. ... A galaxy's mass. ... Estimate the mass of FGC 1908 and compare it to the mass of our galaxy. ...

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• Plastic forming and welding of optical elements for laser technologies and
• Department of Solid State Physics MIPT
• Cadmium Tungstate (CdWO4)

. home . product . gallery . contact .

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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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• Open System Handbook: A Guide to Building Open Systems
• Getting Started in Actor Prolog. Underdetermined Sets.
• DataFax Wizard

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... NamespaceљList . ... instFromObs . ... tcc.axis.instFromObs Namespace Reference . ... Compute instrument position from observed coordinates. ... position of target in observed coordinates (a coordConv.PVTCoord) . ... targInstXY: position of target in instrument coordinates (a tcc.base.ArrayPVT2) (deg) i.e. a position in instrument X,Y relative to inst.iim_ctr, the center of the instrument . ... list tcc.axis.instFromObs.__all__ = ["instFromObs"] . ...

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• lsst.tcc: python/tcc/axis/coordConvWithFP.py Source File
• APO Job Announcements
• Telescope Tracking Smoothness

The aim of this section of the course is to enable you to use simple computer programs to solve a variety of common astronomical tasks. ... I have (somewhat arbitrarily) decided to use Python for this course, because it seems to be gaining popularity fast for astronomical data handling, and because some of you will have encountered it at the ATNF course. ... We've put Python (plus all relevant libraries) on the Stromlo Linux computers moron and maggot. ... Now log in to moron (or maggot). ...