STScI . HST . NICMOS STScI Analysis Newsletter 31 . ... HST Overview . ... CONTENTS: - NICMOS UDF Data Released - Cycle 13 TAC/Panel Meetings - HST Pure Parallel Observations - NICMOS Recovered from Intel Exception - NICMOS Calibration Plan -New NICMOS Exposure Time Calculator - NICMOS Focus Monitor -New IDL Cosmic Ray Persistence Routine -Recent NICMOS Publications +----------------------------------------------------------+ http://www. stsci .edu/ hst /udf NICMOS UDF ...

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• NICMOS Proposing Example - 7
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• NICMOS STScI Analysis Newsletter 37

... The product and processing information for the EPIC instrument. ... Parameter Mand Type Default Constraints pindex yes dataset none valid le name The Pipeline Processing Summary Index File obspage yes string none valid le name Output observation summary page . ppspage yes string none valid le name Output pipeline processing summary page . epxpage yes string none valid le name Output EPIC instruments processing summary ... Pipeline processing HTML summary le. ...

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• Description
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.

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• The MUSE instrument attached to the Very Large Telescope
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Next: The ESO VLT CCD Detectors Software . ... Up: Instrument-Specific Software . ... The framework for data calibration and analysis of the VLT instrumentation is presented, based on the concepts of a calibration plan, pipeline calibration, quality control, and archiving of calibrated data for a ground-based observatory. ... Quality Control Pipeline provides quality assessment for instrument performance data and observing conditions, and tests the results of the Reduction Pipeline. ...

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... Classes . Files . ... casa . casa::SDObservationHandler . ... Private Member Functions | ... include < SDObservationHandler.h > . ... SDObservationHandler ( MeasurementSet &ms, Vector < Bool > &handledCols, const Record &row) . ... Definition at line 89 of file SDObservationHandler.h . ... row . ... Definition at line 102 of file SDObservationHandler.h . ... Definition at line 117 of file SDObservationHandler.h . ... RORecordFieldPtr < Bool > casa::SDObservationHandler::flagRow_p [private] . ...

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... The spectrum is reversed left to right. ... Starting line IDs Line identification in order 26 (x reversed ) Channel Wavelength Calculated Discrepancy Line # 166.3593 8478.3584 8478.3613 0.0029 1 258.5106 8490.3066 8490.3213 0.0146 2 500.5818 8521.4385 8521.3926 -0.0459 3 912.9249 8573 ... 0.0547 4 1178.5211 8605.7764 8605.7803 0.0039 5 1299.3500 8620.4600 8620.4209 -0.0391 6 1698.4974 8667.9404 8667.9492 0.0088 7 line identification in order 34 (x reversed ) Channel Wavelength ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . The Troughton equatorial, 2-inch aperture, 3-feet focal length, arrived in December 1795 and was mounted, in the English style, under the south dome on two stone piers resting on a massive pillar, round which the staircase of the dwelling house winds. ... The correction of observations made with equatorial instruments was the subject of a study by T. R. Robinson the results of which were published in the Trans. ...

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... The NVSS is being made as a service to the astronomical community, and the principal data products are being released into a directory accessible by anonymous FTP as soon as they are produced and verified. ... The large (4 deg x 4 deg) map cubes and total intensity only images and their associated multisource (u,v) data sets are stored as binary files in FITS format (see Grosbol et al. ... The source catalog derived from the available images is kept in directory CATALOG as CATALOG.FIT. ...

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OSSERVATORIO ASTROFISICO DI ARCETRI CENTRO PER L'ASTRONOMIA INFRAROSSA E LO STUDIO DEL MEZZO INTERSTELLARE LARGO ENRICO FERMI, 5 -- I­50125 FIRENZE Firenze, September 30, 1994 FROM: C. Baffa TO: Tirgo Staff SUBJECT: Data handling with Tirgo Nicmos3 instruments All data taken with Tirgo Nicmos3 instruments (Arnica and Longsp) are stored directly as standard FITS files at 16 bits integer format. ... The acquisition program never rewrites over an old file. ... An example in table 1. ...

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... Dept. for Physics of Planetary Systems . ... Laser station . ... Built a network of laser stations (LLS), radio (GNSS) satellites and observation radiointerferometrychnyh observations of quasars (VLBI) ( YA.S. Yatskiv, Medvedsky MM, AA Pace, EE Volvach, YL Kokurin in collaboration with workers in other entities) . ... БЂў Laser station observation satellites is the global network of service stations of the International Earth rotation and conducts active surveillance for international programs. ...

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... VLBA+Italy survey (to contact the schedulers) (closed) E.Fomalont and J.Romney: To provide some review of problems happened with fringe search in VSOP project. (closed) M.Popov : To compose a tentative time -table of possible observations , and inform the observatories on the specific time slots that might be requested for fringe search program in October-November. (continued) C. Gwinn: to try to compile FAKERAT software on modern platforms. (closed) GBT and ...

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• Appendix B: Map of the Document
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SUBWAY.WAD - The Deimos Subway ============================== This is a fairly large PWAD that takes place in a very small subway system and the rooms attached to the stations. ... Your mission, clean out the stations and eliminate whoever is behind the invasion. ... Maybe you can find some more weapons and ammo in the subway before you buy it. Pre-mission briefing includes the fact that the subway has three stations, with several room attached to each station. ... Go get those demons! ...

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STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado€о Solar . ... Spotting Scopes . ...

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... Navigation in the near planetary space, Mars and Phobos observations. ... navigation in the near-planetary space based on images of Mars, Phobos and the starry sky; . Phobos high resolution imaging; . ... angle               angle . ... Number of TV-cameras                     2                       2 KNM — Mars Observation Camera — is being designed as the scientific instrument of the Phobos-Grunt mission. ... Both instruments are developed for Russian Phobos-Grunt project. ...

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OptInt PmWiki . Pm Wiki / . Edit Page | ... Wiki Help . ... Local resources . ... Initial Setup Tasks . ... Cookbook (addons) . ... Most PmWiki configuration is performed in files called local/config.php and pub/css/local.css . ... When you first install PmWiki, the local/config.php file does not exist. ... PmWiki never writes to files in the local/ or cookbook/ directories, so placing your customizations here makes it easier to track the changes and upgrade PmWiki without losing the changes. ...

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GRANAT is the Russian x-ray sattelite launched to the high apogee orbit (200,000 km) and operated almost for 10 years (1989 -1999) , carrying out four major instruments: French SIGMA coded-mask hard x-ray telescope (30-1000 keV), Soviet ART-P coded-mask telescope (2??-60?? keV), all-sky monitor WATCH (6-150 keV), and a gamma-burst detector PHEBUS . ... Since September 1994, GRANAT is in the survey mode. ... Explore pages devoted to individual GRANAT instruments (including main scientific results): . ...

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... At SAO, the ROSAT data for observation rp123456 will be in /data/rdata/godata/rp123456/ . The PROS package contains sample ROSAT and Einstein data which are in the directory /pros/xray/data which is loaded with the IRAF task ``xray''. ... Thus within an arbitrary working directory and within the IRAF environment, to look at an image the command is, tv> display "xdata$rp110590_im2" 1 If Einstein data are loaded at SAO they will appear in the directory /pool14/i1234/ . ...

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• An example of a typical timing analysis
• Contents
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... Both sets of objective transmission gratings consist of hundreds of co-aligned facets mounted to supporting structures on 4 annuli (one for each of the four co-aligned mirror pairs) to intercept the x rays exiting the HRMA. ... The two sets of transmission gratings, attached to the mounting structure are shown in Figure . ... An individual facet has 0.43-m-thick gold grating bars with 50% filling factor and 9920- period, resulting in 1.15-/mm dispersion. The HRC-S is the primary LETG readout. ...

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USA Solar Mission . Courtesy of NASA's National Space Science Data Center . The Solar Maximum Mission (SMM) was designed to provide coordinated observations of solar activity, in particular solar flares, during a period of maximum solar activity. ... Complementary studies were made as part of the SMM guest investigator program, and coordinated in situ measurements of flare particle emissions were made from the ISEE 3 spacecraft. The spacecraft was launched on February 14, 1980. ...

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Next: Observing the Old-Fashioned Way (Gui-Free Observations) Up: Spectral Line Appendices Previous: OLD Basic Analyz Routines For use with data taken BEFORE March 6, 2000 . This appendix contains example analyz sequences used to look at HI spectra. ... Additionally, if you have not run analyz before, instruction (2) should read: If you have not, instruction (3) should read: . ... 7) redln < rec < n : This first stores the individual ON/OFF - 1 data dumps into registers 100 - 100+ - 1. ...

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• ATOMS