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1. Fine Guidance Sensor Instrument Handbook
FGS Instrument Handbook for Cycle 24 . ... Fine Guidance Sensor Instrument Handbook for Cycle 24 > Chapter 7: FGS AstrometryData Processing > 7.4 Epoch-Level Processing . ... 7.4.1 Parallax, Proper Motion, and Reflex Motion . 7.4.2 Binary Stars and Orbital Elements . ... This is true whether the goal is to determine the parallax, proper motion, or reflex motion of an object measured in Position mode, or the orbital elements of a binary system observed in Transfer mode. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/fgs/design/documents/instrumenthandbook/c07_dataproc5.html -- 11.1 Кб -- 12.04.2016
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2. http://zebu.uoregon.edu/2003/hum399/brahesum.html
... He made observations of a supernova (literally: nova= "new star") in 1572 (we now know that a supernova is an exploding star, not a new star). ... Brahe's meticulous observations showed that the supernova did not change positions with respect to the other stars (no parallax). ... This was early evidence against the immutable nature of the heavens, although Brahe did not interpret the absence of parallax for stars correctly, as we discuss below. Brahe made careful observations of a comet in 1577. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/2003/hum399/brahesum.html -- 6.7 Кб -- 07.05.2003
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3. Data Flow System overview
... In order to realize the optimal scientific return from the VLT, ESO has undertaken to develop an end-to-end data flow system from proposal entry to science archive. The VLT Data Flow System (DFS) is being designed and implemented by the DFS Group (ESO Internal access only) in collaboration with VLT Division and Instrumentation Division . ... VLT Control System Interface . ... OBs are the quantum of data that flows within the DFS, collecting state, data and status information as they flow. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/projects/dfs/ -- 12.8 Кб -- 25.05.2004
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4. Reviewtool
... This website gives the possibility to judge the calibration situation of the XMM-Newton and Chandra instruments by comparing joint and individual fits and their parameters on various targets and observations. ... select a target {OPTIONS} . ... select a version {FLUX_VERSIONS} . ... Using all available observations a histograms in various energy ranges are produced. ... select a version {FLUX_VERSIONS} select the method** 1 2 . Flux - output fluxes in various energy bands for all observations . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/ept/html/preview_public.html -- 13.6 Кб -- 27.06.2008
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5. LSFVO: instruments
... Instruments . ... last 10 years in ADS) . in SAO press releases . ... Back to SAO homepage . Last update: . ... moisav sao.ru . Laboratory of Spectroscopy and Photometry of . ... SCORPIO Multimode focal reducer. SCORPIO-2 Multimode focal reducer (the project) . ... Longs-slit spectroscopy . Multi-slit spectroscopy . ... MPFS Multi Pupil Fiber Spectrograph (integral field) . MOFS Multi Object Fiber Spectrograph . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lsfvo/devices_eng.html -- 5.4 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lsfvo/devices_eng.html -- 5.4 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/lsfvo/devices_eng.html -- 5.4 Кб -- 09.04.2016
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6. ASAP
The A TNF S pectral A nalysis P ackage is a new software package that has been developed within the ATNF, to reduce single-dish, single-pointing spectral line observations. ASAP is now used for single-dish data from ATNF instruments and should be able to read data from any telescope if the data can be written in the "sdfits" format. ... The c++ code makes extensive used of the casa libraries (the package formerly known as aips++). ... A binary version for Fedora Linux should be available shortly. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/jun06/ASAP.htm -- 4.0 Кб -- 23.01.2013
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7. Distributed Software for Observations in the Near Infrared
... We have developed an integrated system that performs astronomical observations in Near Infrared bands operating two-dimensional instruments at the Italian National Infrared Facility's ARNICA and LONGSP . ... The user interface is organized as widget-based X11 client. ... 1993; Di Giacomo et al. 1993). ... Moreover, if the interprocess communication interface includes support for networking, the software immediately becomes network distributed software. ... DESQview/X User Guide 1993, Quarterdeck . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/gavryusevv.html -- 9.9 Кб -- 03.11.2000
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8. Methods and instruments to measure/monitor major site properties
... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...
[ Сохраненная копия ]  Ссылки http://site2010.sai.msu.ru/section/2 -- 9.2 Кб -- 09.04.2016
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9. http://www.naic.edu/vscience/schedule/tpfiles/KelleytagT1819tp.ps
Proposal Identi cation No.: T1819 Date Received: 2003-May-12 11:13:38 Technical Page Proposal Type: Regular General Category: Terrestrial Aeronomy Observation Category: Ionosphere Total Time Requested: 32 Hours Proposal Title: Calibration of new DMSP satellite optical instruments using the Arecibo ISR ABSTRACT: A new generation of optical instrumentation has been developed for the Defense Meteorological Satellite Program and its future replacement, NPOES, which is a joint NOAA/DOD Program. ...
[ Текст ]  Ссылки http://www.naic.edu/vscience/schedule/tpfiles/KelleytagT1819tp.ps -- 100.8 Кб -- 19.04.2004
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10. Journal "Peremennye Zvezdy"
Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Moscow 119992, Russia . ... 84/32, Moscow 117997, Russia . ... Our CCD observations compared to times of minima derived from the archival photographic plates and from the NSVS and ASAS-3 data clearly show that the orbital period of the system is variable. ... The phased light curve for the light elements . ... CCD, Moscow . ... and for the current linear light elements (in excellent agreement with the NSVS, ASAS, and our CCD observations): . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1217495 -- 18.2 Кб -- 09.11.2006
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