... Two background corrections can be performed with the package: . Interorder background: The scattered light in the interorder region is measured at a certain number of positions and the background map is provided by polynomial or spline interpolation. ... Sky background: Sky windows are defined on both side of the orders with the comamnd DEFINE/SKY and sky background is extracted using EXTRACT/SKY . ... SKY object 2 CURSOR . EXTRACT/SKY object sky FILTER . ... EXTRACT/ECH object ext . ...

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• echelle

New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...

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• Pulkovo Database of Observations of Visual Double Stars

Observation of the Sunyaev-Zel'dovich E ect toward CL0016+16 at 43 GHz M. Tsuboi et al. Ibaraki University, Japan We performed a mapping observation of the Sunyaev-Zel'dovich e ect toward a distant cluster of galaxies, CL0016+16, at 43 GHz using a newly developed 6-beam SIS receiver installed in the Nobeyama 45-m telescope. The temperature decrement of the cosmic microwave background radiation was measured to be
T  A = 0:490:05 mK at the central position of the cluster. ...

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• OptInt PmWiki : PmWiki / Markup Expressions

... 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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• The STScI NICMOS Calibration Pipeline
• NICMOS Calibration Pipeline: Processing Associations of Exposures
• ADASS 2003 Conference Proceedings

Optics includes the surveys and adjustments to the reflectors as well as the pitch, roll, and focus measurements. ... 080515: platform/tiedown motion during vlbi cal scan . ... Surveying the primary reflector . Surveying the dome position from AO9 . ... year 2002:Td inches/platform inch, TdPos vs temp at platform focus position. dec03: platform corner height vs za when looking at tower. jan10: dynamic load on tiedowns from platform motion. 22feb10: fit tiedown tensions using 2008,2009 data . ...

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• td_move_nuts
• on,off position switching offsets
• byu phased array feed.

... The next step after loading is to apply a number of ``fixes'' that are important for 3-mm data. ... By default atfix applies the ``standard'' gain/elevation model for the antennas. ... As mentioned above, the ATCA uses the chopper wheel method to measure an above atmosphere system temperature. ... On the night of an ATCA reconfiguration, a solution for the antenna positions is derived. ... Task atfix corrects the data for an improved antenna location solution via the dantpos parameter. ... ATFIX . ...

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• kpvslice: interactive position-velocity slicing
• Clock Corrections at Parkes
• casacore: measures/Measures/MeasComet.h Source File

... This is the new procedure for setting theDIS grating zerostep positions. ... Specify which gratings are in eachbay. In an mcnode session, tell the DIS which gratings are loadedwith the command . dis_define_gratings . ... dis grating n=1 type=low (e.g.) . ... dis grating n=1 col=b zerostep=280(e.g.) . ... Edit the grating names in the file/home/apotop/MC/gratings (e.g. low, medium, high). ... Multiply this number by the step/pixelscale for that color grating. The step/pixel scales are: . ...

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• SDSS M1 Mechanical Collimation
• Guider Mechanical Commands
• TUI:Telescope:Slew Window:Options:Calibrate

Contents] [Prev page] [Next page] [Index] . ... Positioning HTML Content Using Styles . Positioning HTML Content Using the <LAYER> Tag . ... Absolute Positioning . ... Creating Positioned Blocks of Content Dynamically . Writing Content in Positioned Blocks . ... Positioning the Flower Layers . Positioning and Moving the Fish and Poles . Defining the onLoad Handler for the BODY Element . ... Adding Another Layer to Contain the Reverse Fish Image . ... The Initialization Functions . ...

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• Colors and backgrounds
• Background color examples

... Bus Hound may be the very first product of its kind -- a software bus analyzer for capturing device I/O and protocol. ... When the capture buffer fills to capacity, Bus Hound can be configured to stop the capture process or continue capturing, keeping the most recent acquired data. ... IDE : Bus Hound captures command and data transfers for ATA and ATAPI devices. ... B us Hound captures I/O using a device driver. ... The below figure demonstrates how Bus Hound captures data for SCSI devices. ...

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• Dome position
• harak_e

Astron 193 Lecture 2, Jan.28, 2015 NOTES 1/ Data vs. ... 4/ Data Storage View Your Data Software to read the data files rrent Astronomy Formats FITS inary with standards, Cu b defined keywords, but may become not good enough for large data of the future LOFAR, SKA in radio, LSST ds9 display the data mage gui, but also access to catalogs download and image the files i event files contain all the information about the observation photons , energy, arrival times ...

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• http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/jcm_20061212.pdf
• QPOE Files
• Spatial Analysis

IRAF/STECF 2-D spectrum point source / background decomposition package . ... The general problem is one of spectral decomposition - of separating the spectra of the point sources from the background. ... The STECF IRAF layered package "specres" provides two tasks to extract point source spectra from 2-D images (either longslit, multislit or cross-dispersed) and decompose the full background over the image. ... A Point Source Function spectrum image is required as a 2-D spectrum. ...

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• NPOI Lab
• SPECHOLUCY (V1.00) --- Dec02 stecf.specres --- SPECHOLUCY (V1.00)
• SPECINHOLUCY (V1.00) --- Dec02 stecf.specres --- SPECINHOLUCY (V1.00)

... Positions in 2000 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2001 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2002 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2003 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2004 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . ...

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• STFC Introductory Solar System Plasmas Summer School
• Human Orrery
• An Overview of the Coupled Earth-Sun System PPARC Introductory Solar System

... SPECIAL HONORS: Eagle Scout; Sam Houston Area Council 1976 Distinguished Eagle Scout Award ; Presidential Medal for Freedom, 1970; NASA Distinguished Service Medal; two Navy Distinguished Flying Crosses; 1967 FAI De Laval and Gold Space Medals (Athens, Greece); the American Academy of Achievement Golden Plate Award ; City of New York Gold Medal in 1969 ; City of Houston Medal for Valor in 1969 ; the National Academy of Television Arts and Sciences special Trustees ...

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• Astronaut Bio: Dale A. Gardner
• Astronaut Bio: James H. Newman (8/2008)
• Astronaut Bio: John E. Blaha (05/2008)

I/146 Positions and Proper Motions (Roeser+ 1988) ================================================================================ Catalogue of Positions and Proper Motions Roeser S., Bastian U. =1988A .. ... 449R ================================================================================ ADC_Keywords: Positional data; Proper motions Description: PPM North gives J2000 positions and proper motions of 181,731 stars north of -2.5 degrees declination. ... The mean epoch is near 1931. ...

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• Positions and Proper Motions - South

... The Time shift for April, 17-18 20 April 1999 . ... The INTMINS April 1999 operations schedule was done on the base of the MIR ground track long-term prediction using the MIR's orbital elements status on 29/03/99 . ... The investigation of the time shift behaviour was began before 29/03/99 on the base of the different orbital elements determined (by KIAM RAN) 22/03/99, 25/03/99 and continued on the base of the orbital elements determined at 31/03/99, 5/04/99. ... Modified 20 April 1999  ...

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• The INTERBALL Tail PROBE orbital elements
• The INTERBALL Auroral PROBE orbital elements
• Trigonometry--what it is good for?

... All the optical elements are mounted in a cryostat aimed at keeping components at a temperature of about 80 K. The focal plane masks (field stops or slits) are mounted on a wheel. ... The collimator is an achromatic doublet lens, which images the entrance pupil of the TNG and provides an almost parallel beam (F-number about 2000) at the pupil plane, where Lyot stops can be placed. Right after the pupil plane, two close wheels mount filters and grisms. ...

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• IBIS - Installation
• Procedures for Observations
• Positions

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... Brief History of Rocket and Space Technology . ... ISS Russian Segment . ... Chronology of Extravehicular Activity . ... Sea Launch . ... Land Launch . ... ILV "dry roll-out" (installation on the launch pad and critical launch readiness checklist); . ... Making the Rocket Segment systems ready for the launch site activities; . ... Contribution of RSC Energia to the Russian Rocket-Space Technology ...

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• S.P. Korolev RSC Energia - International Space Station
• INTERNATIONAL SPACE STATION
• S.P. Korolev RSC Energia - News

... 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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• Keywords_107

Pulkovo NEO Page . ... NEA Accuracy Estimation . ... The estimation of accuracy of the current CCD observations of asteroids and comets is constantly performed at Pulkovo Observatory. ... The (O-C) values, so called "Observed" minus "Calculated" positions, characterize numerically the observations of any observatory, both professional and amateur, during a short period (one or several close nights). ... So the (O-C) values for these objects nearly entirely define the errors of observations. ...

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INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

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• Lunar equatorial positions. Explanations for Computer Ephemeris.
• Central meridian positions for physical observations of Saturn for Computer
• Central meridian positions for physical observations of Uranus for Computer