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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• A Software Package for Automatic Reduction of ISOPHOT Calibration Data
• VLT Data Quality Control
• Recreating Einstein Level One Processing Exposure Masks and Background Maps in

... Analysis of the UVIS03 data show that the gain ratios, relative to the nominal 1.5 , are 1.01-1.04, 2.09-2.15, and 4.28-4.39 at a detector temperature of -82C. A check of the absolute gain of the nominal 1.5 setting was performed using flatfields from the linearity (UVIS05) test; gains were measured at 1.53, 1.52, 1.56, and 1.55, with errors 0.01 , for quadrants A,B,C, and D. Introduction The purpose of the ... Gain ratios for the four quadrants, relative to gain 1.5. ...

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• Fine Guidance Sensor Instrument Handbook
• Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
• FOC Data Handbook

... 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. ...

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... Also the measured signals are a#ected by detector transients, altering the final results considerably. ... The sequence is bounded by two measurements of the FCS , to fix the responsivity for the baseline correction 0 200 400 600 800 1000 measurement time [s] 0.00 0.02 0.04 0.06 0.08 0.10 Volt/second bg source fitted baseline 2. FCS 1. FCS source initial drifting signal corrected signal bg FCS source background signal internal calibration signal source signal corrected ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/bushouseh.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/morganteg.ps.gz
• NICMOS Data Calibration and Analysis

... Parameter Mand Type Default Constraints boxlistset yes lename eboxlist. ts Name of eboxdetect source list imageset yes lename image . ts Names of input EPIC ts images bkgimageset yes lename bkgimage. ts Name of output spline background map expimageset no lename expimage. ts Name of input exposure map detmaskset no lename detmask. ts Name of input detection mask scut no oat 0.01 [0.0  param  10.0] ... 5) If exposure flag is set, multiply spline image by exposure map. ...

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• http://xmm.vilspa.esa.es/sas/5.4.1/doc/omlcbuild.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/omlcbuild.ps.gz
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/omlcbuild.ps.gz

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

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• Data gathering

... Quality Control and Data Processing . ... HOME . ... UVES /UVES . ... retired : . ... This is the home page of the Quality Control and Data Processing Group (QCG) within ESO's Data Management and Operations Division (DMO). ... At ESO Headquarters in Garching, calibration data from all Paranal instruments (VLT, VLTI, survey cameras) are processed, their quality is checked and monitored. ... UVES ECHELLE data, point sources: quality-controlled, homogeneous processing of complete data stream 2000-now ....

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• ESO - Upgrade of the Paranal Astronomical Site Monitor
• ESO - Processed Calibration Files for VLT instruments Now Available
• Data Flow System overview

Next: *imcalc* - Obtain a Up: Calibration Previous: Exposure Map . Background maps are provided by the standard processing for all ROSAT and Einstein instruments. For the PSPC and IPC these are in three standard bands: soft, hard, and broad (Table 6.2). ... N.B.: ROSAT PSPC background maps in SASS 5-6 or higher are generated by smoothing a source-subtracted, exposure corrected image (see the ROSAT Data Products Guide). ... imcalc* - Obtain a background subtracted image for ROSAT PSPC Data . ...

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• The Lynxx Tools
• Rev0, US-Processed Data
• Notes on IPC and PSPC Spectral Fitting

... Donate to Support Science Literacy . ... 2016 Annual Awards . The ASP is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach. ... Shop the AstroShop . ... The Astronomical Society of the Pacific (ASP) is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach.. ...

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• ASP: An Ancient Universe - The Process of Science
• ASP's 2012 Annual Meeting
• ASP: The New and Improved Hubble Space Telescope

... User Guide ] Task: atfix Purpose: Apply various miscellaneous corrections to ATCA visibility data Categories: uv analysis ATFIX performs various miscellaneous offline corrections appropriate for ATCA 3mm data. ... Correct antenna table (when some antennas were off-line) NOTE: This task will usually be used very early in the data reduction process. ... Key: vis The names of the input uv data sets. ... Leave the Tsys calibration as is. constant Apply a constant Tsys between successive Tsys...

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• Spectral Line Processing and FITS files
• Homepage of Matthew Whiting.
• Massaging Steps Performed by UVREAD - UVSET

ANTHONY LASENBY - COSMIC MICROWAVE BACKGROUND . The Cosmic Microwave Background (CMB) provides some of our best and most accurate information about the universe and its evolution. I have been involved in CMB research since 1978, and have worked on experiments including Tenerife, CAT, the VSA and most recently Planck and QUIJOTE . ... In addition, I am interested in several theoretical topics in CMB and early universe research. Planck at Launch . ... Cosmic Microwave Background . ...

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• Astrophysics Group Fringes and Power Spectra from COAST
• Astrophysics Group Cosmic Microwave Background (CMB)
• OptInt PmWiki : Tech Meet 12 | History

... This chapter describes the PEPSYS package for general photometric reductions. The function of photometric reductions is to measure and remove, so far as possible, the instrumental signature from the data. ... The package contains two main parts: a planning program and a reduction program. The planning program interacts with the user to find out the goals of the observing program, and then produces a schedule of the observations needed to meet those goals efficiently. ... ASCII source files . ...

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• Background Correction
• Contents
• ESO-MIDAS User's Guide 94NOV: Volume B

... It can · · obtain ice sample from 20 cm or deeper surface layer, then melt it and extract biomass from the ice surface water by filtration; Laser TOF MS for the measurements of element composition of the biomass; Gas TOF MS for the detection of: 1) volatile components, generated at the heating of biomass sample (closed window mode); 2) secondary ions , emitted from ice matrix by the influence of energetic magnetosphere ... Spectrum of yeast sample. ... Laser TOF MS 6. ...

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• wave processes
• ULF instrument
• Low-frequency electromagnetic sounding instrument for subsurface studies

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope 's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication SSRT - Siberian Solar Radio Telescope . ...

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• Radioastrophysical department ISTP RAS SB

HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11 . ... Onboard mass-spectrometric equipment for study of neutral and ionized components of Earth upper atmosphere. Mass-spectrometer P-11 is one of P-series modifications of the on board radio-frequency monopole spectrometers. ... The instruments of P-series have passed successful approbation in space experiments aboard geophysical rockets MP-12, launched for investigation of Earth upper atmosphere (Ref. ... Measured mass number range, AMU - 1.. ...

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• INFRARED FOURIER-SPECTROMETER SICH-F
• ION AND ELECTRON ENERGY DETECTOR PAN-2
• Researches of Astronomy and Space Physics Department

Operating of the superconducting integrated receiver channel of the TELIS atmospheric sounder. ... The noise temperature of the SIR was measured to be as low as 120 K, with an intermediate frequency band of 4 ­ 8 GHz in double sideband operation; the spectral resolution is well below 1 MHz. The SIR was implemented in the three-channel balloon-borne instrument TELIS (TErahertz and submillimeter LImb Sounder) that detects spectral emission lines of stratospheric trace gases (like ClO and BrO). ...

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• http://www.cplire.ru/html/lab234/pubs/2007_09.pdf
• Research Activities of InformChaos Lab.

... The Zenit-3SLB ILV . ... LAND LAUNCH . ... o Financing of operations performed by OOO International Space Services Contractors. o Land Launch Program coordination and control. o Marketing activity on the SIS territory. ... Leading technical integrator for the Land Launch Complex (coordinator of OOO International Space Services Contractors operations for analytical integration of spacecraft with the Zenit-M SRC). ... Support of operations for SC analytical integration with AU, preformed by RSC...

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• S.P. Korolev RSC Energia - International Space Station
• S.P.Korolev RSC Energia - LAUNCHERS
• RSC "Energia" - Land Launch

The AstroGuide . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . IPAC exists to carry out large, data-intensive processing tasks of critical importance to NASA's infrared astronomy program, and to provide scientific expertise on those projects to the astronomical community. ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• SUE PA Novosibirsk Instrument Making Plant, AstroGuide Listing

... Status of the ELECTRON experiment . ... The objective of the ELECTRON experiment is to perform 3-D measurements of the plasma electrons in the energy range from 10 eV to 26000 eV, with good angular resolution, sensitivity and large dynamical range. ... Figure 1 presents the ELECTRON sensor. ... Click on the picture to view large one) . ... Figure 3 shows dynamical spectra with counting rate measurements performed by ELECTRON experiment during very multiple magnetopause crossings on February, 4, 1996...

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• Space Weather Dials Interpretation Guide
• IKI IPL home page
• ASPI experiment

Analysis of the Systematic Errors of CCD-observations of Asteroids Performed in 2007-2008 . ... Analysis of systematic errors based on CCD-observations taken with Normal Astrograph (D/F = 0.33 m/3.5 m, FOV = 18 16 arcmin, scale = 1 arcsec/pix) of Pulkovo observatory during 2007-2008 has been made. ... A statistical approach that used mean (O-C) values obtained for positions of reference stars within the field of view separated on square bins and magnitude ranges was applied. ...

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• Intl collabration