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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• The ESO VLT CCD Detectors Software
• ADASS 2002 Conference Proceedings
• Post Operational HST Science Instrument Archives

... Data . ... Listed below are the titles and abstracts of the WFPC2 Group's Technical Instrument Reports (TIRs). ... TIR WFPC2 08-04: WFPC2 Two-Filter Spectral Parameters for the Archive (abstract) or PDF (0.05 MB). ... TIR WFPC2 02-05: SMOV3B WFPC2 Lyman-Alpha Throughput Check (abstract) or PDF (0.21 MB). TIR WFPC2 02-04: SMOV3B WFPC2 Photometry Check (abstract) or PDF (1.2 MB). TIR WFPC2 02-03: SMOV3B WFPC2 UV Contamination Monitoring and Throughput Check (abstract) or PDF (0.40 MB). ...

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• WFPC2 ISR Abstract
• WF/PC-1 Instrument Science Reports

... The input dataset is an event list created by rgsframes and is modi ed by the addition of the PI column to the PIXELS table. ... EXPOSURE Required columns: FRAME int32 frame identi er TIME real64 timestamp { PIXELS Required attributes: WINDOWX0 WINDOWY0 telemetry window: origin (node coordinates) WINDOWDX WINDOWDY telemetry window: dimensions RAWY z nominal readout row in HTR mode Required columns: FRAME int32 frame identi er RAWX RAWY y int16 coordinates ENERGY int16 uncalibrated ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/rgsenergy.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/rgsenergy.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgsenergy.ps.gz

Next: INTRODUCTION . ... This article presents the Quality Control system of the Very Large Telescope. ... After a presentation of the QC levels and their implementation for the VLT, the paper discusses the usage of instrument models. ... On the other hand the observatory can control the instrumental configuration, test data analysis procedures, and provide calibration solutions with the help of instrument models. ... Quality Control . ... Instrument models for calibration and quality control . ...

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• ESO - cal07
• ESO - Thesis Topic: Planetary Nebulae and HII regions in the Elliptical Galaxy
• Trend analysis

Workshop on geometric analysis and spectral theory . ... On a class of random walks on groups with infinite number of generators". ... Optimal transportation, weak flows and very degenerate elliptic PDE's". ... Singular solutions to fully nonlinear elliptic equations". ... I will give some hints on how this conjecture is related to minimal surface theory and I will describe some flatness results for non local equations on one hand and on elliptic equations on riemannian manifolds on the other hand. ...

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• Workshop on geometric analysis and spectral theory. Schedule

... An analysis of series of flat­field exposures obtained in echelle mode adds support to the view that the performance of an instrument should be monitored closely and described quantitatively. ... This may result in confusion about basic instru­ mental parameters, the precision of the set­up, the amount and distribution of calibration frames which are required and finally the assumptions on which the data reduction procedure should rely. ... The value for pure random noise is indicated 1). ...

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• STScI NICMOS Software
• VLT First Light
• No Title

... The large body of near infrared observations presented in Testi et al. (1997; 1998) are analysed with the aim of characterizing the young stellar clusters surrounding Herbig Ae/Be stars. The results confirm the tendency of early Be stars to be surrounded by dense clusters of lower mass "companions", while Ae stars are never found to be associated with conspicuous groups. ... Only the most massive stars (10-20Msun) are found to be associated with dense (10^3 pc^-3) stellar clusters. ...

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• cephe (Abstract)
• ARNICA (Abstract)
• Arcetri Correlation Spectrometer

... These sources are much more likely to be gravitationally lensed by intervening galaxies as compared with sources discovered in surveys in other wavebands. ... The effect of lensing by clusters is then discussed briefly. This is expected to increase the source confusion noise in a Planck survey in the directions of clusters, and could provide information about galaxies with flux densities that are too faint to be detected directly by Planck . ... 2 The properties of galaxy--galaxy lensing . ...

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• Inference of Coefficients for Use in Phase Correction
• Analysis of (radio) spectra Bojan Nikolic web pages (r. 329)
• Inference of Coefficients for Use in Phase Correction Bojan Nikolic web pages

P1636 2002-Feb-01 18:06:19 Technical Page Proposal Type: Regular General Category: Pulsars Sub-Category: Continuum Observation Category: Galactic Total Time Requested: 54 Hours Proposal Title: A Complete 1.4-GHz Search for Pulsars in Globular Clusters Using WAPP ABSTRACT: In June 2001 we obtained 1.4-GHz Arecibo pulsar search data toward 10 globular clusters using the WAPP instrument. ... Maybe Part of the observing run. ... This proposal requires coordination with GPS L3 at 1381 MHz. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/StinebringtagP2613tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/StairstagP2741tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/StinebringtagP2613tp.ps

... Abstract (txt) . ... Xiao-li Meng (Harvard U) . ... presentation (pdf) . ... web page: astrostatistics.psu.edu/stat05.html . ... H. Kang (Department of Statistics, Harvard University), D. van Dyk (Department of Statistics, University of California at Irvine), V. Kashyap (Harvard-Smithsonian Center for Astrophysics), A. Connors (Eureka Scientific) . ... Poster (ps) . Poster (pdf) . ... Y. Yu, X.L. Meng (Dept. of Statistics, Harvard Univ.) ... Y. Yu (Dept. of Statistics, Harvard Univ.) ...

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• Topics in AstroStatistics
• Notes on IPC and PSPC Spectral Fitting
• Spectral Analysis

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Science & Technology . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Science with NIFS, Australia's First Gemini Instrument . ... The Near-infrared Integral Field Spectrograph (NIFS) will be Australia's first Gemini instrument. ... These and other science drivers for NIFS are discussed. ... NIFS Core Science . ... Gemini Core Science . ...

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• Near-Infrared Integral-Field Spectrograph (NIFS): An Instrument Proposed for
• Image Digitising and Analysis of Outflows from Young Stars
• UNSWIRF: A Tunable Imaging Spectrometer for the Near-Infrared

Next: CONCLUSION Up: CHIRPLET TRANSFORM SUBSPACES Previous: Nondilational Chirplet Transform . Suppose we choose a windowed sinusoidal FM signal for our mother chirplet. Such a signal has a frequency that periodically rises and falls (much like the vibrato of musical instruments or the wail of a police siren). ... Figure 14 . ... Using the warbling mother chirplet, we also computed the ``dilation-dilation'' ( ) plane of the chirplet transform (Fig. 16 ) for the pendulum data. ...

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• Nerve response
• AIAA Invited paper, 1994
• Boundary layer transition

... One of the instruments, the Troughton equatorial telescope, is maintained at constant temperature and relative humidity, to reduce the rate of deterioration. ... 3.1 Troughton Equatorial Telescope . Figure 1 shows the equatorial telescope constructed by J E Troughton of London and which was erected in the west dome of Armagh Observatory in 1795. ... Troughton, J. E.: c.1790, Instructions for Adjusting the Troughton Equatorial Telescope, Armagh Observatory Archives , M17.2, 3pp. ...

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• Abstract
• Abstract 218
• Abstract 200

Next: Summary of reduction Up: Echelle Reduction Previous: Saving the Data . In the present version we will be concerned with the standard configuration of CASPEC, the Cassegrain Echelle Spectrograph which is in operation at the Cassegrain focus of the ESO 3.6 m telescope. ... In its standard configuration CASPEC uses a a 31.6 lines/mm echelle grating together with a 300 lines/mm grating cross disperser. ... The table shows the change in resolution with the order number. Table: Resolution . ...

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• Molonglo deep sky survey
• Radio patrol survey by Gregory and Taylor
• Introduction

... In this case the F5-F9 dwarfs turn out to be more metal-rich (by 0.1 in [Fe/H] ) thab G and K dwarfs, and the metallicity of the Hyades cluster turns out to be larger than the solar one [Fe/H] Hyades =+0.1 . ... При этом карлики F5-F9 оказываются богаче металлами, чем более поздние звезды, примерно на 0.1 по [Fe/H] , и металличность звезд Гиад относительно Солнца равна [Fe/H] Hyades =+0.1 . ...

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... Europa lander", Moscow >12.02.2009 Outline Planetary instruments for in-situ chemical analysis Laser-induced plasma spectroscopy: principle, instrumentation, features GENTNER proposal of the LIBS instrument for the Europa lander mission State-of-the-art of the instrument Page 2 von Hoerner & Sulger GmbH Int. Symp. ... Page 3 von Hoerner & Sulger GmbH Int. Symp. ... Europa lander", Moscow >12.02.2009 Laser-Induced Breakdown Spectroscopy (LIBS): Principle Page 5 von Hoerner & Sulger GmbH Int. Symp. ...

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• Space Research Institute (IKI) Seminar
• Optico-electronic Instruments for the Phobos-Grunt Mission
• INTERBALL IB_TAIL April 2000 during operation scheduling

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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• Meade Instruments Corporation - Pictor Manual Parts 11
• Meade Instruments Corporation - Pictor Manual Part 16
• Meade Instruments Corporation - Pictor Manual Part 3

SN 1989B Light Curve Analysis. ... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... The observations were inserted against the V magnitude templete of BL, CCD photometric data, (Wells et. al, (1994) and a color trend (B-V) histogram of the mean type Ia SN (BL)(nutemp.gif). Key Words: Amateur Observations, Supernova, Magnitude Estimates, 1989B . ...

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• Further Information and Bibliography
• Abstract Registration Form - INTERNATIONAL SYMPOSIUM "ASTRONOMY - 2005: CURRENT

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . Login . See many more Astronomy Listings by: Category or Alphabet . ... Listed Since October 21, 1998 . ... Web Site . http://www.star-instruments.com/ . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

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• Find The Perfect Gift For Your Favorite Astronomy Nut - an Astronomy Net...
• Astronomy Terms - To Help You Study The Universe - an Astronomy Net Article
• Davis Instruments, AstroGuide Listing

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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• Solartron Instruments