... Wide Field Camera 3 Instrument Handbookfor Cycle 23 > Appendix E: Reduction and Calibration of WFC3 Data > E.7 The Cycle 21 Calibration Plan . ... The Cycle 21 calibration plan is summarized in WFC3 ISR 2014-07 . ... continue to maintain and update the standard reference files (biases, darks, linearity, CTE traps) . continue to monitor the instrument (throughput, gain, hysteresis, bad/hot pixels, filter transmission, IR blobs, grism calibration, CTE decline, stability of post-flash) . ...

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• COS Instrument Handbook
• Instruments/Observations 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. ...

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• ESO - UT1 Science Verification
• ESO - Swedish Heterodyne Facility Instrument Science Verification
• Quality Control Library

... Second, the observatory can control the configuration, test data analysis procedures, and provide calibration solutions with the help of instrument models. This paper presents the VLT object-oriented framework for the development of ETCs (Exposure Time Calculators) and data simulators. ... Instrument simulations are being developed for the purpose of predictive calibration, instrument configuration control, and evaluation of data analysis procedures. ...

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• Calibration and Performance Control for the VLT Instrumentation
• Prototypical Operations Support Tools for NASA Interferometer Missions:
• Distributed Software for Observations in the Near Infrared

... 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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• General information
• The site testing programs in Antarctica and in Arctic
• Results of recent and ongoing site programs

... R2515 Date Received: 2009-Jun-08 12:14:47 Technical Page Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Planetary Radar Solar System 94 hours Hours 2 hours Arecibo Radar Imaging of Six Near-Earth Asteroids During February - May 2010 We plan to observe six NEAs with the Arecibo planetary radar system to continue our very successful program of characterizing these ob jects. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/TaylortagR2564tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/HowelltagR2515tp.ps
• Solar System Studies at AO

... Within the transnational Access program of SOLARNET, European investigators can apply for observing time with the European instruments IBIS and ROSA , which are installed at the Dunn Solar Telescope of the US National Solar Observatory ( DST/NSO ). ... Periodic calls for proposals will be published for requesting SOLARNET observing time with the European instruments IBIS and ROSA, installed at the Dunn Solar Telescope of the US National Solar Observatory (DST/NSO). ... SOLARNET Access . ...

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• Procedures for Observations
• Program parameters
• Arcetri Solar Physics Group: Instrumentation - IBIS

Sometimes we require more than one line for a statement Print *, 'This is a long output line',& ' this is the second part',& ' and this is the third part!' Nowadays, in the free form, we continue a line with the symbol "&" (called ampersand), i.e. with the sign & at the end of the old line instead of an almost arbitrary character in column 6 of the new line. ... Exclamation mark in column 1 of course means a comment line also in the old fixed form. ... 3.1) What does the following line mean? ...

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ATNF Home . About ATNF . ... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Staff list | ... Work experience for school students . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... VLBI . ... Arch | ... CSIRO ATNF Data Archives . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... CSIRO Radio Astronomy Image Archive . ...

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• ATNF Colloquium

... If you have a program to convert data to MIDAS input format, fine. ... All you need to do is cannibalize the part of the existing program that reads the data, and add a short piece of code to re-format the data first as a flat ASCII file, one measurement per line; and then convert this to *.tbl format. ... It's just like the process of creating a program-star table. ... You may decide to write a short MIDAS script to apply your format-conversion program and the edited *.fmt file to each night's data...

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• Reductions --- at last!
• PEPSYS general photometry package
• Preliminaries

. Please use the following for publications and media citations: . "Based on observations obtained with Apache Point Observatory's 0.5-m Astrophysical Research Consortium Small Aperture Telescope." . List of publications based on 0.5-m observations (TBD) . for questions or comments contact archive server .

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• ARCSAT Observers Nightlog Form
• Untitled Document
• APO Telescope Documentation

... The SMS program is a critical endeavor to investigate whether the predictions of standard cold dark matter cosmology are consistent with the observed matter distribution in the Milky Way halo. It is the deepest, most extended search for optically elusive dwarf satellite galaxies and tidal streams to date, covering the entire Southern hemisphere. ... However only a few dwarf satellites have been found around the Milky Way to date - 22 dwarfs compared to 500-10,000 predicted by theory (Klypin et al. ...

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• GSAOI Latest Developments Page
• RSAA Annual Report 1998
• GSAOI Instrument Description Page

Sometimes we require more than one line for a statement Print *, 'This is a long output line',& ' this is the second part',& ' and this is the third part!' Nowadays, in the free form, we continue a line with the symbol "&" (called ampersand), i.e. with the sign & at the end of the old line instead of an almost arbitrary character in column 6 of the new line. ... Exclamation mark in column 1 of course means a comment line also in the old fixed form. ... 3.1) What does the following line mean? ...

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• Armagh Observatory

For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...

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• V.Shergin's Home Page
• GRB follow-up team
• LSFVO: instruments

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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• Technology / Technology / Meade Instruments
• Series / Meade Instruments
• Meade Instruments Corporation - ETX Astro Telescope and ETX Spotting Scope

... 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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• http://xmm.vilspa.esa.es/sas/7.1.0/doc/odfbrowser.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/odfbrowser.ps.gz
• http://xmm.vilspa.esa.es/sas/6.0.0/doc/odfbrowser.ps.gz

The Wind spacecraft. ... It was designed to observe the solar wind approaching Earth, from a position near the Lagrangian point L1, and it is part of the International Solar-Terrestrial Physics (ISTP) Initiative . ... The original plan called for "Wind" to approach its final station over two years, undergoing two close encounters with the Moon to boost its speed. ... For additional details and updates, see the home page of the "Wind" mission. Exploration" home page (index) Glossary . ...

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• FM-3I Instrument
• SPICE System Overview .
• Solar Max

... It was designed to observe the solar wind approaching Earth, from a position near the Lagrangian point L1, and it is part of the International Solar-Terrestrial Physics (ISTP) Initiative . ... The original plan called for "Wind" to approach its final station over two years, undergoing two close encounters with the Moon to boost its speed. ... If however the object is moving , the encounter is not symmetric, and in the end the spacecraft may have gained or lost speed, depending on its trajectory. ...

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• Events on January 10-11, 1997 - INTERBALL observations
• Optico-electronic Instruments for the Phobos-Grunt Mission
• Laboratory facilities for science education and research

Instruments and Methods 139 Data browsing at Metsahovi Radio Observatory Prisse Kononen, Ari Mujunen, and Jan Engelberg Metsahovi Radio Observatory, Kirkkonummi, Finland There are several di erent types of non-astronomical, chronological data which are collected non-stop at Metsahovi Radio Observatory. ... The rst version of the weather data presentation program is available at the site http: kurp.hut.fi local which limits the access only to the network computers of Metsahovi Radio Observatory. ...

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• Pulkovo NEO Page: Ephemeris Support
• Pulkovo NEO Page: Observations

Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

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• Status and Goals of the NICMOS Calibration Plan
• A Color Analysis of NICMOS Parallel Observations
• No Title

... Members . ... The ATM's of Boston was founded in 1934 by a group of persons interested in assisting others in the art of optical polishing the craft of telescope making, and to learn together about the science of astronomy and the use of astronomical instruments. ... Mr. Jones introduced the club to Dr. Harlow Shapley at Harvard College Observatory. ... Regular shop activities resumed with the help of these "professional amateurs" and the club grew to 180 members. ... Club Newsletters . ...

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• Amateur Telescope Makers of Boston ATMoB Observing Awards Program