... List of Tables . ... 1.3.1 Target Acquisitions . ... Chapter 2: COS Data Files . ... 2.2 COS File Names . 2.3 COS File Structures . 2.3.1 COS FITS Table Extension Files . 2.3.2 COS FITS Image Extension Files . ... 2.4.1 Uncalibrated Science Data Files . 2.4.2 Intermediate Science Data Files . 2.4.3 Final Science Data Files (and Product Files) . 2.4.4 Auxiliary Data Files . ... 3.4.15 DQICORR: Initialize Data Quality File . ... 3.6 Customizing COS Data Calibration . ...

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• ACS Instrument Handbook for Cycle 20
• Space Telescope Imaging Spectrograph Instrument Handbook
• Fine Guidance Sensor Instrument Handbook

... NICS will be the only infrared instrument for the first light of the TNG; as a consequence, we decided to incorporate a sufficient degree of operation flexibility by providing the instrument with six different observing modes, three aimed at imaging and three at spectroscopy: . ... It will be possible to use the narrow band filters as order sorters; this will allow to perform high resolution long-slit spectroscopy in the wavelength ranges covered by the available narrow band filters. ...

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• Procedures for Observations
• IBIS: SolarNet Access

... Science . ... Science Users Information Paranal Science Operations Visitor Information jump to navigation jump to content . Paranal Facilities . ... Offered Instruments . ... Paranal News . ... Paranal Telescopes Overview . Telescopes and Instruments . ... Overview . ... Manuals . ... Instrument Operation Team . ... Paranal Science Operations . ... Please submit one report per observing run or telescope/instrument combination. ... About ESO in general: . ... Telescope/Instrument Manuals: . ...

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• ESO - La Silla Science Operations
• ESO - Observing Facilities
• ESO - Instrumentation Development

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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... New Mexico State University is seeking a technical and computer-oriented person as a Support Astronomer for nighttime astronomical observing at Apache Point Observatory (APO) with the Astrophysical Research Consortium (ARC) 3.5m Telescope. б  . ... Paper/email documents will not be accepted. ... TELESCOPE OPERATIONS SPECIALIST . ... Responsibilities include nightly operation of the 3.5m telescope and instruments, Quality monitoring the data streams and system performance and observing efficiency. ...

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• Astrophysical Research Consortium Small Aperture Telescope
• APO Telescope Documentation
• ARC 3.5m | Instrumentation

... Moore Observatory is a research and advanced teaching facility of the University of Louisville. ... The 24-inch Ritchie Chretien (RC24) telescope is a research instrument used by faculty and graduate students involved in studies of exoplanets, optical properties of the atmosphere, and the development of imaging and spectroscopic technology. ... Kent (CDK20S) are collaboratively operated by the University of Louisville and the University of Southern Queensland for both research and education. ...

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... Staff list | ... Murchison Radio-astronomy Observatory . ... Australia Telescope Online Archive (ATOA) . ... VLBI . ... The successful applicant will pursue a range of challenges related to low-frequency, wide-field, and astrometric radio observations at high angular resolution, with substantial scope for personal research direction. ... ASTRON operates the LOFAR and Westerbork radio telescopes and hosts the Joint Institute for VLBI in Europe (JIVE), which operates the European VLBI Network (EVN). ...

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• Pulsar group | Observing / Psrcorr
• Links to Millimetre Telescopes, Instruments, etc.
• ATCA_report

... Recent Topics . ... MAO main . ... Fw: ASTRONET: Task 5.4 - observing schools . ... Subject: Re: ASTRONET: Task 5.4 - observing schools . ... second half of September, and which will be funded by the training and . ... www.iap.fr/opticon/neon_schools/2014/index.html . ... intended for master and starting PhD students. ... actions on observing schools, providing access for students, Master . ... observing schools for master students. ... in form of observing schools for pre-PhD students. ... MAO NASU...

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... The science goal monitoring (SGM) system is a proof-of-concept effort to address these challenges. The SGM will have an interface to help capture higher level science goals from the scientists and translate them into a flexible observing strategy that SGM can execute and monitor. ... The Science Goal Monitor (SGM) system will interact with not only the data processing pipeline for a mission, but when used on board the spacecraft, it will also interact with the raw data from the detector. ...

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• System Interfaces to the STIS Calibration Pipeline
• Real-Time Linux Driving a Spectrometer
• REMOT: A Design for Multiple Site Remote Observing

... The procedure simply observes ON your source for x minutes and then takes a `blank sky' observation OFF your source for the same amount of time and tracking the same azimuth and zenith angle range. ... Typically, observing times are kept to within 5 minutes (with 5 minutes as the most efficient, and therefore default, choice). ... If your scans are for 5 minutes or less, your wait time should be set to 1 minute (the default setting). ... A 5 minute ON/OFF + 10s CAL takes 11.3 minutes. ...

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• observing techniques
• Spectral-Line Observing
• Spectral-Line Observing at AO

... An OBJECT column gives the name of the object observed (usually a star name). ... In critical cases, it is common practice to measure sky on two or more positions around a target object, and these positions must be identified. ... A general treatment of this problem requires a column called OBJECT, bearing the usual name of the object (as in the star tables); a column labelled STARSKY, to distinguish between star+sky, star alone, or sky alone; and additional columns to identify the sky position. ...

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• General instrumental information
• Using a Standard Star
• Instrument Description: CASPEC

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• XMM-Newton Trainee Project 2005
• The European Photon Imaging Camera (EPIC)
• XMM-Newton Trainee Project 2004

... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document “Programmatic Requirements for Gemini Instrumentation Development” states the requirements for the Software Maintenance Manual . ...

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• Dougal Mackey - CV
• GSAOI Other Instrument Links Page
• Other Infrared Instruments.

... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...

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Next: CONICA: The high resolution Up: VLT Status and Instruments Previous: VLT First Light . ... Infrared instruments for the VLT . Instrument Summary . ... The already approved infrared instruments for the VLT are: . ... CONICA: Coude Near Infrared Camera (P.I. R. Lenzen, MPIA, Heidelberg) - an historical name as this instrument will be used for diffraction limited 1-5 m imaging, polarimetry and spectroscopy with the NAOS, Nasmyth Adaptive Optics System on UT1 (P.I. G. Rousset, ONERA ). ...

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• Space Telescope-European Coordinating Facility
• CONICA: The high resolution near-infrared camera for the ESO VLT
• Status and Goals of the NICMOS Calibration Plan

... Meade Instruments Corporation . ... Meade Pictor 616A Color Filter System Instruction Manual . ... Remove the Meade Pictor 616A Color Filter System from the telescope or camera. Use the supplied hex wrench to remove the three screws from the telescope side of the Meade Pictor 616A Color Filter System. Position your Meade Pictor 616A Color Filter System to align with the diagram below. ... Carefully screw each filter into the wheel, and re-assemble the Meade Pictor 616A Color Filter System. ...

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• Telescopes - Products
• Products
• Meade Instruments Corporation - #497 Autostar Computer Controller for ETX-90EC,

GRANAT is the Russian x-ray sattelite launched to the high apogee orbit (200,000 km) and operated almost for 10 years (1989 -1999) , carrying out four major instruments: French SIGMA coded-mask hard x-ray telescope (30-1000 keV), Soviet ART-P coded-mask telescope (2??-60?? keV), all-sky monitor WATCH (6-150 keV), and a gamma-burst detector PHEBUS . ... Since September 1994, GRANAT is in the survey mode. ... Explore pages devoted to individual GRANAT instruments (including main scientific results): . ...

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• The 6th INTEGRAL Workshop "The Obscured Universe"

. [Russian version] . M a i n p a g e . Future seminars . P a s t seminars . Seminar council . " The INTEGRAL Mission " . Dr. Christoph Winkler (Astrophysics Mission Division Research & Scientific Support Department ESA, Netherlands) . Abstract: . It will provide an overview about the spacecraft, instruments and the ground segment. Then the scientific objectives and the observing programme will be described. The current status of the mission shortly before launch and the next milestones will be described.

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• Институт космических исследований РАН (ИКИ РАН)
• INTERBALL IB_TAIL April 2000 during operation scheduling
• IB_MAG5 March 2000 during operations scheduling

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• Observing with VISTA
• VISTA ETC - Exposure Time Calculator
• VISTA - Images of Camera

. Next: A. Christou Up: C.J. Butler Previous: Phenology Contents . 3-9 August, 2004. The youngest late-type stars. High-resolution spectroscopy with the GIRAFFE (Grating Instrument for Radiation Analysis with a Fibre Fed ?chelle) ?chelle Spectrograph on the 1.9m Radcliffe Telescope at the SAAO (with D. Garc?a-Alvarez and J. Drake, Harvard).

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• Armagh Observatory
• Observing times | International Year of Astronomy in Ireland | Astronomy 2009
• Faulkes Telescope