... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

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• MILT Description
• Astrophysical Research Consortium - Apache Point Observatory
• Observers Instructions for filling out the ARCSAT nightlog

... Observing with the major instruments at the United Kingdom Infra-Red Telescope (UKIRT) is already semi-automated by using ASCII files to configure the instruments and then sequence a series of exposures and telescope movements to acquire the data. ... Using an off-line preparation system to create these has significantly improved observing efficiency, as also has the automatic, on-line data reduction system in use by one of the main instruments. ... The Observation Sequencer. ...

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• ETCs and Observations Simulation at the VLT
• TransVERSE: An Architecture for Configuring Astronomical Observations
• Nightly Scheduling of ESO's Very Large Telescope

... HST . ... Missions . ... Data . ... Hubble Heritage Project . Future Missions and . ... HST Overview . Overview . ... Cycle 24 Announcement . ... Retrieving HST Data . ... Figure 6.1: - The Hubble Space Telescope and its components. ... Figure 6.2: - The focal plane of HST and the definitions of the V2, V3, U2, and U3 axes in the coordinate system of the spacecraft. Figure 6.3: - Locations of GHRS apertures relative to spacecraft axes. ... Figure 6.4: - Optical Schematic of the GHRS. ...

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• Pre-2003 Jitter File Description Document
• STIS Instrument Handbook
• The HST Focal Plane and the GHRS Apertures

... 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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... 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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• VLTI Calibrator Selection Help Page
• ESO - Observing conditions: definitions
• ESO - FP7 E-ELT

... Observing Control at the UKIRT A. Bridger and G. Wright Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom F. Economou Joint Astronomy Centre, 660 North Aohoku Place, University Park, Hilo, HI 96720 Abstract. ... Using an o#­line preparation system to create these has significantly improved observing e#ciency, as also has the automatic, on­line data reduction system in use by one of the main instruments. ... The Observation Sequencer. ... Observing Control at the UKIRT 295 3.3. ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/chavana.ps.gz

Radar Astronomy Group . ... This instrument will enable the Observatory to detect asteroids over a very much wider radial range than with the old 420 kilowatt system. ... Here are some recent images of asteroids obtained with the Arecibo Planetary Radar. ... The following data were taken by various observers using the Arecibo Observatory 12.6 cm radar. ... Chris De Vries wrote a description of how to reduce planetary radar data , using the 1988 Venus data taken at the Arecibo Observatory as a model. ...

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• Astronomy at Arecibo Observatory
• National Astronomy and Ionosphere Center (Arecibo Observatory)
• Arecibo Observatory Proposal Cover Sheet

... GSAOI Home . Instrument . ... The Gemini South Adaptive Optics Imager (GSAOI) is a near-infrared adaptive optics camera that will be used with the Multi-Conjugate Adaptive Optics (MCAO) system on the Gemini South 8-m telescope . ... Gemini's major instrumentation goal is to develop its Multi-Conjugate Adaptive Optics (MCAO) system for scientific use on Gemini South. ... Existing adaptive optics systems use a single natural guide star or artifical laser guide star to measure this image blur. ...

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• Software Maintenance Manual
• GSAOI Component Supplier Links Page
• GSAOI Other Links Page

Next: General CCF Components Up: Calibration Access and Data Previous: List of CAL Routines Contents . This section contains descriptions of the structure of CCF constituents. ... The calibration team of the SOC is also providing additional CCF components where required in conjunction with data that were generated with SciSim. ... These CCF components are generated on a need basis and are identical in structure to the real life components. ... Generation from Ground Calibration Data . ...

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• Description
• Exposure Record

... Облучатель 1 . ... Мингалиев М. (САО РАН) . 03-31): Исследование переменности АЯГ в широком диапазоне временных масштабовх, . ... Трушкин С.А. (САО РАН) . ... 01-31): Исследования Солнца 1 (много-азимутальные наблюдения, +- 2h от меридиана) . ... Жеканис Г.В., Призов П.В. (САО РАН) . ... Горшков А.Г. (САО РАН) . ... Берлизев И.В. (САО РАН) . ... Парийский Ю.Н. (САО РАН) . ... Призов П.В. (САО РАН) . ... САО РАН) . ... 29-31): Investigation of radio spectra and variability of GPS sources, . ...

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• SAO RAS home page
• Small telescopes short description
• Telescopes

Next: Order Definition Up: Echelle Reduction Method Previous: Retrieving demonstration and . ... That is the mapping between the space wavelength, spectral order and the space sample x , line y in the raw image. ... Sections and describe the solution of this mapping. The second step in the reduction, described in Section , is to estimate the image background. ... In the rest of this Section the algorithms used in each step of the reduction are described. ...

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• Instrument Description: CASPEC
• Introduction
• Observations and data reduction

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Upflows at the edges of active regions - called AR outflows , are studied using multi-instrument observations. ... The evolution of the photospheric magnetic field associated with the footpoints of the upflow region and the plasma properties of active region upflows are investigated aiming at providing such information for benchmarking data-driven modelling of this solar feature that is presented in Galsgaard et al. ...

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• Doppler Imaging and Flare Activity on HR1099

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Astrophysics graduate student programs . ... Facilities . ATNF facilities . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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• The instrument
• casacore: casa::MSObservationEnums Class Reference
• Pulsar Group Main/Psrfits

Modern AstroStatistics has emerged as a new field in recent times, informed by a Bayesian foundation, utilizing powerful computational tools like MCMC, and applied to diverse analysis and inference problems in Astronomy. ... The goal of our Special Session is to review current practices, highlight modern techniques, and explore how the transition into the realm of Big Data Astronomy can be facilitated. ... Big Computing in Astronomy: Perspectives and Challenges . ...

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• Harvard College Observatory History in Images
• Smithsonian Astrophysics Observatory Predoctoral Fellowships, 2004

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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• General description of the database
• Description of database

... Astrophysics Group . ... VSA . ... CAT . ... The Very Small Array is a custom-built radio telescope (operating between 26-36 GHz), designed expressly to make high resolution observations of the cosmic microwave background (CMB) radiation on angular scales around and below one degree. ... The VSA has been operated in ?compact array? and ?extended array? configurations (see the technical description below) and data collected to achieve high sensitivity in both regimes have been analysed. ... 1.75 GHz)...

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• OptInt PmWiki : Final Design Review Material
• Abstract
• VLBI observations of the quasar 3C380

. Сайт временно не работает.

18. Radioastronomy reduction procedures

19. Description of the RadioAstron project, english version

20. Meade Instruments - Telescopes, Solar Telescopes, Binoculars, Spotting Scopes