... Instrument Status . Science Verification . ... CRIRES . ... SV observer shall submit their proposals using the Science Verification proposal template Proposers are asked to provide at least a short summary of the science goal, coordinates and magnitudes of GS and science target, a finding chart , the observing wavelength ID, as specified in appendix A of the UM and DIT, NDIT settings of science detectors as computed with the exposure time calculator (see below). ... with a 0.2 arcsec slit. ...

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• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
• ESO - Thesis Topic: High-mass Star Formation at High-Angular Resolution
• ESO - Galaxies2015

WFC3 Instrument Handbook for Cycle 24 . ... Wide Field Camera 3 Instrument Handbook for Cycle 24 > Chapter 3: Choosing the Optimum HST Instrument > 3.2 Choosing Between Instruments . ... For studies at optical wavelengths, the trade-offs to consider when deciding between WFC3/UVIS and ACS/WFC include pixel size, field of view and, to some extent, throughput. ... Because ACS/HRC could not be repaired during SM4, WFC3 offers imaging at the finest pixel scale of any HST instrument at optical wavelengths. ...

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• COS Instrument Handbook
• Marshall Perrin's Research
• Fundamental Properties of the Instrument

... Over the last decade the uninterrupted, high-resolution coverage of the Sun both from the excellent range of telescopes aboard many spacecraft and from ground-based instruments has led to a wealth of observations of small-scale dynamic events observed from the chromosphere to the transition region and corona. ... SoHO observations have further characterized many transient features, such as bi-directional jets, blinkers, coronal jets, and bright points. ...

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The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...

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• Lunar Prospector
• Arcetri Solar Physics Group: Instrumentation - IBIS
• Roba Simone Busoni

Proposal Identification No.: P2590 Date Received: 2010­Jun­01 16:38:37 Technical Page Proposal Type: Regular General Category: Pulsars Observation Category: Total Time Requested: 8 Hours Minimum Useful Time : 1 hour Proposal Title: Continued high ­resolution scintillation observations of two pulsars : B0834 +06 and B1133 +16 ABSTRACT: Understanding, characterizing, and correcting for interstellar time ...

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• http://www.naic.edu/vscience/schedule/tpfiles/StinebringtagP2590tp.pdf
• http://www.naic.edu/general/download-pdf/AOradar.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/RichardsontagR3035tp.ps

... ARC 3.5m | Instrument Summary . ... ARCES (Echelle) : the ARC Echelle spectrograph, a high resolution (R~31,500) echelle spectrograph that observes the entire wavelength range from 3200 е to 10000 in a single image on a 2048x2048 CCD. This instrument is permanently mounted at the NA1 port. ... In addition to the facility instruments, several visitor instruments have been used at the 3.5m, and some of these are available to the ARC observing community by contacting the instrument PIs: . ...

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• Astrophysical Research Consortium - Apache Point Observatory

... 4 November 1994 . orbit . ... 0.0128 . ... orbit period . ... satellite mass . 1950 kg . scientific payload mass . 550 kg . ... For more information send a mail to: info@sputnik.infospace.ru . 1997-2002 SMIS IKI RAN and SRC "PLANETA" Moscow, Russia. ...

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... 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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• Methods and instruments, general issues
• General information

... GSAOI Home . ... Science . ... Despite vast increase in our understanding of the evolutionary nature of planetary nebulae (PNe) during the last three decades, a central question remains: where is the missing mass? Theoretical evolutionary tracks predict that all stars with masses in the range 1.4-8 M Sun should become PNe. ... Clearly, much of the mass of the planetary nebula shell must remain un-ionized, and much of it may be in molecular form. ... The Magellanic Cloud PNe are ideal for this. ...

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• GSAOI Instrument Description Page
• GSAOI Gemini Pictures Page
• GSAOI Bulk Motions Science Page

Next: The Transmission Gratings Up: The Instruments Previous: The Instruments . ... A conventional cross-grid charge detector reads out the photo-induced charge cloud and the electronics determine an arrival time to 16s, and the position with a resolution of about 18 m or 0.37 arcsec. ... The Massachusetts Institute of Technology's Center for Space Research, in collaboration with Lincoln Laboratories, developed the detector system and manufactured the CCDs; Lockheed-Martin integrated the instrument. ...

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• The Instruments
• The Transmission Gratings
• AXAF-Chandra

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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• ETCs and Observations Simulation at the VLT
• Wavelength Calibration at Moderately High Resolution
• Fitting and Modeling in the ASC Data Analysis Environment

... Percent of photons detected 100 80 Silicon L-edge 100.6 eV 1,240 SX-TE/CCD-512SB SX-TE/CCD-1024SB Photon Wavelength (е) 12.4 124 1.24 60 Silicon K-edge 1.8 keV 40 20 Special Applications Application # 2: Soft X-Ray Photolithography of Semiconductors The short wavelength of soft X-rays can potentially decrease the feature sizes of circuits produced in semiconductors relative to optical methods in use now. ... Damage and Protection Exposure of the CCD surface to X-rays can eventualy damage the CCD. ...

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• Instrument Description: CASPEC
• Instrument descriptors
• Character descriptor FILTCAT

... The project assumes creation of an international space observatory - the interferometer "Earth - Space - Space" in order to perform of astronomical investigations in millimeter, submillimeter and infrared regions with extremely high sensitivity (to a few nanoJanskies units of flux density in continuum spectrum) and extremely high angular resolution (to a parts of microsecond of arc or, possibly, nanosecond). ... radio-interferometric channels of the system "Space - Space", region 0.2 - 3 mm; . ...

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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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• HYPERBOLOID Results Page
• IKI - Space Research Institute of Russian Academy of Sciences
• Optico-electronic Instruments for the Phobos-Grunt Mission

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

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• Hardware sector, archive 2004

Next: VLT First Light Up: Front Cover Previous: Participants . VLT First Light . ... Image Quality of the VLT . ... Near IR Astronomy with the ESO VLT . Introduction and Overview . Infrared instruments for the VLT . Instrument Summary . ... Performance . ... CONICA: The high resolution near-infrared camera for the ESO VLT . Introduction . Design of Imaging Optics . Analyzing Optics . Cryo-mechanical Design . ...

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• CONICA: The high resolution near-infrared camera for the ESO VLT
• No Title
• Near IR Astronomy with the ESO VLT

. XMM-Newton Science Analysis System . rgsproc (rgsproc-1.26.2) [???] . Meta Index / Home Page . Instrument . Mode . RGS . Spectroscopy . RGS . High Time Resolution . XMM-Newton SOC/SSC -- 2007-11-15

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. english || русский . Main . Location . Telescope . Instruments . Program . Science . Publications . Images . Photos . Links . The following focal instruments are currently available at the telescope: . CCD-photometer . TFOSC -- medium and low resolution spectrometer . ( The page at TUG ) . High resolution echelle-spectrometer in coude focus . High Energy Astrophysics Department 2016 IKI RAN

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... European Remote Sensing Satellite (ERS-1) was launched on 17 July 1991, and the follow mission ERS-2 (with the same sensors and an Ozone monitoring instrument added) was launched on 21 April 1995. ... ERS-2 has a fixed repeat cycle of 35 days, and follows ERS-1 tracks with one day's delay. ... Swath width is 102.5 km (telemetered), spatial resolution is about 25x25 m. The Advanced SAR (ASAR) instrument is carried by ESA's ENVISAT satellite launched on 1 March 2002. ... Swath . ... Spatial Resolution...

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• INTERBALL/ELECTRON EXPERIMENT
• Scientific tasks of GRS and HEND
• DIGITAL WDC EXCHANGE FORMAT FOR OBSERVATORY 1.0 MINUTE VALUES

... Dodson, Legge et al, ApJ, 2003 Spectral Line Sources · Requirement of high brightness temperatures means no thermal emission · Masers: Galactic Extragalactic · OH, H2O · OH, H2O, SiO, CH3OH · Galactic extra-galactic HI absorption VLBI arrays · VLBA (Very Long Baseline Array) Dedicated US array of ten 25m telescopes 330 MHz ­ 90 GHz · EVN (European VLBI Network) Formal collaboration of radio telescopes in Europe, Asia and South Africa ~15 telescopes 15m to 100m 330 MHz ­ 22/43 GHz ...

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• http://www.atnf.csiro.au/projects/askap/techdocs/JB_Fair_UV_pdf.pdf
• MAPPIT 2: Second Generation High-Resolution Imaging at the AAT
• A Chromatic Aberration