... The choice of the spectrograph design (Fig.2) is determined by the quantity R, the overall dimensions of the PF cage and the restrictions on the rigidity of the structure of the device. ... As the camera's objective a fast 4-lens aplanat is used having a focal distance F cam =140 mm and a relative aperture of 1:1.8, the resolution at the centre is no less than 80 gr/mm, that over the field at a distance of 3 mm from the edge along the frame ( ) diagonal is 35 gr/mm. ...

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• Optimization of spectroscopic observations
• On the problem of high spectral resolution observations of faint objects
• The prime focus echelle spectrograph and the MSS

Next: IPCS observations and data Up: Spectral survey of Case Previous: The sample description . The observations were carried out with the 6m telescope of the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) in the period from December 1992 to October 1996. ... 1986 ]). Since January 1996 we used for registration Tektronix CCD 1024 1024 provided by Astrophysical Institute Potsdam (AIP, Germany) in the frame of mutual cooperation between AIP and SAO RAS. ...

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• SAO 6m observations
• Observations
• Calar Alto 2.2m observations

... Science . ... Science Users Information > Science and Technical Meetings > Conferences 2012 > Circumstellar Dynamics at High Resolution . ... Observing with ESO Telescopes . ... Data Handling and Products . ... If you are interested in participate in the workshop please fill out the registration form . ... The workshop will take place in Foz do Iguaц§u, Brazil, close to the magnificent Iguaц§u Waterfalls, a network of 275 waterfalls in the Iguaц§u River that lies in the border of Brazil and...

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• ESO - 8th VLTI Summer School: High angular resolution in astrophysics: optical
• ESO - Galaxies2015
• ESO - Newsletter May 2014

... Telescopes . ... 1996: . According to the interferometric observations at 6-m telescope with the panoramic infrared detector NICMOS-3, for the first time in the world the angular diameters of the mirid stars R Cas and R Leo were measured at the wavelengths between 1045nm and 2170nm. ... A study of fluctuations of the galactic gas emission at high latitudes within the "Cold" survey band with high sensitivity was made with the RATAN-600 radio telescope. ... Archive . ...

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• RCJ0311+0507
• Hardware sector, archive 2009
• SAO RAS home page

COS Instrument Handbook for Cycle 24 . ... Cosmic Origins SpectrographInstrument Handbook for Cycle 24 > Chapter 2: Special Considerations for Cycle 24 > 2.2 COS Observations Below 1150 е: Resolution and Wavelength Calibration Issues . ... COS Observations Below 1150 е: Resolution and Wavelength Calibration Issues . ... In such cases, for each CENWAVE and FP-POS position, a separate GO-wavecal exposure should be taken with Segment A ?on? immediately adjacent to the Segment B science observations. ...

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• Limitations on the Calibration Accuracy for COS/FUV Observations of Extended
• Calibration of COS Observations of Extended Targets in Cycle 24
• HDF-S Data Products

Subject, Object and Problems of Astrophysics. Practical and Theoretical Astrophysics. ... Visual Telescope; Problems Which Are Solved with the Its Help. ... Resolution of Telescopes. ... Effectiveness of Telescope in Respect of Resolution. ... Optical Power of Telescopes for Star-like and Extensive Objects. Boundary Magnitude. Reasons of Light Dissipation in Telescopes. ... Spectral Instruments in Astrophysics. ... Basic Photometrical Ideas, Magnitudes and Their Measurement. ...

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• Optical static Fourier spectrometer
• Solar Physics

Next: Pulsar bin-mode observations Up: ATCA Bin Mode Observations Previous: ATCA Correlator Bin Modes . Miriad 's atlod task has an option, options=hires which converts a RPFITS file observed in high time resolution bin-mode into an apparently normal dataset with fine time resolution. ... In high resolution time mode, the time difference between consecutive integrations might be smaller than this tolerance. ... Miriad manager . ...

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• immerge
• Pulsar bin-mode observations
• Archive of VLBI Observations Majordomo List

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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... REGISTRATION . ... 119991, Leninski prospekt 53, Moscow, Russia . ... The sun from radio to gamma rays new results from space and ground based observatories . ... Solar observations with high temporal and spatial resolution new look from SDO and Hi-C . ... Towards the sun: InterHelioProbe, Solar Orbiter, Solar-C . ... The sun as a star: solar cycle and space weather . ... Novbember 5, 2013 . Deadline for letter of invitation request . ... Publication of the workshop's program . ...

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• TESIS
• Moscow workshop: The Sun from quiet to active 2011
• TESIS - Telescopes for EUV Spectral Imaging of the Sun

... We will consider the rms, (K), for observations with a receiver of system temperature, T , frequency resolution, per polarization, and total integration time per observing cycle, . ... For ``in-band'' frequency switching, the line under investigation is always in the observing band. ... Position Switching or ``Out-of-Band'' Frequency Switching: Here the line is only observed for one half of the time, with noise being present all of the time. ...

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• Arecibo Observatory observations of 2005 YU55
• Seventh NAIC/NRAO Single Dish Summer School

... Aloisi, A. The Old Stellar Population . Alonso-Herrero, A. HST /NICMOS Observations of the . ... Balcells, M. HST-NICMOS Observations of Galactic . ... Baum, S.A. Investigating the Evolution of . ... Becklin, E.E. A Coronagraphic Search for . ... Clampin, M. The Old Stellar Population . ... Close, L. HST NICMOS Observations of . ... The Stellar Population in . Geballe, T.R. HST NICMOS Observations of . ... Greggio, L. The Old Stellar Population . ... Leitherer, C. The Old Stellar Population . ...

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• No Title
• NICMOS Data Calibration and Analysis
• NICMOS and the VLT: A New Era of High Resolution Near Infrared Imaging and

... Green and blue curves - CYGAM telescope (squares - no constraints on the angle a , triangles - a <0.5 0 ); red curve - EGRET telescope. Effective area versus photon incidence angle to relative the longitudinal telescope axis (squares - no constraints on the angle a , triangles - a <0.5 0 , spectral index g= 2). ... Angular resolution for normal to the axis X incidence versus source power law spectrum index (squares- no constraints on the angle a , triangles- a <0,5 0 ). ... CYGAM (PDF, 450 Kb) . ...

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• High resolution IR-spectrometer
• OFO IKI / Registration
• Two points (INTERBALL-1 and MAGION-4) observations of magnetopause motion

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• Arcetri Solar Physics Group: High Resolution Studies
• AO on AR 8970
• serplines (Abstract)

grdlandmask - Create "wet-dry" mask grdfile from shoreline data base. grdlandmask -G mask _ grd _ file ] -I xinc [ m|c ][/ yinc [ m|c ]] -R west / east / south / north [ r ] [ -A min _ area [/ min _ level / max _ level ] ] [ -D resolution ] [ -F ] [ -N maskvalues [ o ] ] [ -V ] grdlandmask reads the selected shoreline database and uses that information to decide which nodes in the specified grid are over land or over water. ... The resolution drops off by ~80% between data sets. Default is l ]. ...

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• Science with CXO

THE NAUTICAL ASTRONOMICAL ALMANAC (in Russian-English) . NAA-2 provides an easy access to useful navigational publications aboard a ship. ... In conformity with the STCW95 Code provisions, every watch officer, chief mate and master should be able to use classic methods of nautical astronomy, so they will surely appreciate the new ?Nautical astronomical almanac? available. ... Ph.D. M.L. Sveshnikov (editor-in-chief), . ... Ph.D. N.I. Glebova , . ... THE NAUTICAL ASTRONOMICAL ALMANAC . ...

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• AY2008 (preface)
• AY2007 (preface)
• AY2011 (preface)

... The motivation for this task is to create one high resolution response matrix for a set of observations without the need for creating individual high resolution matrices. ... This task creates a single response matrix file using information from a list of spectrum from multiple observations, and can also combine spectra and background spectra of the same instrument and spectral order to produce final files that can be used for futher, quantitative analysis in a fitting package such as Xspec. ...

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• SciSim simulation of Abell 2199 X-ray spectrum
• Functionality

... No flares were detected during the 3.5 hours of monitoring. ... The resultant spectrum was of sufficient quality to allow the detection of emission lines with an integrated flux of 10$^{-15}$ erg cm$^{-2}$ s$^{-1}$ or greater. Lines of C I, O I, O V, Cl I and Fe XXXI were detected. ... From the upper limit on the observed line width, we derive an upper limit of 38 km s$^{-1}$ for the turbulent velocity in the 10$^{7}$ K plasma. ...

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• Armagh Observatory
• Explosive Events
• An Overview of the Coupled Earth-Sun System PPARC Introductory Solar System

... Using multifrequency radio data obtained with the GMRT, VLA and RT, we are defining a sample of young radio AGN in the Spitzer FLS field which are associated with midinfrared sources. ... GMRT Observations The Spitzer extragalactic First Look Survey (FLS) field was observed with the Giant Metrewave Radio Telescope (GMRT, Figure 1), Pune, India, at 610 MHz in March 2004. ... Figure 1: Three of the antennas in the inner square kilometre of the Giant Metrewave Radio Telescope (GMRT). ...

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• http://www.mrao.cam.ac.uk/~bn204/phd_era/publications/kiel.pdf
• LOFAR MKSP Workshop
• VLBI observations of the quasar 3C380

... In order to overcome undersampling, two or more frames of the same field may be obtained which are shifted with respect to each other by fractions of a pixel. ... Obviously science programs such as photometry of dense star fields and the morphological classification of distant galaxies would benefit from a method allowing a proper combination of two or more ``dithered'' WFPC-2 frames, i.e., frames that are shifted with respect to each other by fractions of a pixel. ...

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• The ISO Post-Mission Archive
• Indexing and Searching Distributed Astronomical Data Archives
• ADASS 2003 Conference Proceedings

... Galaxy Evolution Explorer (GALEX) . ... Searching for SZ clusters . ... Baryon content of galaxy clusters and cosmology . ... 3 sigma peaks: Observational Signatures of High Redshift Galaxies and Low Redshift Clusters . CLUSTERS OF GALAXIES . ... Clusters of galaxies seen in X-rays: war and peace . ... Chandra X-ray Observations of Clusters/Groups/Galaxies . ... Common timing features in neutron stars and black holes . ... X-ray luminosity function of low-mass X-ray binaries in galaxies . ...

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• Spectrum-Roentgen-Gamma - The astrophysical Project at IKI RAN
• SIXA acceptance tests, 2000
• RTT150 project data archive