... HST . ... Data . ... HST Overview . Overview . ... Instruments . ... Instrument Handbook . COS Data Handbook . ... For more information about the use of this FP-POS option see Section 5.8.2 of the COS Instrument Handbook. ... COS has the advantage of a fairly large aperture so that there are only small aperture losses ( see Section 5.1.9 of the COS IHB). ... The available spectroscopic resolving powers (R) available to observers with COS are listed in Table 5.1 of the COS Instrument Handbook. ...

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• Time resolved observations with STIS/MAMA (TIME-TAG mode)
• FUV-MAMA Repeller Off as an Available Mode for High Resolution Spectroscopy
• Proposing Overview

... The technology needed to implement a Distributed Astronomical Data Archive (DADA) is available today (e.g., Fullton 1993). Query interface standards are needed, however, before the DADA information will be discoverable. ... These parameters would be used to index each dataset in each catalog. ... The technology is available today to perform cross-catalog queries, to fetch the data at the click of a mouse, quickly to add new observation catalogs, and to distribute the load across multiple machines. ...

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• Space Science Education Resource Directory
• PICsIM - the INTEGRAL/IBIS/PICsIT Observation Simulation Tool for Prototype
• Towards a General Definition for Spectroscopic Resolution

... December 21, 1997 . ... Advantages are briefly discussed of gaining in spectral resolution, which is accompanied by losses in signal level, as compared with the attempts to improve the accuracy of measurement of line parameters by means of rising the S/N ratio alone with increasing the exposure time. To partially solve the problem of observations of faint objects at the BTA a new design echelle spectrometer is proposed. high resolution spectroscopy . ...

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• Optimization of spectroscopic observations
• Directory handling functions

XMM-Newton Science Analysis System Page: 1 omslewchain August 16, 2005 Abstract Chain script used to run slew pipeline tasks 1 Instruments/Modes 2 Use pipeline processing /no interactive analysis /no 3 Description This package contains a PERL script which takes a set of image mode OM SDF les in a single directory and processes them in a pipeline to produce OM image mode pipeline products see Fig. ... Refer to the index of all errors and warnings available in the HTML version of the SAS documentation. ...

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• Algorithm
• Analysis options
• Description

... Science Publications > Science Announcements > 8th VLTI Summer School: High angular resolution in astrophysics: optical interferometry from theory to observations . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... Optical/infrared long-baseline interferometry has reached a new stage with the advent of multi-telescope arrays accessible to a broad community of astronomers, most notably VLTI . ...

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• ESO - Science Announcements
• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
• ESO - Improvement to FLAMES Spectral Resolution and Sensitivity

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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• delaysolver CentralProcessor 0.11 documentation
• New HI Observations of the Prototype Polar Ring Galaxy NGC 4650A
• Archive of VLBI Observations Majordomo List

... The NVSS is being made as a service to the astronomical community, and the principal data products are being released into a directory accessible by anonymous FTP as soon as they are produced and verified. ... The large (4 deg x 4 deg) map cubes and total intensity only images and their associated multisource (u,v) data sets are stored as binary files in FITS format (see Grosbol et al. ... The source catalog derived from the available images is kept in directory CATALOG as CATALOG.FIT. ...

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• SSL/TLS Strong Encryption: How-To - Apache HTTP Server
• Per-user web directories - Apache HTTP Server
• Observations and Analysis

... In this directory we give the files containing the continuous U-band data, namely m01-yy.dat, m03-yy.dat, m04-yy.dat, m05-yy.dat and m06-yy.dat. The 01, 03 etc in the filename refers to the local (Hawaii) date of the start of the night, in fact its the night of 1/2, 3/4 March etc, which corresponds to the UT date 2, 4 etc. ... The corrected U-band monitoring is contained in the file yy-fl-cU.dat in the form heliocentric Julian date (HJD-2447000.0) and U-band magnitude. ...

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• Armagh Observatory
• C.J. Butler, Research Astronomer
• The /etc directory

... At SAO, the ROSAT data for observation rp123456 will be in /data/rdata/godata/rp123456/ . The PROS package contains sample ROSAT and Einstein data which are in the directory /pros/xray/data which is loaded with the IRAF task ``xray''. ... Thus within an arbitrary working directory and within the IRAF environment, to look at an image the command is, tv> display "xdata$rp110590_im2" 1 If Einstein data are loaded at SAO they will appear in the directory /pool14/i1234/ . ...

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• An example of a typical timing analysis
• Intern Directory
• *qpspec* - Time Resolved Spectral Fitting

... 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
• Footnotes

Solar High Resolution Studies . ... Solar Group . ... High quality observations obtained in recent years have highlighted the fact that the solar atmosphere is extremely dynamic, and wholly permeated and shaped by magnetic fields at very small spatial scales. ... The Solar Group in Arcetri is initiating a project to study some of the topics and techniques that will be brought to the forefront of solar physics as this new physical regime is explored. ... Small Scale Activity . ...

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• Per-user web directories - Apache HTTP Server
• CQTau disks (Abstract)
• High Resolution Observations of Hot Molecular Cores

... There are result from two global VLBI observations at 3.6 cm spaced about 2 years. ... The analysis of the apparent motion, indication of the jet flow trajectory and the other implications for the CSS quasars are discussed. ... The quasar 3C380 ( ; thus 1 arcsec corresponds to 4 kpc for , ) is one of the most powerful radio sources (its radio luminosity at 2.7 GHz is ) ( Wilkinson et al. ... 3C380 is a member of the class of Compact Steep Spectrum (CSS) sources. ...

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• OptInt PmWiki : PmWiki / File Permissions
• OptInt PmWiki : PmWiki / Initial Setup Tasks
• Download building of the radiospec package Bojan Nikolic web pages (r. 329)

... 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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• Large telescopes application form
• Comet C/2014 Q2 (Lovejoy) and asteroid 357439 2004 BL86
• RCJ0311+0507

... Position Switching Separation Tolerance with Arecibo in L-Band . ... Using the ALFA Receiver for OH Observations . ... Carl Heiles . ... C. Salter and T. Ghosh . ... 2001-05.pdf . ... Multi-Beam Array System Feed Selection . ... Main Beam and First Sidelobe Parameters for Arecibo's Receiver Systems . ... The LBW Feed: Polarized Sidelobes outside the Main Beam . ... The LBW Feed: The Mueller matrix in 1999 and 2000 . ... The LBW Feed: Pointing Accuracy, Beamwidth, Beam Squint, Beam Squash . ...

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• ATOMS by Number
• Data and Analysis
• OLD ANALYZ instruction sequences HI in galaxies

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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• Practical Astrophysics

Netscape 1.12 (X11) ============================================================================== *********************************************** IMPORTANT! ... Security Fix Description ============================================================================== TECHNICAL BACKGROUND Netscape Navigator uses random information to generate session encryption keys of either 40 or 128 bits in length. ... SunOS 4.1, Linux, and BSDI: These distributions also includes a directory called "nls". ...

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• http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/numana03.txt
• http://crydee.sai.msu.ru/ftproot/pub/comp/hardware/matrox/doc/win95faq.doc
• crydee.sai.msu.ru archive : Directory tree

... Previous: Ground Tracking Station (GTS) Products . ... GRT Log File . ... GRT Gain Curves . ... What: Co-observing GRTs will each generate a log file identical to those for ground-based VLBI experiments. ... Where: Files are placed by GRTs on their regional server ( Regional Servers for GRT logs etc ) in the sub-directory named for the month and year (e.g. may97 ) below the sub-directory named gps . ... Where: Files are placed by GRTs on their regional server ( Regional Servers for GRT logs etc ). ...

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• Appendix B: Map of the Document
• RadioAstron Announcement of Opportunity - 1, english version
• Help for xxx E-Print Archive (index)

The close position of main satellite and subsatellite (distance between them about 1000 km) and using the similar sets of Faraday cups (VDP and VDP-S) with high resolution measurements (up to 16 Hz for the main satellite and up to 10 Hz for the subsatellite) allow us to determine the small-scale variations of the magnetopause shape and position and to estimate the velocity of the magnetopause motion. ... Two point observation of the magnetopause motion: the INTERBALL project. ...

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• Main research and development work completed in 2009 and ready for
• Optico-electronic Instruments for the Phobos-Grunt Mission
• Two-Polarization Radar

The IAA RAS . ... View details . ... Observatories 'Svetloe' and 'Zelenchukskaya' participate in frequent VLBI-observation sessions organized by the International VLBI Service for Geodesy and Astrometry . ... As part of collaboration with the U. S. Naval observatory in the areas of EOP determination and analysis the USNO uses IAA RAS daily EOP data obtained from SLR and VLBI. ... The IAA RAS and the Centre National d'Etudes Spatiales carry out joint DORIS observations on the Badary observatory. ...

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• Software
• Institute of Applied Astronomy Russian Academy of Sciences.
• AY2007 (preface)

On the multifunctional orbital piloted complex Mir Russian Federation Government resolves: . To accept Russian Space Agency and Korolev Rocket- Space Corporation Energy's proposal to continue the exploitation of the multifunctional orbital piloted complex Mir (further - complex Mir) in 1999-2002. ... Russian Space Agency is to provide coordination and checking over carrying out the work determined by this Resolution. Russian Federation Government . ...

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