... Main page . ... Parameters . ... Modes: . ... Long-slit . ... Back to SAO web page . ... This page is designed by A.V. Moiseev . ... The SCORPIO-2 project: . Spectral Camera with Optical Reducer for Photometric and Interferometric Observations - 2 . The SCORPIO-2 main parameters . ... Spectral range . ... Spectral resolution . R=500-4000 in long-slit mode . R=4000-15000 in scanning FPI mode . The CCD detector . ... The quantum efficiency measurements for CCD detector ...

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• SCORPIO-2 project: description
• SCORPIO-2 project: filters
• SCORPIO-2 project: Fabry-Perot

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• The LongSp Description
• Determination of the Detector Parameters
• Arcetri Spectral Code related publications

... 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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Next: Head Positions and Track Up: OBSOLETE SECTIONS Previous: Mark III Observations Contents . ... Mark II recording systems have been removed from most active VLBI stations and the main Mark II correlators are no longer operating. ... Below is an example of a simple Mark II schedule. ... OBSMODE = '6cm Mark~II Standard Setup' ! ... SRCFILE = sources.obs ! ... EXAMPLE: Setup file for Mark~II observations (1 channel) at 6cm. -------------------------------------------------------------------- ! ...

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• Making a Fake Observation
• Parameters Specific to the VLA
• User Parameters - Preparation of the Science field data CentralProcessor 0.11

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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• lte-codes: sterne model atmospheres
• Refereed Journal Publications 2004
• Homepage of "Jorick Vink"

... L-Wide . ... Receiver History . ... Available Filters: . ... Use with e.g. filter 5) NOTE 2 1120-1220 3 1230-1470 4 1550-1820 5 1100-1800 6 1360-1470 7 1320 hipass NOTE 8 1180-1280 9 1280 hipass (ext Output unit. ... Consequently, the calibration for data collected using the hipass 1320 and the hipass 1370 filters only will be mis-calibrated (i.e. by using the opposite polarisation calibration data). ... It is now possible to select any bandpass filter that is not in the 1320 hipass band. ...

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• Alfacal
• GALFA System Description
• WAPP File Format Page

... They include: 4 dither patterns, 4 chop patterns, and 3 dither-chop patterns. For each of these, the observer will be able to specify, during the Phase II Proposal submission, the total number of positions desired (2 to 40), the dither size (0 to 40 arcsecs), the chop size (0 to 1800 arcsecs), and the orientation of the pattern on the sky. ... In addition, the figure number where the pattern is graphically shown is given in column 5 of Table 10.1 . ... Figure 10.3 . ... 0.0 - 1800.0 . ...

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• STSDAS release notes
• Resume for Robert E. Douglas, Jr.
• How precise are the parameters of my double star as measured in Transfer Mode?

... This tool is designed to create formatted and unformatted file-by-file reports from fits headers, or fits files. fitsreport reads from a configuration file all the keys to be displayed: . ... retrieve non-FITS information (file name, path name). ... The tool reads all fits files in the given path, evaluates the configuration file fitsreport_raw.cfg (to be in ${DFO_CONFIG_DIR}) and dumps the output into out. ... This is more evident in the other config file, fitsreport_raw.cfg. ...

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• ESO - FP7 E-ELT
• VLTI Calibrator Selection Help Page
• ESO - E-ELT Telescope Design

Next: Three-dimensional Data Analysis in IRAF and ZODIAC+ . ... A data analysis system has been developed at SRON, which has been designed to allow rigorous control of the quality of its processed data products. ... This means recording all parameters of all steps which lead to the establishment of the final data products (Figure 1 ). ... Figure: A processing pipeline is a sequence of tasks with several input/output files and parameters, which pass data from one task to the next. ...

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• A Graphical User Interface for a Development Environment (GUIDE)
• A Distributed System for ``Phase II'' Proposal Preparation
• A Computer-Based Technique for Automatic Description and Classification of

Our publications in 2000 year Kniazev, A. Y.; Pustilnik, S. A.; Masegosa, J.; Marquez, I.; Ugryumov, A. V.; Martin, J.-M.; Izotov, Y. I.; Engels, D.; Brosch, N.; Hopp, U.; Merlino, S.; Lipovetsky, V. A. Astronomy and Astrophysics, v.357, p.101-110 (05/2000) . Compressed postscript version of the paper (170Kb) . ... 07/2000) . ... Kniazev, A. Yu.; ... Kniazev A.Y. Compressed postscript version of the 1st lecture (100Kb) . Kniazev A.Y. Compressed postscript version of the 2nd lecture (350Kb) . ...

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• Session parameters
• Mean astrophysical parameters from LEDA
• Parameters

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/mosenkov.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf
• Enslish version of database

... CV & PUBLICATIONS | ... Nicholls, DC, Dopita, MA, Sutherland, RS, Jerjen, H, & Kewley, LJ " Metal-poor Dwarf Galaxies in the SIGRID Galaxy Sample. ... Nicholls DC, Jerjen, H, Dopita MA, & Basurah, H. (2014) " Nebular Metallicities in Two Isolated Local Void Dwarf Galaxies ", Astrophysical Journal 780, 88 * . ... Sweet SM, Drinkwater MJ, Meurer G, Bekki K, Dopita MA, Kilborn V, & Nicholls DC, " CHOIRS H I Galaxy Groups: The Metallicity of Dwarf Galaxies" , (2014) Astrophysical Journal , 782, 35 * . ...

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• GSAOI Instrument Description Page
• Raquel Salmeron's Publications
• GSAOI CoDR Pictures Page

... 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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• Astrophysics Group AMI Publications
• Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the
• OptInt PmWiki : Design Documentation | History

... Multicomponent order parameter and penetration depth of YBCO single crystals . Yu.A.Nefyodov, A.A.Golubov, M.R.Trunin, M.T.Beal-Monod. ... Phenomenological description of the microwave surface impedance and complex conductivity of high-T c single crystals . ... Microwave surface impedance anisotropy of YBaCuO single crystals with different oxygen content. ... Microwave surface impedance and complex conductivity of high-Tc single crystals: Current state and unsolved problems. ... Publications . ...

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NAME httpd - Apache hypertext transfer protocol server SYNOPSIS httpd [ - X ] [ - R libexecdir ] [ - d serverroot ] [ - f config ] [ - C directive ] [ - c directive ] [ - D parameter ] httpd [ - h ] [ - l ] [ - L ] [ - v ] [ - V ] [ - S ] [ - t ] [ - T ] DESCRIPTION httpd is the Apache HyperText Transfer Protocol (HTTP) server program. ... This manual page only lists the command line arguments. ... Paths in this manual may not reflect those compiled into httpd. ... The default is /usr/local/apache . ...

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... Structure of Data . ... Catalog . ... In SAI OCL Catalog, we introduce our work on investigation of the Milky Way system of open star clusters. The main goal of our study is a search for new clusters using huge surveys. 168 new clusters have been already discovered by us using J,H,Ks data from 2MASS point source catalog. ... For 141 new clusters, we found their physical parameters using J,H,Ks data from 2MASS catalog and, for a number of clusters, our UBVRI CCD observational magnitudes. ...

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• SAI OCL Catalog Structure
• SAI OCL Catalog Description
• SAI OCL Catalog Publications

Hide Zen home . ... sncat2sntab.pl - convert old catalog to table sn . ... CREATE TABLE cats ( id integer PRIMARY KEY, name text ); -- a list of properties of galaxy CREATE TABLE properties ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy _property ( gid integer REFERENCES galaxy (id), pid integer REFERENCES properties(id), value float, UNIQUE( gid ,pid) ); CREATE t=# select * from galaxy; id | ...

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• CREATE FULLTEXT CONFIGURATION
• ALTER FULLTEXT CONFIGURATION
• CREATE FULLTEXT DICTIONARY

... The Post-Reduction Off-line Software (PROS) is a portable x-ray analysis software system designed to run under NOAO's Image Reduction and Analysis Facility (IRAF). The PROS system provides IRAF users with tasks that will properly access the x-ray data. ... Similarly many IRAF tasks will be useful for x-ray data. ... The IRAF system, previous to the development of the PROS software, provided many of the features needed to analyze generic astronomical data, optical data in particular. ...

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• Topics in AstroStatistics
• The AstroStat Slog Blog Archive The Banff Challenge [Eqn]
• Model Spectra for Spectral-Fitting Program

... Samara State Aerospace University Staff Timbay Ivan Aleksandrovich . ... Belokonov I.V. , Timbai I.A. The selection of the design parameters of the aerodynamically stabilized nanosatellite of the CubeSat standard // 3rd IAA-RACTs Conference on Scientific and Technological Experiments on Automatic Space Vehicles and Small Satellites, SPEXP 2014, 9- 11 September 2014, Samara; Russian Federation, Elsevier, 2015, P. 88-96 . ... Shakhmatov E.V. , Belokonov I.V. , Timbai I.A. and others. ... 2014. ...

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• Belokonov Igor Vitalevich
• Samara University scientists designed new materials for the accumulator of the
• The complex 'Shtil-M' No. designed in SSAU began data transmission from the

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• Observing with VISTA