... 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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• Arecibo Observatory 610/700-MHz Band Receiver
• Arecibo Observatory: S-High Receiver
• Arecibo Observatory: S-Low Band Receiver

The Parkes 21cm Multibeam Receiver is a new facility available on the Parkes Telescope which is operated by the Australia Telescope National Facility (ATNF), CSIRO. The facility consists of a 13-beam cooled 21cm receiver system, located at the prime focus of the 64m dish. ... Completed 21cm Multibeam Receiver being hoisted up to the Parkes focus cabin. ... It is now available, in 64 MHz mode and in pulsar mode, for normal National Facility use. ... Beam 1 . Beams 2-7 . ... Frequency Range . ...

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• PmWiki | Main / Data
• PmWiki | Main / T2over
• Parameters Specific to the VLA

Modified 11 April 1999. The last modifications concerns to the new ground tracks selection on the base of the more wide list of the INSPIRE particpants. ... The range value was changed from 2 deg to 4 deg for the distance between lat/lon of the graund track and place of the INSPIRE members. Plots of predicted tracks under USA and Europe 11 April 1999 . April, 17, 1999 (USA) . April, 17, 1999 (EUR) . ... 11 April 1999 . ... place . ... Back to the IKI Satellite Situation Center (SSC) . ...

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... Apache HTTP Server Version 2.4 . ... Session encryption support . ... session_crypto_module . ... The session will be encrypted with the given key. Different servers can be configured to share sessions by ensuring the same encryption key is used on each server. ... The SessionCryptoPassphrase directive specifies the keys to be used to enable symmetrical encryption on the contents of the session before writing the session, or decrypting the contents of the session after reading the session. ...

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• mod_file_cache - Apache HTTP Server
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• mod_macro - Apache HTTP Server

... New version of magnetic field data (descriptor "itm") is now available with small corrections in offsets and attitude coverage. ... Full set of INTERBALL-TAIL AKR radiointensity KP for AKR instrument is now available (descriptor "ita"). ... KP data availability plots are created. ... Magnetic field data (descriptor "itm") after 1st January, 1998 are recomputed with corrected Bx_GSE offset (this was just 0.5 nT correction). ... CDF files for plasma wave KP are now available (descriptor "itw"). ...

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• INTERBALL-TAIL KP
• List of currently available KP AZ.
• INTERBALL-TAIL KP list

... eparam* - edit parameter files . ... Type ``<esc>-?'' within a parameter editor for more details on commands. *tupar* - Edit table headers . Table files (* .tab ) consist of a header including a variety of parameters and the table itself. It is possible to edit the header using tupar and the table with tedit provided you have write-access to the file. ... Works like emacs but uses <ctrl> D to exit. *hedit* - edit image file header . qphedit* - edit .qp file headers . ...

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• Parameters
• Converting the XPA API to 2.0
• Changes for release 1.8

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• ngasMonitor
• extractStat
• OYSTER Lab

... B.1 New functionality . ... B.3 Semantic changes from CSS1 . ... CSS2 builds on CSS1 and all valid CSS1 style sheets are valid CSS2 style sheets. The changes between the CSS1 specification (see [CSS1] ) and this specification fall into three groups: new functionality, updated descriptions of CSS1 functionality, and changes to CSS1. ... Several internationalization features, including list numbering styles , support for bidirectional text , and support for language-sensitive quotation marks . ...

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• Long description for change bar example
• Argument association
• Backward and Forward compatibility

... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...

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ALMA | ... Phase Correction Algorithms | ... On this page, we describe what the phase correction algorithms set out to do and the framework we have developed to optimally use all of the available information. ... We are developing a Bayesian framework to combine all the information we have about the current and future meterological conditions (which are naturally accommodated as priors in a Bayesian scheme) with detailed physical models of the atmosphere. ...

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• OptInt PmWiki : Design Documentation | History
• OptInt PmWiki : Preliminary Design Review | History
• OptInt PmWiki : Production Software PDR To Do List | History

Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Moscow 119992, Russia . ... 84/32, Moscow 117997, Russia . ... Our CCD observations compared to times of minima derived from the archival photographic plates and from the NSVS and ASAS-3 data clearly show that the orbital period of the system is variable. ... The phased light curve for the light elements . ... CCD, Moscow . ... and for the current linear light elements (in excellent agreement with the NSVS, ASAS, and our CCD observations): . ...

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Stellarium 0.12.3 . ... Classes . ... ClassљList . ClassљIndex . ... TuiNodeEnum Class Reference . ... setValue (QString s) . TuiNodeEnum (const QString &text, QObject *receiver, const char *method, QStringList items, QString defValue, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNodeResponse љ . ... virtual QStringљ . ... TuiNodeEditable (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ...

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• Stellarium: TuiNodeFloat Class Reference
• Stellarium: TuiNodeInt Class Reference
• Stellarium: TuiNodeColor Class Reference

... 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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• Recent changes in Earth's albedo and its implications for climate change
• Influence of Climate Variables on Tree-Ring Widths of Different Species
• SCL Sfit SYN Commands

Contact Russet McMillan (primary) or your Observing Specialists (secondary) for additional information. Contact Jack Dembicky for web page errors, corrections, ommisions, or additions. This page last updated: July 6, 2004 - JMD . This page last checked: September 14, 2003 - JMD . Configuring TUI to use the Echelle . Setting up the Echelle exposure parameters . Taking your Calibration lamps . ... Setting up multiple exposures . ... Stopping an exposure (discarding data) . ...

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• lsst.coordConv: coordConv::Coord Class Reference
• Astrophysical Research Consortium - Apache Point Observatory
• TUI:Scripts:Built In Scripts:Telescope:Pointing Data

Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...

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• ОТЧЕТ

... Description . ... The SCORPIO-2 project: . ... The multi-mode spectrograph SCORPIO-2 was developed using the experience of observations at the 6-m telescope BTA with the SCORPIO focal reducer . ... The focal reducer consists of several units ('floors') mounted in the common case in the following order (from the telescope focal plane): . ... The focal reducer is connected with the platform-adapter which used for guiding by offset stars and for illumination the spectrograph by calibration lamps. ...

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• LWN: Porting device drivers to the 2.6 kernel
• comedi_dio_config
• comedi_set_buffer_size

AUTOMATIC STATION OF ECOLOGICAL CONTROL . ... STATE OF ASEC DEVELOPMENT . ... ASEC . ... Warranted life-time of balloons and calibration mixed gases, months . ... Telemetry system supplying information from each station to ecological center on technical state of gas analyzing equipment and instruments, emergency situations and unauthorized opening of the station. available . ... Calibration mixed gasses are stored inside the balloons as part of ASEC. ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• S.P. Korolev RSC Energia - News
• S.P.Korolev RSC Energia - LAUNCHERS

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• AI SPbU library of scattering codes
• Database of Optical Properties -- Level: subpage
• Circular polarization: change of sign

... UNIX commands . C shell (csh) . ... with special meaning for shell . changing . directories . ... command line . ... command alias . command history . command interpreter . command path . command substitution . command syntax . commands . ... arguments to . ... creating . ... executing in shell scripts . ... read arguments as input to shell scripts . ... use in shell scripts . ... files . ... conditional statements See shell script . ... programs See shell scripts . ...

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• Example of changing the login shell with the chsh command
• Changing your shell
• Example of changing a password with the passwd command

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

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• Indexing and Searching Distributed Astronomical Data Archives
• The SRON-HeaD Data Analysis System
• ETCs and Observations Simulation at the VLT